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    <title>Recent cee_ucla_oapdeposits items</title>
    <link>https://escholarship.org/uc/cee_ucla_oapdeposits/rss</link>
    <description>Recent eScholarship items from Open Access Policy Deposits</description>
    <pubDate>Thu, 18 Jun 2026 20:23:19 +0000</pubDate>
    <item>
      <title>Ground Motion Intensity Measures at Liquefaction Field Case History Sites</title>
      <link>https://escholarship.org/uc/item/6mb9x17b</link>
      <description>Ground Motion Intensity Measures at Liquefaction Field Case History Sites</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/6mb9x17b</guid>
      <pubDate>Fri, 12 Jun 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Pretell, Renmin</name>
      </author>
      <author>
        <name>Brandenberg, Scott J</name>
      </author>
      <author>
        <name>Stewart, Jonathan P</name>
        <uri>https://orcid.org/0000-0003-3602-3629</uri>
      </author>
    </item>
    <item>
      <title>Charging ahead unfairly: An examination of temporal Shifts in electric vehicle supply equipment accessibility across California's communities</title>
      <link>https://escholarship.org/uc/item/100481pv</link>
      <description>Charging ahead unfairly: An examination of temporal Shifts in electric vehicle supply equipment accessibility across California's communities</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/100481pv</guid>
      <pubDate>Fri, 22 May 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Kuai, Chenchen</name>
      </author>
      <author>
        <name>Mugodzeri, Daisy</name>
      </author>
      <author>
        <name>Bills, Tierra S</name>
      </author>
    </item>
    <item>
      <title>Response to “Comment on ‘State-of-the-Science Data and Methods Need to Guide Place-Based Efforts to Reduce Air Pollution Inequity’”</title>
      <link>https://escholarship.org/uc/item/9gp7v7qj</link>
      <description>Response to “Comment on ‘State-of-the-Science Data and Methods Need to Guide Place-Based Efforts to Reduce Air Pollution Inequity’”</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/9gp7v7qj</guid>
      <pubDate>Wed, 22 Apr 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Gohlke, Julia M</name>
      </author>
      <author>
        <name>Harris, Maria H</name>
      </author>
      <author>
        <name>Roy, Ananya</name>
      </author>
      <author>
        <name>Thompson, Tammy M</name>
      </author>
      <author>
        <name>DePaola, Mindi</name>
      </author>
      <author>
        <name>Alvarez, Ramón A</name>
      </author>
      <author>
        <name>Anenberg, Susan C</name>
      </author>
      <author>
        <name>Apte, Joshua S</name>
      </author>
      <author>
        <name>Demetillo, Mary Angelique G</name>
      </author>
      <author>
        <name>Dressel, Isabella M</name>
      </author>
      <author>
        <name>Kerr, Gaige H</name>
      </author>
      <author>
        <name>Marshall, Julian D</name>
      </author>
      <author>
        <name>Nowlan, Aileen E</name>
      </author>
      <author>
        <name>Patterson, Regan F</name>
      </author>
      <author>
        <name>Pusede, Sally E</name>
      </author>
      <author>
        <name>Southerland, Veronica A</name>
      </author>
      <author>
        <name>Vogel, Sarah A</name>
      </author>
    </item>
    <item>
      <title>Panel Review of the USGS 2025 Puerto Rico and U.S. Virgin Islands Time-Independent Earthquake Rupture Forecast</title>
      <link>https://escholarship.org/uc/item/66009373</link>
      <description>In August 2024, the National Seismic Hazard Model (NSHM) Steering Committee appointed a 14-member panel (herein referred to as “The Panel” or “Panel”) to review the time-independent earthquake rupture forecast (ERF) for the 2025 update of the Puerto Rico and U.S. Virgin Islands (PRVI) component of the NSHM (herein referred to as “PRVI25-ERF”). This report summarizes the Panel’s findings and recommendations. The primary materials for Panel review were nine papers documenting the PRVI25-ERF draft model. The Panel was also informed about the process to update the ERF in three briefings by the
U.S. Geological Survey (USGS) development team (herein referred to as the “USGS Team” or “Team”).

The PRVI25-ERF model is a substantial improvement over the current model, which was released in 2003 (PRVI03-ERF; Mueller et al., 2003, 2010). The USGS Team has incorporated substantial new information obtained about the region and its tectonic environment over the past twenty years, and they have...</description>
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      <pubDate>Wed, 22 Apr 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Jordan, Thomas H</name>
      </author>
      <author>
        <name>Abrahamson, Norman A</name>
      </author>
      <author>
        <name>Anderson, John G</name>
      </author>
      <author>
        <name>DeShon, Heather R</name>
      </author>
      <author>
        <name>Harris, Ruth</name>
      </author>
      <author>
        <name>Hough, Susan</name>
      </author>
      <author>
        <name>LaForge, Roland</name>
      </author>
      <author>
        <name>Makdisi, Andrew</name>
      </author>
      <author>
        <name>Marzocchi, Warner</name>
      </author>
      <author>
        <name>Toro, Gabe</name>
      </author>
      <author>
        <name>Velasquez, Jessica</name>
      </author>
      <author>
        <name>Lopez Venegas, Alberto M</name>
      </author>
      <author>
        <name>von Hillebrandt-Andrade, Christa</name>
      </author>
      <author>
        <name>Wong, Ivan</name>
      </author>
    </item>
    <item>
      <title>Assessing Transportation Barriers to Maternal Care for Black Women in Los Angeles County</title>
      <link>https://escholarship.org/uc/item/2488h0fg</link>
      <description>The United States ranks among the worst high-income countries for maternal health outcomes, with Black women experiencing disproportionately high and alarming rates of maternal mortality and morbidity. In Los Angeles County, Black women are four times more likely to die from pregnancy-related causes than women of other racial and ethnic groups. These disparities may partially be attributed to social determinants of health, including transportation access. Lack of transportation can hinder access to healthcare, with significant consequences for reproductive health. This study investigates how transportation barriers affect Black birthing people's access to maternal healthcare in Los Angeles. In partnership with Black Women for Wellness, we conducted a descriptive, observational study using an online survey completed by 235 respondents, all of whom self-identified as women. Findings reveal that Black women in Los Angeles face substantial transportation barriers when seeking maternal...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/2488h0fg</guid>
      <pubDate>Wed, 22 Apr 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Usigbe, Rebecca O</name>
      </author>
      <author>
        <name>Ibrahim-Watkins, Zanobia R</name>
      </author>
      <author>
        <name>Williams, Astrid</name>
      </author>
      <author>
        <name>Wilson, Sylvie</name>
      </author>
      <author>
        <name>Cunliffe, Zoe</name>
      </author>
      <author>
        <name>Brown, Gabrielle</name>
      </author>
      <author>
        <name>Shaw-Wakeman, Tianna</name>
      </author>
      <author>
        <name>Patterson, Regan F</name>
      </author>
    </item>
    <item>
      <title>Review of the 2025 Puerto Rico and Virgin Islands National Seismic Hazard Model</title>
      <link>https://escholarship.org/uc/item/0gc9d0d3</link>
      <description>The National Seismic Hazard Model Program Steering Committee (NSHM-SC) conducts participatory peer-review during the development of NSHM products, working with the NSHM development team in the U.S. Geological Survey (USGS). This report documents the review processes and outcomes related to the development of NSHM products for application to Puerto Rico and the Virgin Islands (PRVI). The committee consists of nine members who were selected by the USGS, based on expertise and experience. 

The USGS requested a written report from the NSHM-SC answering the following questions relevant to publication of the 2023 NSHM for PRVI:

•	Was the National Seismic Hazard Model adequately reviewed?
•	Did the USGS respond appropriately to the review comments and recommendations? 
•	Is the model suitable for release and to serve as the basis for hazard mitigation?

The SC responses to the three main questions are:

Was the National Seismic Hazard Model adequately reviewed?

The NSHM-SC, and earthquake...</description>
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      <pubDate>Wed, 22 Apr 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Stewart, Jonathan P</name>
        <uri>https://orcid.org/0000-0003-3602-3629</uri>
      </author>
      <author>
        <name>Atkinson, Gail M</name>
      </author>
      <author>
        <name>Baker, Jack W</name>
      </author>
      <author>
        <name>DeShon, Heather R</name>
      </author>
      <author>
        <name>Gregor, Nick</name>
      </author>
      <author>
        <name>Jordan, Thomas H</name>
      </author>
      <author>
        <name>Kelson, Keith I</name>
      </author>
      <author>
        <name>Maffei, Janiele</name>
      </author>
      <author>
        <name>Wong, Ivan</name>
      </author>
    </item>
    <item>
      <title>Earthquake Loss Estimates and Policy Implications for Nonductile Concrete Buildings in Los Angeles</title>
      <link>https://escholarship.org/uc/item/57z8k7pq</link>
      <description>The collapse potential of nonductile concrete buildings represents a substantial life safety hazard globally that can be mitigated through carefully crafted policy. Mitigation policy should be approached incrementally by (1) understanding problem scale, (2) screening for low‐ and high‐risk buildings, (3) performing engineering analysis for potentially vulnerable buildings, and (4) retrofit or replacement of high‐risk structures. This research addresses initial stages of this sequence for Los Angeles, California. The intent was to investigate approaches for informing mitigation priorities by: characterizing the inventory of approximately 1,500 pre‐1976 concrete buildings; estimating risk, including identification of building types that contribute most substantially to the risk; and investigating the impact of retrofit policy alternatives. Loss estimates for scenario events are based on the HAZUS™ Advanced Engineering Building Module. Depending on model assumptions, losses range...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/57z8k7pq</guid>
      <pubDate>Mon, 13 Apr 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Anagnos, Thalia</name>
      </author>
      <author>
        <name>Comerio, Mary C</name>
        <uri>https://orcid.org/0009-0004-5732-0213</uri>
      </author>
      <author>
        <name>Stewart, Jonathan P</name>
        <uri>https://orcid.org/0000-0003-3602-3629</uri>
      </author>
    </item>
    <item>
      <title>Deep Ensemble Learning for Rapid Large-Scale Postearthquake Damage Assessment: Application to Satellite Images from the 2023 Türkiye Earthquakes</title>
      <link>https://escholarship.org/uc/item/2991h059</link>
      <description>Extensive field reconnaissance damage surveys, publicly available after the Türkiye earthquake sequence of 2023, provided a unique opportunity to devise and validate a rapid postevent damage assessment framework that uses Artificial Intelligence (AI) techniques to overcome typical challenges encountered in rapid regional damage assessment efforts. By analyzing publicly available satellite images of the significantly impacted city of Antakya, we manually identified and segmented fully or partially collapsed buildings and buildings with visible damage. These were then paired with the various damage state labels in the government data. An AI-based framework was subsequently developed to automate segmentation and damage assessment processes, delivering damage state estimates for other affected regions. The resulting tool, dubbed rapid postearthquake aerial imagery damage assessment (RAPID-A), is an ensemble of various deep segmentation models that work on satellite image channels...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/2991h059</guid>
      <pubDate>Wed, 8 Apr 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Soleimani-Babakamali, Mohammad Hesam</name>
      </author>
      <author>
        <name>Askari, Mohammad</name>
        <uri>https://orcid.org/0009-0002-4136-8947</uri>
      </author>
      <author>
        <name>Heravi, Mohammad Ali</name>
      </author>
      <author>
        <name>Sisman, Rafet</name>
      </author>
      <author>
        <name>Attarchian, Nahid</name>
      </author>
      <author>
        <name>Askan, Aysegul</name>
      </author>
      <author>
        <name>Soleimani, Rojiar</name>
      </author>
      <author>
        <name>Taciroglu, Ertugrul</name>
        <uri>https://orcid.org/0000-0001-9618-1210</uri>
      </author>
    </item>
    <item>
      <title>Resilient high-temperature reverse osmosis desalination membranes</title>
      <link>https://escholarship.org/uc/item/4fj8p215</link>
      <description>Conventional thin-film composite (TFC) reverse osmosis (RO) membranes experience irreversible performance loss at high temperatures, restricting their use in industries with high-temperature streams, including oil and gas, pharmaceuticals, electronics, power generation, food production, and hybrid desalination plants. However, the mechanisms driving the performance decline of TFC membranes at high temperatures remain poorly understood. Herein, we combine controlled experiments, molecular dynamics simulations, and micromechanical modeling to elucidate TFC failure mechanisms and to evaluate thermally resilient thin-film cross-linked (TFX) composite membrane. Upon exposure to elevated temperatures (&amp;gt;60°C), salt rejection of TFC dropped from ~99 to &amp;lt;90%, with irreversible structural damage in the polysulfone layer, confirmed by scanning electron microscopy. In contrast, the TFX membrane maintained ~99% salt rejection and showed no signs of physical degradation up to 80°C. Our...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/4fj8p215</guid>
      <pubDate>Fri, 27 Mar 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Wu, Jishan</name>
      </author>
      <author>
        <name>Xiao, Minhao</name>
      </author>
      <author>
        <name>He, Jinlong</name>
      </author>
      <author>
        <name>Tang, Rachel</name>
      </author>
      <author>
        <name>Soares, Katie</name>
      </author>
      <author>
        <name>Hou, Ziwei</name>
      </author>
      <author>
        <name>Wang, Xinyi</name>
      </author>
      <author>
        <name>Jassby, David</name>
      </author>
      <author>
        <name>Elimelech, Menachem</name>
      </author>
      <author>
        <name>Hoek, Eric MV</name>
        <uri>https://orcid.org/0000-0002-9674-1916</uri>
      </author>
    </item>
    <item>
      <title>Early Results from GLASS-JWST. I: Confirmation of Lensed z ≥ 7 Lyman-break Galaxies behind the Abell 2744 Cluster with NIRISS</title>
      <link>https://escholarship.org/uc/item/8rj1j94d</link>
      <description>We present the first search for z ≥ 7, continuum-confirmed Lyman break sources with NIRISS/WFS spectroscopy over the Abell 2744 Frontier Fields cluster, as part of the GLASS-JWST-ERS survey. With ∼15 hr of preimaging and multiangle grism exposures in the F115W, F150W, and F200W filters, we describe the general data handling (i.e., reduction, cleaning, modeling, and extraction processes) and analysis for the GLASS-JWST survey. We showcase the power of JWST to peer deep into reionization, when most intergalactic hydrogen is neutral, by confirming two galaxies at z = 8.04 ± 0.15 and z = 7.90 ± 0.13 by means of their Lyman breaks. Fainter continuum spectra are observed in both the F150W and F200W bands, indicative of blue (−1.69 and −1.33) UV slopes and moderately bright absolute magnitudes (−20.37 and −19.68 mag). We do not detect strong Lyα in either galaxy, but do observe tentative (∼2.7–3.8σ) He ii λ1640 Å, O iii]λλ1661,1666 Å, and N iii]λλ1747,1749 Å line emission in one, suggestive...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/8rj1j94d</guid>
      <pubDate>Wed, 11 Mar 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Roberts-Borsani, Guido</name>
      </author>
      <author>
        <name>Morishita, Takahiro</name>
      </author>
      <author>
        <name>Treu, Tommaso</name>
        <uri>https://orcid.org/0000-0002-8460-0390</uri>
      </author>
      <author>
        <name>Brammer, Gabriel</name>
      </author>
      <author>
        <name>Strait, Victoria</name>
      </author>
      <author>
        <name>Wang, Xin</name>
        <uri>https://orcid.org/0009-0006-8812-5175</uri>
      </author>
      <author>
        <name>Bradac, Marusa</name>
        <uri>https://orcid.org/0000-0001-5984-0395</uri>
      </author>
      <author>
        <name>Acebron, Ana</name>
      </author>
      <author>
        <name>Bergamini, Pietro</name>
      </author>
      <author>
        <name>Boyett, Kristan</name>
      </author>
      <author>
        <name>Calabró, Antonello</name>
      </author>
      <author>
        <name>Castellano, Marco</name>
      </author>
      <author>
        <name>Fontana, Adriano</name>
      </author>
      <author>
        <name>Glazebrook, Karl</name>
      </author>
      <author>
        <name>Grillo, Claudio</name>
      </author>
      <author>
        <name>Henry, Alaina</name>
      </author>
      <author>
        <name>Jones, Tucker</name>
        <uri>https://orcid.org/0000-0001-5860-3419</uri>
      </author>
      <author>
        <name>Malkan, Matthew</name>
        <uri>https://orcid.org/0000-0001-6919-1237</uri>
      </author>
      <author>
        <name>Marchesini, Danilo</name>
      </author>
      <author>
        <name>Mascia, Sara</name>
      </author>
      <author>
        <name>Mason, Charlotte</name>
      </author>
      <author>
        <name>Mercurio, Amata</name>
      </author>
      <author>
        <name>Merlin, Emiliano</name>
      </author>
      <author>
        <name>Nanayakkara, Themiya</name>
      </author>
      <author>
        <name>Pentericci, Laura</name>
      </author>
      <author>
        <name>Rosati, Piero</name>
      </author>
      <author>
        <name>Santini, Paola</name>
      </author>
      <author>
        <name>Scarlata, Claudia</name>
      </author>
      <author>
        <name>Trenti, Michele</name>
      </author>
      <author>
        <name>Vanzella, Eros</name>
      </author>
      <author>
        <name>Vulcani, Benedetta</name>
      </author>
      <author>
        <name>Willott, Chris</name>
      </author>
    </item>
    <item>
      <title>The nature of an ultra-faint galaxy in the cosmic dark ages seen with JWST</title>
      <link>https://escholarship.org/uc/item/823315h2</link>
      <description>In the first billion years after the Big Bang, sources of ultraviolet (UV) photons are believed to have ionized intergalactic hydrogen, rendering the Universe transparent to UV radiation. Galaxies brighter than the characteristic luminosity L*&amp;nbsp;(refs.&amp;nbsp;1,2) do not provide enough ionizing photons to drive this cosmic reionization. Fainter galaxies are thought to dominate the photon budget; however, they are surrounded by neutral gas that prevents the escape of the Lyman-α photons, which has been the dominant way to identify them so far. JD1 was previously identified as a triply-imaged galaxy with a magnification factor of 13 provided by the foreground cluster Abell 2744 (ref. 3), and a photometric redshift of z ≈ 10. Here we report the spectroscopic confirmation of this very low luminosity (≈0.05 L*) galaxy at z = 9.79, observed 480 Myr after the Big Bang, by means of the identification of the Lyman break and redward continuum, as well as multiple ≳4σ emission lines, with...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/823315h2</guid>
      <pubDate>Wed, 11 Mar 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Roberts-Borsani, Guido</name>
      </author>
      <author>
        <name>Treu, Tommaso</name>
        <uri>https://orcid.org/0000-0002-8460-0390</uri>
      </author>
      <author>
        <name>Chen, Wenlei</name>
      </author>
      <author>
        <name>Morishita, Takahiro</name>
      </author>
      <author>
        <name>Vanzella, Eros</name>
      </author>
      <author>
        <name>Zitrin, Adi</name>
      </author>
      <author>
        <name>Bergamini, Pietro</name>
      </author>
      <author>
        <name>Castellano, Marco</name>
      </author>
      <author>
        <name>Fontana, Adriano</name>
      </author>
      <author>
        <name>Glazebrook, Karl</name>
      </author>
      <author>
        <name>Grillo, Claudio</name>
      </author>
      <author>
        <name>Kelly, Patrick L</name>
      </author>
      <author>
        <name>Merlin, Emiliano</name>
      </author>
      <author>
        <name>Nanayakkara, Themiya</name>
      </author>
      <author>
        <name>Paris, Diego</name>
      </author>
      <author>
        <name>Rosati, Piero</name>
      </author>
      <author>
        <name>Yang, Lilan</name>
      </author>
      <author>
        <name>Acebron, Ana</name>
      </author>
      <author>
        <name>Bonchi, Andrea</name>
      </author>
      <author>
        <name>Boyett, Kit</name>
      </author>
      <author>
        <name>Bradač, Maruša</name>
      </author>
      <author>
        <name>Brammer, Gabriel</name>
      </author>
      <author>
        <name>Broadhurst, Tom</name>
      </author>
      <author>
        <name>Calabró, Antonello</name>
      </author>
      <author>
        <name>Diego, Jose M</name>
      </author>
      <author>
        <name>Dressler, Alan</name>
      </author>
      <author>
        <name>Furtak, Lukas J</name>
      </author>
      <author>
        <name>Filippenko, Alexei V</name>
        <uri>https://orcid.org/0000-0003-3460-0103</uri>
      </author>
      <author>
        <name>Henry, Alaina</name>
      </author>
      <author>
        <name>Koekemoer, Anton M</name>
      </author>
      <author>
        <name>Leethochawalit, Nicha</name>
      </author>
      <author>
        <name>Malkan, Matthew A</name>
        <uri>https://orcid.org/0000-0001-6919-1237</uri>
      </author>
      <author>
        <name>Mason, Charlotte</name>
      </author>
      <author>
        <name>Mercurio, Amata</name>
      </author>
      <author>
        <name>Metha, Benjamin</name>
      </author>
      <author>
        <name>Pentericci, Laura</name>
      </author>
      <author>
        <name>Pierel, Justin</name>
      </author>
      <author>
        <name>Rieck, Steven</name>
      </author>
      <author>
        <name>Roy, Namrata</name>
      </author>
      <author>
        <name>Santini, Paola</name>
      </author>
      <author>
        <name>Strait, Victoria</name>
      </author>
      <author>
        <name>Strausbaugh, Robert</name>
      </author>
      <author>
        <name>Trenti, Michele</name>
      </author>
      <author>
        <name>Vulcani, Benedetta</name>
      </author>
      <author>
        <name>Wang, Lifan</name>
      </author>
      <author>
        <name>Wang, Xin</name>
        <uri>https://orcid.org/0009-0006-8812-5175</uri>
      </author>
      <author>
        <name>Windhorst, Rogier A</name>
      </author>
    </item>
    <item>
      <title>A massive interacting galaxy 510 million years after the Big Bang</title>
      <link>https://escholarship.org/uc/item/80h7j3rn</link>
      <description>James Webb Space Telescope observations have spectroscopically confirmed the existence of galaxies as early as 300 Myr after the Big Bang and with a higher number density than what was expected based on galaxy formation models and Hubble Space Telescope observations. Yet, most sources confirmed spectroscopically so far in the first 500 Myr have rest-frame ultraviolet (UV) luminosities below the characteristic luminosity (MUV*$${M}_\mathrm{UV}^{* }$$), limiting the signal-to-noise ratio for investigating substructure. Here we present a high-resolution spectroscopic and spatially resolved study of a bright galaxy (MUV = −21.66 ± 0.03, ~2MUV*$$\sim 2{M}_\mathrm{UV}^{* }$$) at a redshift z = 9.3127 ± 0.0002 (510 Myr after the Big Bang) with an estimated stellar mass of 1.6−0.4+0.5×109M⊙$$\left(1.6_{-0.4}^{+0.5}\right)\times 10^{9}\,M_{\odot }$$, forming 19−6+5$$1{9}_{-6}^{+5}$$ solar masses per year and with a metallicity of about one tenth that of solar. The system has a morphology...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/80h7j3rn</guid>
      <pubDate>Wed, 11 Mar 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Boyett, Kristan</name>
      </author>
      <author>
        <name>Trenti, Michele</name>
      </author>
      <author>
        <name>Leethochawalit, Nicha</name>
      </author>
      <author>
        <name>Calabró, Antonello</name>
      </author>
      <author>
        <name>Metha, Benjamin</name>
      </author>
      <author>
        <name>Roberts-Borsani, Guido</name>
      </author>
      <author>
        <name>Dalmasso, Nicoló</name>
      </author>
      <author>
        <name>Yang, Lilan</name>
      </author>
      <author>
        <name>Santini, Paola</name>
      </author>
      <author>
        <name>Treu, Tommaso</name>
        <uri>https://orcid.org/0000-0002-8460-0390</uri>
      </author>
      <author>
        <name>Jones, Tucker</name>
        <uri>https://orcid.org/0000-0001-5860-3419</uri>
      </author>
      <author>
        <name>Henry, Alaina</name>
      </author>
      <author>
        <name>Mason, Charlotte A</name>
      </author>
      <author>
        <name>Morishita, Takahiro</name>
      </author>
      <author>
        <name>Nanayakkara, Themiya</name>
      </author>
      <author>
        <name>Roy, Namrata</name>
      </author>
      <author>
        <name>Wang, Xin</name>
        <uri>https://orcid.org/0009-0006-8812-5175</uri>
      </author>
      <author>
        <name>Fontana, Adriano</name>
      </author>
      <author>
        <name>Merlin, Emiliano</name>
      </author>
      <author>
        <name>Castellano, Marco</name>
      </author>
      <author>
        <name>Paris, Diego</name>
      </author>
      <author>
        <name>Bradač, Maruša</name>
      </author>
      <author>
        <name>Malkan, Matt</name>
        <uri>https://orcid.org/0000-0001-6919-1237</uri>
      </author>
      <author>
        <name>Marchesini, Danilo</name>
      </author>
      <author>
        <name>Mascia, Sara</name>
      </author>
      <author>
        <name>Glazebrook, Karl</name>
      </author>
      <author>
        <name>Pentericci, Laura</name>
      </author>
      <author>
        <name>Vanzella, Eros</name>
      </author>
      <author>
        <name>Vulcani, Benedetta</name>
      </author>
    </item>
    <item>
      <title>Early Results from GLASS-JWST. IV. Spatially Resolved Metallicity in a Low-mass z ∼ 3 Galaxy with NIRISS* *Based on observations acquired by the JWST under the ERS program ID 1324 (PI T. Treu).</title>
      <link>https://escholarship.org/uc/item/66v9h178</link>
      <description>We report the first gas-phase metallicity map of a distant galaxy measured with the James Webb Space Telescope (JWST). We use the NIRISS slitless spectroscopy acquired by the GLASS Early Release Science program to spatially resolve the rest-frame optical nebular emission lines in a gravitationally lensed galaxy at z = 3.06 behind the A2744 galaxy cluster. This galaxy (dubbed GLASS-Zgrad1) has stellar mass ∼108.6 M ⊙, instantaneous star formation rate ∼8.6 M ⊙ yr−1 (both corrected for lensing magnification), and global metallicity one-fourth solar. From its emission-line maps ([O iii], Hβ, Hγ, [Ne iii], and [O ii]), we derive its spatial distribution of gas-phase metallicity using a well-established forward-modeling Bayesian inference method. The exquisite resolution and sensitivity of JWST/NIRISS, combined with lensing magnification, enable us to resolve this z ∼ 3 dwarf galaxy in ≳50 resolution elements with sufficient signal, an analysis hitherto not possible. We find that the...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/66v9h178</guid>
      <pubDate>Wed, 11 Mar 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Wang, Xin</name>
        <uri>https://orcid.org/0009-0006-8812-5175</uri>
      </author>
      <author>
        <name>Jones, Tucker</name>
        <uri>https://orcid.org/0000-0001-5860-3419</uri>
      </author>
      <author>
        <name>Vulcani, Benedetta</name>
      </author>
      <author>
        <name>Treu, Tommaso</name>
        <uri>https://orcid.org/0000-0002-8460-0390</uri>
      </author>
      <author>
        <name>Morishita, Takahiro</name>
      </author>
      <author>
        <name>Roberts-Borsani, Guido</name>
      </author>
      <author>
        <name>Malkan, Matthew A</name>
        <uri>https://orcid.org/0000-0001-6919-1237</uri>
      </author>
      <author>
        <name>Henry, Alaina</name>
      </author>
      <author>
        <name>Brammer, Gabriel</name>
      </author>
      <author>
        <name>Strait, Victoria</name>
      </author>
      <author>
        <name>Bradač, Maruša</name>
      </author>
      <author>
        <name>Boyett, Kristan</name>
      </author>
      <author>
        <name>Calabrò, Antonello</name>
      </author>
      <author>
        <name>Castellano, Marco</name>
      </author>
      <author>
        <name>Fontana, Adriano</name>
      </author>
      <author>
        <name>Glazebrook, Karl</name>
      </author>
      <author>
        <name>Kelly, Patrick L</name>
      </author>
      <author>
        <name>Leethochawalit, Nicha</name>
      </author>
      <author>
        <name>Marchesini, Danilo</name>
      </author>
      <author>
        <name>Santini, P</name>
      </author>
      <author>
        <name>Trenti, M</name>
      </author>
      <author>
        <name>Yang, Lilan</name>
      </author>
    </item>
    <item>
      <title>Early Results from GLASS-JWST. XVIII. A First Morphological Atlas of the 1 &amp;lt; z &amp;lt; 5 Universe in the Rest-frame Optical</title>
      <link>https://escholarship.org/uc/item/52k7z859</link>
      <description>We present a rest-frame optical morphological analysis of galaxies observed with the NIRCam imager on the James Webb Space Telescope (JWST) as part of the GLASS-JWST Early Release Science program. We select 388 sources at redshifts 0.8 &amp;lt; z &amp;lt; 5.4 and use the seven 0.9–5 μm NIRCam filters to generate rest-frame gri composite color images, and conduct visual morphological classification. Compared to Hubble Space Telescope (HST)–based work we find a higher incidence of disks and bulges than expected at z &amp;gt; 1.5, revealed by rest-frame optical imaging. We detect 123 clear disks (58 at z &amp;gt; 1.5) of which 76 have bulges. No evolution of bulge fraction with redshift is evident: 61% at z &amp;lt; 2 (N = 110) versus 60% at z ≥ 2 (N = 13). A stellar mass dependence is evident, with bulges visible in 80% of all disk galaxies with mass &amp;gt;109.5 M ⊙ (N = 41) but only 52% at M &amp;lt; 109.5 M ⊙ (N = 82). We supplement visual morphologies with nonparametric measurements of Gini and asymmetry...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/52k7z859</guid>
      <pubDate>Wed, 11 Mar 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Jacobs, C</name>
      </author>
      <author>
        <name>Glazebrook, K</name>
      </author>
      <author>
        <name>Calabrò, A</name>
      </author>
      <author>
        <name>Treu, T</name>
        <uri>https://orcid.org/0000-0002-8460-0390</uri>
      </author>
      <author>
        <name>Nannayakkara, T</name>
      </author>
      <author>
        <name>Jones, T</name>
        <uri>https://orcid.org/0000-0001-5860-3419</uri>
      </author>
      <author>
        <name>Merlin, E</name>
      </author>
      <author>
        <name>Abraham, R</name>
      </author>
      <author>
        <name>Stevens, ARH</name>
      </author>
      <author>
        <name>Vulcani, B</name>
      </author>
      <author>
        <name>Yang, L</name>
      </author>
      <author>
        <name>Bonchi, A</name>
      </author>
      <author>
        <name>Boyett, K</name>
      </author>
      <author>
        <name>Bradač, M</name>
      </author>
      <author>
        <name>Castellano, M</name>
      </author>
      <author>
        <name>Fontana, A</name>
      </author>
      <author>
        <name>Marchesini, D</name>
      </author>
      <author>
        <name>Malkan, M</name>
        <uri>https://orcid.org/0000-0001-6919-1237</uri>
      </author>
      <author>
        <name>Mason, C</name>
      </author>
      <author>
        <name>Morishita, T</name>
      </author>
      <author>
        <name>Paris, D</name>
      </author>
      <author>
        <name>Santini, P</name>
      </author>
      <author>
        <name>Trenti, M</name>
      </author>
      <author>
        <name>Wang, X</name>
        <uri>https://orcid.org/0009-0006-8812-5175</uri>
      </author>
    </item>
    <item>
      <title>The GLASS-JWST Early Release Science Program. I. Survey Design and Release Plans</title>
      <link>https://escholarship.org/uc/item/072006g3</link>
      <description>The GLASS-JWST Early Release Science (hereafter GLASS-JWST-ERS) Program will obtain and make publicly available the deepest extragalactic data of the ERS campaign. It is primarily designed to address two key science questions, namely, “what sources ionized the universe and when?” and “how do baryons cycle through galaxies?”, while also enabling a broad variety of first look scientific investigations. In primary mode, it will obtain NIRISS and NIRSpec spectroscopy of galaxies lensed by the foreground Hubble Frontier Field cluster, Abell 2744. In parallel, it will use NIRCam to observe two fields that are offset from the cluster center, where lensing magnification is negligible, and which can thus be effectively considered blank fields. In order to prepare the community for access to this unprecedented data, we describe the scientific rationale, the survey design (including target selection and observational setups), and present pre-commissioning estimates of the expected sensitivity....</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/072006g3</guid>
      <pubDate>Wed, 11 Mar 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Treu, T</name>
        <uri>https://orcid.org/0000-0002-8460-0390</uri>
      </author>
      <author>
        <name>Roberts-Borsani, G</name>
      </author>
      <author>
        <name>Bradac, M</name>
        <uri>https://orcid.org/0000-0001-5984-0395</uri>
      </author>
      <author>
        <name>Brammer, G</name>
      </author>
      <author>
        <name>Fontana, A</name>
      </author>
      <author>
        <name>Henry, A</name>
      </author>
      <author>
        <name>Mason, C</name>
      </author>
      <author>
        <name>Morishita, T</name>
      </author>
      <author>
        <name>Pentericci, L</name>
      </author>
      <author>
        <name>Wang, X</name>
        <uri>https://orcid.org/0009-0006-8812-5175</uri>
      </author>
      <author>
        <name>Acebron, A</name>
      </author>
      <author>
        <name>Bagley, M</name>
      </author>
      <author>
        <name>Bergamini, P</name>
      </author>
      <author>
        <name>Belfiori, D</name>
      </author>
      <author>
        <name>Bonchi, A</name>
      </author>
      <author>
        <name>Boyett, K</name>
      </author>
      <author>
        <name>Boutsia, K</name>
      </author>
      <author>
        <name>Calabró, A</name>
      </author>
      <author>
        <name>Caminha, GB</name>
      </author>
      <author>
        <name>Castellano, M</name>
      </author>
      <author>
        <name>Dressler, A</name>
      </author>
      <author>
        <name>Glazebrook, K</name>
      </author>
      <author>
        <name>Grillo, C</name>
      </author>
      <author>
        <name>Jacobs, C</name>
      </author>
      <author>
        <name>Jones, T</name>
        <uri>https://orcid.org/0000-0001-5860-3419</uri>
      </author>
      <author>
        <name>Kelly, PL</name>
      </author>
      <author>
        <name>Leethochawalit, N</name>
      </author>
      <author>
        <name>Malkan, MA</name>
        <uri>https://orcid.org/0000-0001-6919-1237</uri>
      </author>
      <author>
        <name>Marchesini, D</name>
      </author>
      <author>
        <name>Mascia, S</name>
      </author>
      <author>
        <name>Mercurio, A</name>
      </author>
      <author>
        <name>Merlin, E</name>
      </author>
      <author>
        <name>Nanayakkara, T</name>
      </author>
      <author>
        <name>Nonino, M</name>
      </author>
      <author>
        <name>Paris, D</name>
      </author>
      <author>
        <name>Poggianti, B</name>
      </author>
      <author>
        <name>Rosati, P</name>
      </author>
      <author>
        <name>Santini, P</name>
      </author>
      <author>
        <name>Scarlata, C</name>
      </author>
      <author>
        <name>Shipley, HV</name>
      </author>
      <author>
        <name>Strait, V</name>
      </author>
      <author>
        <name>Trenti, M</name>
      </author>
      <author>
        <name>Tubthong, C</name>
      </author>
      <author>
        <name>Vanzella, E</name>
      </author>
      <author>
        <name>Vulcani, B</name>
      </author>
      <author>
        <name>Yang, L</name>
      </author>
    </item>
    <item>
      <title>Ultrahigh pressure compaction-resistant thin film crosslinked composite reverse osmosis membranes</title>
      <link>https://escholarship.org/uc/item/0nf558m4</link>
      <description>In this study, we present a class of thin-film crosslinked (TFX) composite reverse osmosis (RO) membranes that resist physical compaction at ultrahigh pressures (up to 200 bar). Since RO membranes experience compaction at virtually all pressure ranges, the ability to resist compaction has widespread implications for RO membrane technology. The process described herein involves crosslinking a phase inverted porous polyimide (PI) support membrane followed by interfacial polymerization of a polyamide layer, thereby forming a fully thermoset composite membrane structure. We explore a range of phase inversion membrane formation parameters such as PI concentration, solvent-cosolvent ratios, coagulation bath composition, and crosslinking methods in addition to interfacial polymerization reaction chemistry and conditions. Overall, TFX membranes exhibit significantly less compaction compared to hand-cast and commercial high-pressure RO membranes, experiencing less than 10% decline in water...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/0nf558m4</guid>
      <pubDate>Tue, 3 Mar 2026 00:00:00 +0000</pubDate>
      <author>
        <name>Wu, Jishan</name>
      </author>
      <author>
        <name>Quezada-Renteria, Javier A</name>
      </author>
      <author>
        <name>He, Jinlong</name>
      </author>
      <author>
        <name>Xiao, Minhao</name>
      </author>
      <author>
        <name>Chen, Yuanmiaoliang</name>
      </author>
      <author>
        <name>Fan, Hanqing</name>
      </author>
      <author>
        <name>Wang, Xinyi</name>
        <uri>https://orcid.org/0009-0006-8812-5175</uri>
      </author>
      <author>
        <name>Chen, Fiona</name>
      </author>
      <author>
        <name>Pataroque, Kevin</name>
      </author>
      <author>
        <name>Suleiman, Yara</name>
      </author>
      <author>
        <name>Shahbazmohamadi, Sina</name>
      </author>
      <author>
        <name>Sreejith, NA</name>
      </author>
      <author>
        <name>Sitaraman, Hariswaran</name>
      </author>
      <author>
        <name>Day, Marc</name>
      </author>
      <author>
        <name>Li, Ying</name>
      </author>
      <author>
        <name>Jassby, David</name>
      </author>
      <author>
        <name>McCutcheon, Jeffrey R</name>
      </author>
      <author>
        <name>Elimelech, Menachem</name>
      </author>
      <author>
        <name>Hoek, Eric MV</name>
        <uri>https://orcid.org/0000-0002-9674-1916</uri>
      </author>
    </item>
    <item>
      <title>Regional Data Sets Included in the NGA-West3 Ground Motion Database</title>
      <link>https://escholarship.org/uc/item/12d2p4n5</link>
      <description>The Next Generation Attenuation (NGA)-West3 Program database builds upon that of NGA-West2 for shallow crustal earthquakes in active tectonic regimes to provide a robust data set to develop the next iteration of NGA ground motion models (GMMs). Researchers from Italy, Japan, New Zealand, Taiwan, United Arab Emirates, and the United States, amongst others, have collaborated to develop consistently processed data with uniform metadata from the respective regions, with data for other regions drawn from literature (e.g., Greece, Japan, and Türkiye). Over 80,000 three-component ground motions from 632 events with magnitudes generally greater than 4.0 across the Western United States (mostly in California) have been newly added, and the total database size is over 175,000 ground motions (generally three-component except for two-component records from KiK-Net stations in Japan). The database is being used by several teams of NGA GMM developers and will be publicly released sometime in...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/12d2p4n5</guid>
      <pubDate>Thu, 20 Nov 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Buckreis, Tristan E</name>
      </author>
      <author>
        <name>Brandenberg, Scott J</name>
      </author>
      <author>
        <name>Mohammed, Shako</name>
      </author>
      <author>
        <name>Nweke, Chuckwuebuka C</name>
      </author>
      <author>
        <name>Shams, Rashid</name>
      </author>
      <author>
        <name>Bahrampouri, Mahdi</name>
      </author>
      <author>
        <name>Bradley, Brendon A</name>
      </author>
      <author>
        <name>Huang, Jyun-Yan</name>
      </author>
      <author>
        <name>Kishida, Tadahiro</name>
      </author>
      <author>
        <name>Lanzano, Giovanni</name>
      </author>
      <author>
        <name>Li, Meibai</name>
      </author>
      <author>
        <name>Luzi, Lucia</name>
      </author>
      <author>
        <name>Pajaro Miranda, Cesar</name>
      </author>
      <author>
        <name>Zimmaro, Paolo</name>
      </author>
      <author>
        <name>Bozorgnia, Yousef</name>
      </author>
      <author>
        <name>Donahue, Jennifer L</name>
      </author>
      <author>
        <name>Stewart, Jonathan P</name>
        <uri>https://orcid.org/0000-0003-3602-3629</uri>
      </author>
    </item>
    <item>
      <title>MSA-3D: Dissecting Galaxies at z ∼ 1 with High Spatial and Spectral Resolution</title>
      <link>https://escholarship.org/uc/item/74d8z25d</link>
      <description>Integral field spectroscopy (IFS) is a powerful tool for understanding the formation of galaxies across cosmic history. We present the observing strategy and first results of MSA-3D, a novel JWST program using multi-object spectroscopy in a slit-stepping strategy to produce IFS data cubes. The program observed 43 normal star-forming galaxies at redshifts 0.5 ≲ z ≲ 1.5, corresponding to the epoch when spiral thin-disk galaxies of the modern Hubble sequence are thought to emerge, obtaining kiloparsec-scale maps of rest-frame optical nebular emission lines with spectral resolution R ≃ 2700. Here we describe the multiplexed slit-stepping method, which is &amp;gt;15 times more efficient than the NIRSpec IFS mode for our program. As an example of the data quality, we present a case study of an individual galaxy at z = 1.104 (stellar mass M* = 1010.3M⊙, star formation rate, SFR = 3M⊙ yr−1) with prominent face-on spiral structure. We show that the galaxy exhibits a rotationally supported...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/74d8z25d</guid>
      <pubDate>Wed, 19 Nov 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Barišić, Ivana</name>
      </author>
      <author>
        <name>Jones, Tucker</name>
        <uri>https://orcid.org/0000-0001-5860-3419</uri>
      </author>
      <author>
        <name>Mortensen, Kris</name>
      </author>
      <author>
        <name>Nanayakkara, Themiya</name>
      </author>
      <author>
        <name>Chen, Yuguang</name>
      </author>
      <author>
        <name>Sanders, Ryan</name>
      </author>
      <author>
        <name>Bullock, James S</name>
        <uri>https://orcid.org/0000-0003-4298-5082</uri>
      </author>
      <author>
        <name>Bundy, Kevin</name>
      </author>
      <author>
        <name>Faucher-Giguère, Claude-André</name>
      </author>
      <author>
        <name>Glazebrook, Karl</name>
      </author>
      <author>
        <name>Henry, Alaina</name>
      </author>
      <author>
        <name>Ju, Mengting</name>
      </author>
      <author>
        <name>Malkan, Matthew</name>
        <uri>https://orcid.org/0000-0001-6919-1237</uri>
      </author>
      <author>
        <name>Morishita, Takahiro</name>
      </author>
      <author>
        <name>Obreschkow, Danail</name>
      </author>
      <author>
        <name>Roy, Namrata</name>
      </author>
      <author>
        <name>Salcedo, Juan M Espejo</name>
      </author>
      <author>
        <name>Shapley, Alice E</name>
      </author>
      <author>
        <name>Treu, Tommaso</name>
        <uri>https://orcid.org/0000-0002-8460-0390</uri>
      </author>
      <author>
        <name>Wang, Xin</name>
        <uri>https://orcid.org/0009-0006-8812-5175</uri>
      </author>
      <author>
        <name>Westfall, Kyle B</name>
        <uri>https://orcid.org/0000-0003-1809-6920</uri>
      </author>
    </item>
    <item>
      <title>Extrapolation Algorithm for Computing z1.0 from Shallow Measured Velocity Profile</title>
      <link>https://escholarship.org/uc/item/5v38s1xv</link>
      <description>Ground motion models (GMMs) use depth to shear wave velocity (VS) isosurfaces to quantify site response effects arising from sediment thickness, with z1.0 (i.e., the depth to Vs = 1,000 m/s) often used. However, direct measurements of z1.0 are rare, and z1.0 is poorly resolved in tomographic measurements often used to develop community velocity models (CVMs), particularly in shallow layers and near basin edges. To address this challenge, we present an algorithm for estimating z1.0 for shear wave velocity profiles that do not reach VS = 1,000 m/s. The model is conditioned on the shear wave velocity at the bottom of the profile, VS (zp), and the average gradient near the bottom of the profile (dVS/dz). Using 253 direct z1.0 measurements from the shear wave velocity profile database (VSPDB), we regressed coefficients for VS (zp) = 500 to 1,000 m/s. We then used the algorithm to extend 622 VS profiles that reach ≥500 m/s, but not 1,000 m/s, and quantify distributions of z1.0 based...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/5v38s1xv</guid>
      <pubDate>Wed, 19 Nov 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Shams, Rashid</name>
      </author>
      <author>
        <name>Buckreis, Tristan E</name>
      </author>
      <author>
        <name>Nweke, Chukwuebuka C</name>
      </author>
      <author>
        <name>Brandenberg, Scott J</name>
      </author>
      <author>
        <name>Stewart, Jonathan P</name>
        <uri>https://orcid.org/0000-0003-3602-3629</uri>
      </author>
    </item>
    <item>
      <title>BEACON: JWST NIRCam Pure-parallel Imaging Survey. I. Survey Design and Initial Results</title>
      <link>https://escholarship.org/uc/item/1k50b56x</link>
      <description>We introduce the Bias-free Extragalactic Analysis for Cosmic Origins with NIRCam (BEACON) survey, a JWST Cycle 2 program allocated up to 600 pure-parallel hours of observations. BEACON explores high-latitude areas of the sky with JWST/NIRCam over ∼100 independent sight lines, totaling ∼0.3 deg2, reaching a median F444W depth of ≈28.2 AB mag (5σ). Based on existing JWST observations in legacy fields, we estimate that BEACON will photometrically identify 25–150 galaxies at z &amp;gt; 10 and 500–1000 at z ∼ 7–10 uniquely enabled by an efficient multiple filter configuration spanning 0.9–5.0 μm. The expected sample size of z &amp;gt; 10 galaxies will allow us to obtain robust number density estimates and to discriminate between different models of early star formation. In this paper, we present an overview of the survey design and initial results using the first 19 fields. We present 129 galaxy candidates at z ≳7 identified in those fields, including 11 galaxies at z ≳10 and several UV-luminous...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/1k50b56x</guid>
      <pubDate>Wed, 19 Nov 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Morishita, Takahiro</name>
      </author>
      <author>
        <name>Mason, Charlotte A</name>
      </author>
      <author>
        <name>Kreilgaard, Kimi C</name>
      </author>
      <author>
        <name>Trenti, Michele</name>
      </author>
      <author>
        <name>Treu, Tommaso</name>
        <uri>https://orcid.org/0000-0002-8460-0390</uri>
      </author>
      <author>
        <name>Vulcani, Benedetta</name>
      </author>
      <author>
        <name>Zhang, Yechi</name>
      </author>
      <author>
        <name>Abdurro’uf</name>
      </author>
      <author>
        <name>Alavi, Anahita</name>
      </author>
      <author>
        <name>Atek, Hakim</name>
      </author>
      <author>
        <name>Bahé, Yannick</name>
      </author>
      <author>
        <name>Bradač, Maruša</name>
      </author>
      <author>
        <name>Bradley, Larry D</name>
      </author>
      <author>
        <name>Bunker, Andrew J</name>
      </author>
      <author>
        <name>Coe, Dan</name>
      </author>
      <author>
        <name>Colbert, James</name>
      </author>
      <author>
        <name>Gelli, Viola</name>
      </author>
      <author>
        <name>Hayes, Matthew J</name>
      </author>
      <author>
        <name>Jones, Tucker</name>
        <uri>https://orcid.org/0000-0001-5860-3419</uri>
      </author>
      <author>
        <name>Kodama, Tadayuki</name>
      </author>
      <author>
        <name>Leethochawalit, Nicha</name>
      </author>
      <author>
        <name>Liu, Zhaoran</name>
      </author>
      <author>
        <name>Malkan, Matthew A</name>
        <uri>https://orcid.org/0000-0001-6919-1237</uri>
      </author>
      <author>
        <name>Mehta, Vihang</name>
      </author>
      <author>
        <name>Metha, Benjamin</name>
      </author>
      <author>
        <name>Newman, Andrew B</name>
      </author>
      <author>
        <name>Rafelski, Marc</name>
      </author>
      <author>
        <name>Roberts-Borsani, Guido</name>
      </author>
      <author>
        <name>Rutkowski, Michael J</name>
      </author>
      <author>
        <name>Scarlata, Claudia</name>
      </author>
      <author>
        <name>Stiavelli, Massimo</name>
      </author>
      <author>
        <name>Sutanto, Ryo A</name>
      </author>
      <author>
        <name>Takahashi, Kosuke</name>
      </author>
      <author>
        <name>Teplitz, Harry I</name>
      </author>
      <author>
        <name>Wang, Xin</name>
        <uri>https://orcid.org/0009-0006-8812-5175</uri>
      </author>
    </item>
    <item>
      <title>Relationship between Factors of Safety against Soil Liquefaction Triggering and Liquefaction Effects on Ground Motions</title>
      <link>https://escholarship.org/uc/item/0bj414s7</link>
      <description>We assess soil liquefaction effects on ground surface motions as a function of factor of safety against liquefaction triggering (FSliq) The effects of soil liquefaction on ground motions are quantified by the ratio of acceleration response spectra (AFliq) calculated based on one-dimensional effective- and total-stress simulations conducted in a finite-difference code. Three methods for computing FSliq are explored: one from a liquefaction triggering model, including a magnitude scaling factor, and two from cycle counting for ground surface motion or shear stresses at depth. Our results indicate that soil liquefaction leads to a predominant amplification of ground motions in the short- and long-period ranges and de-amplification of ground motions in the intermediate period range, approximately from 0.1 to 0.9 s. We found that FSliq is a promising indicator of the liquefaction effects on ground motions and that ground motions at sites with FSliq higher than 0.9 are only moderately...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/0bj414s7</guid>
      <pubDate>Wed, 19 Nov 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Pretell, Renmin</name>
      </author>
      <author>
        <name>Brandenberg, Scott J</name>
      </author>
      <author>
        <name>Stewart, Jonathan P</name>
      </author>
      <author>
        <name>Gingery, James R</name>
      </author>
      <author>
        <name>Zafir, Zia</name>
      </author>
    </item>
    <item>
      <title>Sub-Regional Site Response in the San Francisco Bay Area</title>
      <link>https://escholarship.org/uc/item/78j5f3vp</link>
      <description>Initial results of an ongoing project to develop a site response model specific to Northern California are presented, focusing on the San Francisco Bay Area (SFBA). Although current NGA-West2 ground motion models were developed for application across broad regions (such as California), they have the potential to be biased when applied to particular sub-regions. This study investigates the impacts of the unique geology in the SFBA on site response features. A model conditioned on time-averaged shear-wave velocity in the upper 30 m (VS30) and broad geomorphic categories (future iterations of the model will also consider depths to shear-wave velocity isosurfaces, z1.0) is used in this study. A critical element in the modeling process is to reflect the impact of different geologic conditions through the selected geomorphic categories, including (from rock to soil) Franciscan, Great Valley Sequence, and Tertiary rock, shelf deposits, valleys, and basins. When all sites are grouped,...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/78j5f3vp</guid>
      <pubDate>Mon, 17 Nov 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Mohammed, Shako</name>
      </author>
      <author>
        <name>Shams, Rashid</name>
      </author>
      <author>
        <name>Buckreis, Tristan E</name>
      </author>
      <author>
        <name>Nweke, Chukwuebuka C</name>
      </author>
      <author>
        <name>Brandenberg, Scott J</name>
      </author>
      <author>
        <name>Stewart, Jonathan P</name>
        <uri>https://orcid.org/0000-0003-3602-3629</uri>
      </author>
    </item>
    <item>
      <title>Identification of Site Response Features Using Microtremor HVSR</title>
      <link>https://escholarship.org/uc/item/47h152kk</link>
      <description>Frequency-dependent horizontal-to-vertical spectral ratios (HVSR) of three-component recordings provide information on-site resonant frequencies, which are potentially useful for predicting site response. We compute microtremor-derived HVSR (mHVSR) from Fourier amplitude spectra (FAS) using a relational database for site data, mainly in California. Using these data, we identify sites with peaks, sites with no peaks, and characteristics of peaks for sites that have them. Using a separate relational database for earthquake ground motion studies, we identify period-dependent response-spectra site terms, which reflect the mean offsets of site-specific ground motions from predictions of a ground motion model (GMM). Those site terms may have peaks, no peaks, or transitions from low-to-high values (with or without peaks) over some period range. This paper evaluates the degree to which features of site terms can be mapped to features of mHVSR at the same site. This is an important step...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/47h152kk</guid>
      <pubDate>Mon, 17 Nov 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Ornelas, Francisco Javier G</name>
        <uri>https://orcid.org/0009-0008-3798-6332</uri>
      </author>
      <author>
        <name>de la Torre, Christopher A</name>
      </author>
      <author>
        <name>Buckreis, Tristan E</name>
      </author>
      <author>
        <name>Nweke, Chukwuebuka C</name>
      </author>
      <author>
        <name>Brandenberg, Scott J</name>
      </author>
      <author>
        <name>Stewart, Jonathan P</name>
        <uri>https://orcid.org/0000-0003-3602-3629</uri>
      </author>
    </item>
    <item>
      <title>Application of Liquefaction Susceptibility Criteria within a Logic Tree Framework</title>
      <link>https://escholarship.org/uc/item/1149q7sg</link>
      <description>The probabilistic assessment of seismic ground failure hazards at any given site typically follows a three-step process that includes (1) estimating the probability of a given soil unit being susceptible to liquefaction (with the complement representing the probability of strength loss associated with cyclic softening); (2) estimating the probability that liquefaction would be triggered (if susceptible) or that cyclic softening would occur (if non-susceptible) given soil characteristics and anticipated ground shaking levels; and (3) estimating the potential impacts (surface manifestation, deformations, instabilities) from liquefied or softened strata. The three-stage liquefaction and cyclic softening hazard assessment process can be illustrated using a logic tree to allow different models and model weights to be considered in each step. We propose a logic tree formulation in which different weights are used for cyclic strength evaluation procedures for susceptible and non-susceptible...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/1149q7sg</guid>
      <pubDate>Mon, 17 Nov 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Sahin, Arda</name>
      </author>
      <author>
        <name>Jana, Amalesh</name>
      </author>
      <author>
        <name>Ulmer, Kristin J</name>
      </author>
      <author>
        <name>Brandenberg, Scott J</name>
      </author>
      <author>
        <name>Evans, T Matthew</name>
      </author>
      <author>
        <name>Kramer, Steven L</name>
      </author>
      <author>
        <name>Stewart, Jonathan P</name>
        <uri>https://orcid.org/0000-0003-3602-3629</uri>
      </author>
      <author>
        <name>Stuedlein, Armin W</name>
      </author>
    </item>
    <item>
      <title>Using Laboratory Data to Model the Cyclic Strength Transition from Clean Sands to Fines-Dominated Soils</title>
      <link>https://escholarship.org/uc/item/0zs615nn</link>
      <description>Existing fine corrections in liquefaction triggering models are generally formulated as an additive or multiplicative factor applied to the penetration resistance and were derived from liquefaction case history databases. Fines influence both the measured tip resistance and the cyclic resistance ratio (CRR) of the soil to varying extents. However, the fine corrections currently used in triggering models simultaneously represent the effect of fines on CRR and on penetration resistance through a single correction factor. Our long-term research objective is to develop separate fine corrections for CRR and penetration resistance. This paper focuses on the effect of fines on CRR. We present a framework that envisions modeling the CRR of clean sands based on relative density, DR, and represents the CRR of fines-dominated soils using a cyclic softening framework. An interpolation function will then bridge the gap between these two extremes, using regression of the gathered laboratory...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/0zs615nn</guid>
      <pubDate>Mon, 17 Nov 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Renugah, Varun Nigesh Sivakumar</name>
      </author>
      <author>
        <name>Sahin, Arda</name>
      </author>
      <author>
        <name>Brandenberg, Scott J</name>
      </author>
      <author>
        <name>Stewart, Jonathan P</name>
        <uri>https://orcid.org/0000-0003-3602-3629</uri>
      </author>
    </item>
    <item>
      <title>Panel Review of Ground Motion Characterization Model for the 2025 Update of the NSHM for Puerto Rico and the Virgin Islands</title>
      <link>https://escholarship.org/uc/item/28m4b7jr</link>
      <description>The 2025 update of the National Seismic Hazard Model (NSHM) for Puerto Rico and the Virgin Islands (PRVI) replaces a previous version of the model from 2003. The 2025 update has two major components – a seismic source characterization (SSC) model and a ground motion characterization (GMC) model. In August 2024, the Steering Committee for the NSHM formed this Panel to review the GMC component of the NSHM work for PRVI. The panel is advisory, meaning that we provide input on technical issues for consideration by the Steering Committee and the USGS NSHM team, but we do not have decision making authority. Final modeling decisions are presented in separate USGS documents, including Shumway et al. (2025), Moschetti et al. (2025), Moschetti (2025), and Withers et al. (2025). Where modeling decisions depart from our recommendations, the rationale is explained in those publications.</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/28m4b7jr</guid>
      <pubDate>Sun, 16 Nov 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Stewart, Jonathan P</name>
        <uri>https://orcid.org/0000-0003-3602-3629</uri>
      </author>
      <author>
        <name>Gregor, Nicholas</name>
      </author>
      <author>
        <name>Abrahamson, Norman</name>
      </author>
      <author>
        <name>Al Atik, Linda</name>
      </author>
      <author>
        <name>Cabas, Ashly</name>
      </author>
      <author>
        <name>Campbell, Kenneth W</name>
      </author>
      <author>
        <name>Martinez Cruzado, Jose A</name>
      </author>
      <author>
        <name>Pezeshk, Shahram</name>
      </author>
      <author>
        <name>Seyhan, Emel</name>
      </author>
    </item>
    <item>
      <title>Evaluation of Vertical Seismic Load Effects Specified in the United States Building Code</title>
      <link>https://escholarship.org/uc/item/71s9j3nz</link>
      <description>This study evaluates the efficacy of two alternative methods for estimating vertical seismic load effects (Ev), which are specified in United States building codes (e.g., ASCE 7-22) and guidelines, and employed in the seismic design of structures. In both approaches, the vertical seismic load is computed as a percentage of the nominal dead load. One method uses 20% of the horizontal short-period design spectral acceleration (SDS) as the dead load factor, while the other computes the dead load factor as 30% of the vertical spectral acceleration value at the (vertical) structural period of interest (Sav). The two approaches are evaluated and compared using (1) the results of probabilistic seismic hazard analysis carried out by the USGS (which is the backbone data for ASCE 7-22) for 19,316 sites in California, and (2) the NGA-West2 ground motion models for over 3,000 seismic scenarios. The results are presented in terms of the probability distribution of the ratio of the Ev values...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/71s9j3nz</guid>
      <pubDate>Wed, 5 Nov 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Bolourani, Anahita</name>
      </author>
      <author>
        <name>Burton, Henry V</name>
      </author>
      <author>
        <name>Bozorgnia, Yousef</name>
        <uri>https://orcid.org/0000-0003-1773-2489</uri>
      </author>
    </item>
    <item>
      <title>Nonlinear Structural Model Parameter Updating Using Residual Drift Measurements from Sequential Seismic Events</title>
      <link>https://escholarship.org/uc/item/492485bh</link>
      <description>Model parameter updating can enhance the use of nonlinear structural response simulation to guide decision-making in the postearthquake environment. Since most structures in high seismic regions are not instrumented with sensors, the response history during ground shaking is usually not available after an earthquake. Nevertheless, technologies such as Light Detection and Ranging (LiDAR) and drone-mounted imaging devices have made it possible to more effectively measure residual deformations after the shaking has subsided. It is within this context that a framework for performing nonlinear structural model parameter updating based only on residual drift measurements is proposed. The considered setting is one where a structure is subjected to a sequence of ground motions (without repairs), whereby after each event, the structural model parameters are updated using a Bayesian formulation and the measured residual drift. The methodology is demonstrated by using experimental data from...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/492485bh</guid>
      <pubDate>Wed, 5 Nov 2025 00:00:00 +0000</pubDate>
      <author>
        <name>De, Budhaditya</name>
      </author>
      <author>
        <name>Burton, Henry V</name>
      </author>
    </item>
    <item>
      <title>Preliminary Ergodic Site Response Model for California Conditioned on mHVSR</title>
      <link>https://escholarship.org/uc/item/1ht67955</link>
      <description>Traditional ergodic ground motion models (GMMs), typically conditioned on the time-averaged shear-wave velocity in the upper 30 m of soil (VS30), exhibit high site-to-site variability due to their inability to capture site-specific features such as resonances caused by impedance contrasts. Microtremor-based horizontal-to-vertical spectral ratios (mHVSR), which can contain peaks linked to site resonances, offer a useful supplement to VS30 for site response prediction. We use peak features from mHVSR spectra from 685 sites across California and neighboring regions (e.g., Nevada, Oregon) to develop mHVSR-conditioned site response models, which reduce site-to-site variability compared to a baseline linear site amplification model.</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/1ht67955</guid>
      <pubDate>Fri, 10 Oct 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Ornelas, Javier</name>
      </author>
      <author>
        <name>de la Torre, Christopher A</name>
      </author>
      <author>
        <name>Buckreis, Tristan</name>
      </author>
      <author>
        <name>Nweke, Chukwuebuka C</name>
      </author>
      <author>
        <name>Brandenberg, Scott J</name>
      </author>
      <author>
        <name>Stewart, Jonathan P</name>
        <uri>https://orcid.org/0000-0003-3602-3629</uri>
      </author>
    </item>
    <item>
      <title>Not just PAH3.3: Why galaxies turn red in the near-infrared</title>
      <link>https://escholarship.org/uc/item/6m52s4n8</link>
      <description>We measured the spectral properties of a sample of 20 galaxies at z ∼ 0.35 selected for having surprisingly red JWST/NIRCAM F200W-F444W colors. Of these, 19 galaxies were observed with JWST/NIRSpec in the PRISM configuration, while the remaining galaxy was observed with the high-resolution gratings. Of the 20 galaxies in our sample, 17 exhibit strong 3.3 μm polycyclic aromatic hydrocarbon (PAH) emission (equivalent width (EW) (PAH3.3) ≥ 0.03 μm). In these galaxies, the strength of the color excess does not depend on environment and correlates with EW(PAH3.3). Nonetheless, the presence of the PAH3.3 alone cannot fully explain the color excess, as an EW of ∼0.1 μm is able to increase the color of galaxies by only 0.13 mag. A contribution from a hot dust component is required to explain the excess. Both the PAH3.3 EW and flux correlate with the Hα EW and flux, suggesting that they are produced by the same mechanism. Five of the galaxies of our sample showing PAH3.3 would be classified...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/6m52s4n8</guid>
      <pubDate>Wed, 8 Oct 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Vulcani, Benedetta</name>
      </author>
      <author>
        <name>Treu, Tommaso</name>
        <uri>https://orcid.org/0000-0002-8460-0390</uri>
      </author>
      <author>
        <name>Malkan, Matthew</name>
        <uri>https://orcid.org/0000-0001-6919-1237</uri>
      </author>
      <author>
        <name>Lai, Thomas S-Y</name>
      </author>
      <author>
        <name>Calabrò, Antonello</name>
      </author>
      <author>
        <name>Castellano, Marco</name>
      </author>
      <author>
        <name>Napolitano, Lorenzo</name>
      </author>
      <author>
        <name>Mascia, Sara</name>
      </author>
      <author>
        <name>Poggianti, Bianca M</name>
      </author>
      <author>
        <name>Santini, Paola</name>
      </author>
      <author>
        <name>Fritz, Jacopo</name>
      </author>
      <author>
        <name>Metha, Benjamin</name>
      </author>
      <author>
        <name>Yoon, Ilsang</name>
      </author>
      <author>
        <name>Wang, Xin</name>
        <uri>https://orcid.org/0009-0006-8812-5175</uri>
      </author>
    </item>
    <item>
      <title>JWST NIRSpec Spectroscopy of the Remarkable Bright Galaxy GHZ2/GLASS-z12 at Redshift 12.34</title>
      <link>https://escholarship.org/uc/item/4cq166f2</link>
      <description>We spectroscopically confirm the M UV = −20.5 mag galaxy GHZ2/GLASS-z12 to be at redshift z = 12.34. The source was selected via NIRCam photometry in GLASS-JWST Early Release Science data, providing the first evidence of a surprising abundance of bright galaxies at z ≳ 10. The NIRSpec PRISM spectrum shows detections of N iv, C iv, He ii, O iii, C iii, O ii, and Ne iii lines and the first detection at high redshift of the O iii Bowen fluorescence line at 3133 Å rest frame. The prominent C iv line with rest-frame equivalent width (EW) ≈ 46 Å puts GHZ2 in the category of extreme C iv emitters. GHZ2 displays UV lines with EWs that are only found in active galactic nuclei (AGNs) or composite objects at low/intermediate redshifts. The UV line-intensity ratios are compatible with both AGNs and star formation in a low-metallicity environment, with the low limit on the [Ne iv]/[N iv] ratio favoring a stellar origin of the ionizing photons. We discuss a possible scenario in which the high...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/4cq166f2</guid>
      <pubDate>Wed, 8 Oct 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Castellano, Marco</name>
      </author>
      <author>
        <name>Napolitano, Lorenzo</name>
      </author>
      <author>
        <name>Fontana, Adriano</name>
      </author>
      <author>
        <name>Roberts-Borsani, Guido</name>
      </author>
      <author>
        <name>Treu, Tommaso</name>
        <uri>https://orcid.org/0000-0002-8460-0390</uri>
      </author>
      <author>
        <name>Vanzella, Eros</name>
      </author>
      <author>
        <name>Zavala, Jorge A</name>
      </author>
      <author>
        <name>Haro, Pablo Arrabal</name>
      </author>
      <author>
        <name>Calabrò, Antonello</name>
      </author>
      <author>
        <name>Llerena, Mario</name>
      </author>
      <author>
        <name>Mascia, Sara</name>
      </author>
      <author>
        <name>Merlin, Emiliano</name>
      </author>
      <author>
        <name>Paris, Diego</name>
      </author>
      <author>
        <name>Pentericci, Laura</name>
      </author>
      <author>
        <name>Santini, Paola</name>
      </author>
      <author>
        <name>Bakx, Tom JLC</name>
      </author>
      <author>
        <name>Bergamini, Pietro</name>
      </author>
      <author>
        <name>Cupani, Guido</name>
      </author>
      <author>
        <name>Dickinson, Mark</name>
      </author>
      <author>
        <name>Filippenko, Alexei V</name>
        <uri>https://orcid.org/0000-0003-3460-0103</uri>
      </author>
      <author>
        <name>Glazebrook, Karl</name>
      </author>
      <author>
        <name>Grillo, Claudio</name>
      </author>
      <author>
        <name>Kelly, Patrick L</name>
      </author>
      <author>
        <name>Malkan, Matthew A</name>
        <uri>https://orcid.org/0000-0001-6919-1237</uri>
      </author>
      <author>
        <name>Mason, Charlotte A</name>
      </author>
      <author>
        <name>Morishita, Takahiro</name>
      </author>
      <author>
        <name>Nanayakkara, Themiya</name>
      </author>
      <author>
        <name>Rosati, Piero</name>
      </author>
      <author>
        <name>Sani, Eleonora</name>
      </author>
      <author>
        <name>Wang, Xin</name>
        <uri>https://orcid.org/0009-0006-8812-5175</uri>
      </author>
      <author>
        <name>Yoon, Ilsang</name>
      </author>
    </item>
    <item>
      <title>Emission-line galaxies at z ∼ 1 from near-IR HST slitless spectroscopy: metallicities, star formation rates, and redshift confirmations from VLT/FORS2 spectroscopy</title>
      <link>https://escholarship.org/uc/item/30c5x3pc</link>
      <description>We follow up emission line galaxies identified through the near-infrared slitless HST/WFC3 WISP survey with VLT/FORS2 optical spectroscopy. Over 4 WISP fields, we targeted 85 of 138 line emission objects at 0.4 &amp;lt; z &amp;lt; 2 identified in WFC3 spectroscopy. Half the galaxies are fainter than HAB = 24 mag, and would not have been included in many well-known surveys based on broad-band magnitude selection. We confirm 95 per cent of the initial WFC3 grism redshifts in the 38 cases where we detect lines in FORS2 spectroscopy. However, for targets which exhibited a single emission line in WFC3, up to 65 per cent at z &amp;lt; 1.28 did not have expected emission lines detected in FORS2 and hence may be spurious (although this false-detection rate improves to 33 per cent using the latest public WISP emission line catalogue). From the Balmer decrement, the extinction of the WISP galaxies is consistent with A(H α) = 1 mag. From SED fits to multiband photometry including Spitzer 3.6 μm, we...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/30c5x3pc</guid>
      <pubDate>Wed, 8 Oct 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Boyett, K</name>
      </author>
      <author>
        <name>Bunker, AJ</name>
      </author>
      <author>
        <name>Chevallard, J</name>
      </author>
      <author>
        <name>Battisti, A</name>
      </author>
      <author>
        <name>Henry, AL</name>
      </author>
      <author>
        <name>Wilkins, S</name>
      </author>
      <author>
        <name>Malkan, MA</name>
        <uri>https://orcid.org/0000-0001-6919-1237</uri>
      </author>
      <author>
        <name>Caruana, J</name>
      </author>
      <author>
        <name>Atek, H</name>
      </author>
      <author>
        <name>Baronchelli, I</name>
      </author>
      <author>
        <name>Colbert, J</name>
      </author>
      <author>
        <name>Dai, YS</name>
      </author>
      <author>
        <name>Gardner, Jonathan P</name>
      </author>
      <author>
        <name>Rafelski, M</name>
      </author>
      <author>
        <name>Scarlata, C</name>
      </author>
      <author>
        <name>Teplitz, HI</name>
      </author>
      <author>
        <name>Wang, X</name>
        <uri>https://orcid.org/0009-0006-8812-5175</uri>
      </author>
    </item>
    <item>
      <title>Addressing the Needs and Challenges in Evaluating Liquefaction: A Survey of the State-of-Practice</title>
      <link>https://escholarship.org/uc/item/7bn5d3kc</link>
      <description>This paper presents results from a survey investigating the current state-of-practice in liquefaction evaluations. Practitioners completed the survey during presentations of a Next Generation Liquefaction modeling team at local professional society chapters. The survey contained questions on topics within four general categories: site characterization, methods for liquefaction evaluation, approaches to layered and profile-based analyses, and general background information about the survey respondent. Key findings are that (i) practitioners use a wide mix of different site investigation techniques to evaluate liquefaction, (ii) most practitioners in at least some of their projects apply a depth cutoff below which they do not consider liquefaction, (iii) few practitioners modify cone penetration test data based on findings from collocated borings, and (iv) a significant majority apply liquefaction procedures to every layer in the profile rather than identifying and analyzing a critical...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/7bn5d3kc</guid>
      <pubDate>Wed, 1 Oct 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Ulmer, Kristin J</name>
      </author>
      <author>
        <name>Brandenberg, Scott</name>
      </author>
      <author>
        <name>Hudson, Kenneth S</name>
      </author>
      <author>
        <name>Zimmaro, Paolo</name>
      </author>
      <author>
        <name>Kramer, Steven L</name>
      </author>
      <author>
        <name>Stewart, Jonathan P</name>
        <uri>https://orcid.org/0000-0003-3602-3629</uri>
      </author>
    </item>
    <item>
      <title>A decade of DesignSafe: enabling open science in natural hazards</title>
      <link>https://escholarship.org/uc/item/8806364n</link>
      <description>A decade of DesignSafe: enabling open science in natural hazards</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/8806364n</guid>
      <pubDate>Thu, 11 Sep 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Rathje, Ellen M</name>
      </author>
      <author>
        <name>Kumar, Krishna</name>
      </author>
      <author>
        <name>Esteva, Maria</name>
      </author>
      <author>
        <name>Brandenberg, Scott J</name>
      </author>
      <author>
        <name>Cockerill, Tim</name>
      </author>
      <author>
        <name>Dawson, Clint</name>
      </author>
      <author>
        <name>Padgett, Jamie E</name>
      </author>
      <author>
        <name>Pinelli, Jean-Paul</name>
      </author>
      <author>
        <name>Stanzione, Dan</name>
      </author>
    </item>
    <item>
      <title>Engineering attributes of ground motions from February 2023 Türkiye earthquake sequence</title>
      <link>https://escholarship.org/uc/item/3n2686p5</link>
      <description>The 2023 Türkiye earthquake sequence includes the 6 February M7.81 mainshock followed approximately 9 h later by an M7.74 event, and many smaller aftershocks including M6.81 and M6.37 events on 6 and 20 February, respectively. These events occurred in a region near the plate boundary of the East Anatolian Fault, in the proximity of which numerous ground motion recording stations had been installed north of the Türkiye–Syria border. As a result, the events were well recorded both near the fault and at rupture distances up to 582 km. We describe the available recordings and component-specific data processing performed with the aim of optimizing usable bandwidth. The resulting database includes 337, 365, 284, and 229 usable three-component recordings from the M7.81, M7.74, M6.81, and M6.37 events, respectively. We also present source, path, and site metadata that were compiled according to uniform protocols. Comparisons to a global ground motion model (GMM) for active tectonic regions...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/3n2686p5</guid>
      <pubDate>Thu, 11 Sep 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Buckreis, Tristan E</name>
      </author>
      <author>
        <name>Pretell, Renmin</name>
      </author>
      <author>
        <name>Sandikkaya, M Abdullah</name>
      </author>
      <author>
        <name>Kale, Özkan</name>
      </author>
      <author>
        <name>Askan, Aysegul</name>
      </author>
      <author>
        <name>Brandenberg, Scott J</name>
      </author>
      <author>
        <name>Stewart, Jonathan P</name>
        <uri>https://orcid.org/0000-0003-3602-3629</uri>
      </author>
    </item>
    <item>
      <title>Proxy-Based VS30 Estimation for Utah Conditioned on Surface Geology and Surface Gradient</title>
      <link>https://escholarship.org/uc/item/4rp0w60h</link>
      <description>The shear-wave velocity profile database was augmented with 259 profiles from 205 unique sites in Utah to facilitate the assignment of site parameters for 95 ground motion recording sites in this region as part of the NGA-West3 project. Three profiles were paired with Utah ground motion stations but 92 other stations lack a co-located profile. A proxy-based model to predict the time-averaged velocity in the upper 30 m of the site (VS30) was developed that considers surface geology and surface gradient for Quaternary units in Utah. The Quaternary surface geologic units considered are Holocene alluvium (Ha), fill (Hf), Pleistocene or undifferentiated Quaternary alluvium (Pa/Qal), alluvium/deltaic (Pad), deltaic (Pd), deltaic-lacustrine or lacustrine (Pdl/Pl), glacial (Pg), undifferentiated Quaternary alluvium - deltaic - eolian (Qa/Qdel/Qe), undifferentiated Quaternary alluvium/deltatic/lacustrine and Holocene deltaic/lacustrine (Qalm/Qdl/Hdl), and lacustrine (Ql). For each unit,...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/4rp0w60h</guid>
      <pubDate>Sat, 6 Sep 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Choi, Joseph</name>
      </author>
      <author>
        <name>Stewart, Jonathan P</name>
        <uri>https://orcid.org/0000-0003-3602-3629</uri>
      </author>
      <author>
        <name>Buckreis, Tristan</name>
      </author>
      <author>
        <name>Brandenberg, Scott</name>
      </author>
    </item>
    <item>
      <title>Ground-motion models for inelastic response spectra using NGA-West2 database</title>
      <link>https://escholarship.org/uc/item/80v3g7gp</link>
      <description>This article presents ground-motion models (GMMs) for inelastic response spectra using the NGA-West2 database. The inelastic response spectra are defined in terms of constant ductility. The GMMs are used to observe the effect of event scenarios, site conditions, and oscillator properties on maximum displacement. Using a large database enabled us to quantify the magnitude scaling of inelastic response as compared to that for the traditional elastic GMMs. We observe that using the magnitude scaling of elastic GMM for hazard analysis of inelastic structural response can be unconservative for large magnitudes and large ductility ratios. To compare our models with models in the literature, we use the developed GMMs to compute the Reduction Factor due to inelasticity. Comparison of this model with models in the literature shows the importance of considering the effect of magnitude on the Reduction Factor. We also observe that the ratio of RotD100/RotD50 is larger for inelastic single-degree-of-freedom...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/80v3g7gp</guid>
      <pubDate>Wed, 27 Aug 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Bahrampouri, Mahdi</name>
      </author>
      <author>
        <name>Bozorgnia, Yousef</name>
        <uri>https://orcid.org/0000-0003-1773-2489</uri>
      </author>
      <author>
        <name>Campbell, Kenneth W</name>
      </author>
      <author>
        <name>Mazzoni, Silvia</name>
      </author>
    </item>
    <item>
      <title>Response of BART’s Berkeley Hills tunnel to fault displacement and impact on system functionality</title>
      <link>https://escholarship.org/uc/item/5h99s64q</link>
      <description>Response of BART’s Berkeley Hills tunnel to fault displacement and impact on system functionality</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/5h99s64q</guid>
      <pubDate>Wed, 27 Aug 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Zengin, Esra</name>
      </author>
      <author>
        <name>Bozorgnia, Yousef</name>
        <uri>https://orcid.org/0000-0003-1773-2489</uri>
      </author>
      <author>
        <name>Stewart, Jonathan P</name>
        <uri>https://orcid.org/0000-0003-3602-3629</uri>
      </author>
    </item>
    <item>
      <title>Fault Displacement Hazard Initiative research program</title>
      <link>https://escholarship.org/uc/item/1905b9gz</link>
      <description>Fault Displacement Hazard Initiative research program</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/1905b9gz</guid>
      <pubDate>Wed, 27 Aug 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Bozorgnia, Yousef</name>
        <uri>https://orcid.org/0000-0003-1773-2489</uri>
      </author>
      <author>
        <name>Abrahamson, Norman</name>
      </author>
      <author>
        <name>Baize, Stéphane</name>
      </author>
      <author>
        <name>Boncio, Paolo</name>
      </author>
      <author>
        <name>Chen, Rui</name>
      </author>
      <author>
        <name>Chiou, Brian</name>
      </author>
      <author>
        <name>Dawson, Timothy</name>
      </author>
      <author>
        <name>Kottke, Albert</name>
      </author>
      <author>
        <name>Kuehn, Nicolas</name>
      </author>
      <author>
        <name>Lavrentiadis, Grigorios</name>
      </author>
      <author>
        <name>Madugo, Christopher</name>
      </author>
      <author>
        <name>Madugo, Danielle</name>
      </author>
      <author>
        <name>Milliner, Christopher</name>
      </author>
      <author>
        <name>Moss, Robb</name>
      </author>
      <author>
        <name>Nurminen, Fiia</name>
      </author>
      <author>
        <name>Sarmiento, Alexandra</name>
      </author>
      <author>
        <name>Thomas, Kate</name>
      </author>
      <author>
        <name>Thompson, Stephen</name>
      </author>
      <author>
        <name>Valentini, Alessandro</name>
      </author>
      <author>
        <name>Visini, Francesco</name>
      </author>
      <author>
        <name>Zandieh, Arash</name>
      </author>
    </item>
    <item>
      <title>Residual displacement ground-motion model</title>
      <link>https://escholarship.org/uc/item/06s747mx</link>
      <description>Residual displacement ground-motion model</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/06s747mx</guid>
      <pubDate>Wed, 27 Aug 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Zengin, Esra</name>
      </author>
      <author>
        <name>Bozorgnia, Yousef</name>
        <uri>https://orcid.org/0000-0003-1773-2489</uri>
      </author>
      <author>
        <name>Mazzoni, Silvia</name>
      </author>
      <author>
        <name>Campbell, Kenneth</name>
      </author>
    </item>
    <item>
      <title>A Global Application Programming Interface–Enabled Earthquake Ground Motion Relational Database for Engineering Applications</title>
      <link>https://escholarship.org/uc/item/3707d79n</link>
      <description>We present a application programming interface (API)-enabled relational database of global earthquake ground motion intensity measures, associated metadata, and processed time-series data. Raw ground motion records were processed by the authors using either manual or semi-automated processing procedures, and every processed record has passed a quality review by a trained analyst. Computed intensity measures include peak acceleration and velocity, pseudo-spectral acceleration response spectra, cumulative absolute velocity, Arias Intensity, and Fourier amplitude spectra. The processed time-series data, associated metadata, and ground motion intensity measures were organized into a web-served relational database consisting of 32 tables connected by primary/foreign key pairs. Ground motion metadata and intensity measures (but not time-series) from the Next-Generation Attenuation (NGA)-East and NGA-West2 projects and the Hellenic Strong-Motion Database are also contained in the database....</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/3707d79n</guid>
      <pubDate>Thu, 14 Aug 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Buckreis, Tristan E</name>
      </author>
      <author>
        <name>Nweke, Chukwuebuka C</name>
      </author>
      <author>
        <name>Wang, Pengfei</name>
      </author>
      <author>
        <name>Brandenberg, Scott J</name>
      </author>
      <author>
        <name>Ramos-Sepúlveda, Maria E</name>
      </author>
      <author>
        <name>Shams, Rashid</name>
      </author>
      <author>
        <name>Mohammed, Shako</name>
      </author>
      <author>
        <name>Pretell, Renmin</name>
      </author>
      <author>
        <name>Mazzoni, Silvia</name>
      </author>
      <author>
        <name>Zimmaro, Paolo</name>
      </author>
      <author>
        <name>Stewart, Jonathan P</name>
        <uri>https://orcid.org/0000-0003-3602-3629</uri>
      </author>
    </item>
    <item>
      <title>Analysis of Near-Surface Shear Wave Velocity Data for Site Response Applications in the Sacramento- San Joaquin Delta Region of California</title>
      <link>https://escholarship.org/uc/item/2mb8n5p9</link>
      <description>Analysis of Near-Surface Shear Wave Velocity Data for Site Response Applications in the Sacramento- San Joaquin Delta Region of California</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/2mb8n5p9</guid>
      <pubDate>Thu, 14 Aug 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Buckreis, Tristan E</name>
      </author>
      <author>
        <name>Wang, Pengfei</name>
      </author>
      <author>
        <name>Stewart, Jonathan P</name>
        <uri>https://orcid.org/0000-0003-3602-3629</uri>
      </author>
      <author>
        <name>Brandenberg, Scott J</name>
      </author>
      <author>
        <name>Driller, Michael M</name>
      </author>
    </item>
    <item>
      <title>Next Generation Liquefaction Laboratory Database for Susceptibility and Cyclic Strength Assessment</title>
      <link>https://escholarship.org/uc/item/5wb104pw</link>
      <description>Next Generation Liquefaction Laboratory Database for Susceptibility and Cyclic Strength Assessment</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/5wb104pw</guid>
      <pubDate>Wed, 9 Jul 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Sahin, Arda</name>
      </author>
      <author>
        <name>Jana, Amalesh</name>
      </author>
      <author>
        <name>Beyzaei, Christine Z</name>
      </author>
      <author>
        <name>Sancio, Rodolfo</name>
      </author>
      <author>
        <name>Ulmer, Kristin J</name>
      </author>
      <author>
        <name>Brandenberg, Scott J</name>
      </author>
      <author>
        <name>Kramer, Steven L</name>
      </author>
      <author>
        <name>Stewart, Jonathan P</name>
      </author>
      <author>
        <name>Stuedlein, Armin W</name>
      </author>
    </item>
    <item>
      <title>Reliability-based quantification of the benefits of machine learning predictive models in seismic structural design and performance assessment</title>
      <link>https://escholarship.org/uc/item/2fr4r5pn</link>
      <description>Reliability-based quantification of the benefits of machine learning predictive models in seismic structural design and performance assessment</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/2fr4r5pn</guid>
      <pubDate>Thu, 24 Apr 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Aladsani, Muneera A</name>
      </author>
      <author>
        <name>Burton, Henry V</name>
      </author>
    </item>
    <item>
      <title>Evaluation of a modified IDEXX method for antimicrobial resistance monitoring of extended Beta-lactamases-producing Escherichia coli in impacted waters near the U.S.-Mexico border</title>
      <link>https://escholarship.org/uc/item/5nq3h61w</link>
      <description>As part of a One Health approach, the World Health Organization (WHO) has deemed extended beta-lactamases-producing &lt;i&gt;Escherichia coli&lt;/i&gt; (ESBL-Ec) as an appropriate proxy for antimicrobial resistance (AMR) in human, animal, and environmental samples. Traditional methods for ESBL-Ec quantification involve a labor-intensive process of membrane filtration, culturing in the presence and absence of antibiotics, and colony confirmation. The emerging modified IDEXX method utilizes IDEXX Colilert-18 test kits, recognized by the USEPA for the enumeration of total coliforms and &lt;i&gt;E. coli&lt;/i&gt; in water samples, modified with cefotaxime for measurement of ESBL-Ec in environmental samples. However, this method has yet to be validated for ocean or sewage-contaminated water and has not been compared against the plate-based method with mTEC for surface water. In this study, ESBL-Ec in ocean and river waters of the Tijuana River Estuary were analyzed by three methods: membrane filtration using...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/5nq3h61w</guid>
      <pubDate>Wed, 26 Mar 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Jimenez, Karina</name>
      </author>
      <author>
        <name>Kong, Yuwei</name>
        <uri>https://orcid.org/0009-0004-3703-7891</uri>
      </author>
      <author>
        <name>Zhang, Yuhui</name>
      </author>
      <author>
        <name>Ferketic, Drew</name>
      </author>
      <author>
        <name>Nagori, Sana K</name>
      </author>
      <author>
        <name>Yang, Julie</name>
      </author>
      <author>
        <name>Yulo, Anastasia A</name>
      </author>
      <author>
        <name>Kramer, Brianna</name>
      </author>
      <author>
        <name>Prado, Ofelia G</name>
      </author>
      <author>
        <name>Cason, Taylor</name>
      </author>
      <author>
        <name>Chowdhry, Renee</name>
      </author>
      <author>
        <name>Kemsley, Angela</name>
      </author>
      <author>
        <name>Espinosa, Leopoldo Mendoza</name>
      </author>
      <author>
        <name>Steele, Joshua A</name>
      </author>
      <author>
        <name>Griffith, John</name>
      </author>
      <author>
        <name>Jay, Jennifer A</name>
      </author>
    </item>
    <item>
      <title>Monitoring Coastal Water Turbidity Using Sentinel2—A Case Study in Los Angeles</title>
      <link>https://escholarship.org/uc/item/0pw3j7bt</link>
      <description>Los Angeles coastal waters are an ecologically important marine habitat and a famed recreational area for tourists. Constant surveillance is essential to ensure compliance with established health standards and to address the persistent water quality challenges in the region. Remotely sensed datasets are increasingly being applied toward improved detection of water quality by augmenting monitoring programs with spatially intensive and accessible data. This study evaluates the potential of satellite remote sensing to augment traditional monitoring by analyzing the relationship between in situ and satellite-derived turbidity data. Field measurements were performed from July 2021 to March 2024 to build synchronous matchup datasets consisting of satellite and field data. Correlation analysis indicated a positive relationship between satellite-derived and field-measured turbidity (R2 = 0.451). Machine learning models were assessed for predictive accuracy, with the random forest model...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/0pw3j7bt</guid>
      <pubDate>Wed, 26 Mar 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Kong, Yuwei</name>
      </author>
      <author>
        <name>Jimenez, Karina</name>
      </author>
      <author>
        <name>Lee, Christine M</name>
      </author>
      <author>
        <name>Winter, Sophia</name>
      </author>
      <author>
        <name>Summers-Evans, Jasmine</name>
      </author>
      <author>
        <name>Cao, Albert</name>
      </author>
      <author>
        <name>Menczer, Massimiliano</name>
      </author>
      <author>
        <name>Han, Rachel</name>
      </author>
      <author>
        <name>Mills, Cade</name>
      </author>
      <author>
        <name>McCarthy, Savannah</name>
      </author>
      <author>
        <name>Blatzheim, Kierstin</name>
      </author>
      <author>
        <name>Jay, Jennifer A</name>
      </author>
    </item>
    <item>
      <title>Implications of Pyrolytic Gas Dynamic Evolution on Dissolved Black Carbon Formed During Production of Biochar from Nitrogen-Rich Feedstock</title>
      <link>https://escholarship.org/uc/item/17q9867f</link>
      <description>Gases and dissolved black carbon (DBC) formed during pyrolysis of nitrogen-rich feedstock would affect atmospheric and aquatic environments. Yet, the mechanisms driving biomass gas evolution and DBC formation are poorly understood. Using thermogravimetric-Fourier transform infrared spectrometry and two-dimensional correlation spectroscopy, we correlated the temperature-dependent primary noncondensable gas release sequence (H&lt;sub&gt;2&lt;/sub&gt;O → CO&lt;sub&gt;2&lt;/sub&gt; → HCN, NH&lt;sub&gt;3&lt;/sub&gt; → CH&lt;sub&gt;4&lt;/sub&gt; → CO) with specific defunctionalization stages in the order: dehydration, decarboxylation, denitrogenation, demethylation, and decarbonylation. Our results revealed that proteins in feedstock mainly contributed to gas releases, and low-volatile pyrolytic products contributed to DBC. Combining mass difference analysis with Fourier transform ion cyclotron resonance mass spectrometry, we showed that 44-60% of DBC molecular compositions were correlated with primary gas-releasing reactions. Dehydration...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/17q9867f</guid>
      <pubDate>Thu, 27 Feb 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Zhang, Xiaoxiao</name>
      </author>
      <author>
        <name>Xu, Zibo</name>
      </author>
      <author>
        <name>Sun, Yuqing</name>
      </author>
      <author>
        <name>Mohanty, Sanjay K</name>
      </author>
      <author>
        <name>Lei, Hanwu</name>
      </author>
      <author>
        <name>Khan, Eakalak</name>
      </author>
      <author>
        <name>Tsang, Daniel CW</name>
      </author>
    </item>
    <item>
      <title>Spatial distribution of damage potential of the 2023 Pazarcik Turkey earthquake using inelastic-response spectra of recorded and simulated ground motions</title>
      <link>https://escholarship.org/uc/item/5xn5p9dt</link>
      <description>On 6 February 2023, a devastating earthquake of magnitude 7.7 struck the southeastern part of Turkey, followed by multiple aftershocks. The sequence of earthquakes caused extensive damage in Southern Turkey and Northern Syria. This study evaluates the destructive potential of ground shaking resulting from the Pazarcik mainshock by developing spatial distribution of inelastic demand spectra across the region by using the recorded ground motions. These spectra provide an additional step toward more realistic estimates of the damage potential of ground shaking than the traditional elastic response spectra. Given the recorded ground motions, we also developed simulated ground-motion time series at numerous un-instrumented sites. We used these recorded and simulated motions to estimate ductility demands across the affected area. Constant-ductility spectra were derived using recording stations within 100 km of the fault rupture. The results indicated that in the near-fault area, and...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/5xn5p9dt</guid>
      <pubDate>Wed, 26 Feb 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Zengin, Esra</name>
      </author>
      <author>
        <name>Bozorgnia, Yousef</name>
        <uri>https://orcid.org/0000-0003-1773-2489</uri>
      </author>
      <author>
        <name>Tamhidi, Aidin</name>
      </author>
      <author>
        <name>Mazzoni, Silvia</name>
      </author>
    </item>
    <item>
      <title>Mitigating CaCO3 crystal nucleation and growth through continuous ion displacement via alternating electric fields</title>
      <link>https://escholarship.org/uc/item/7x65t4q4</link>
      <description>Mineral crystal formation poses a challenge on surfaces (e.g., heat exchangers, pipes, membranes, etc.) in contact with super-saturated fluids. Applying alternating currents (AC) to such surfaces can prevent surface crystallization under certain conditions. Here, we demonstrate that ion displacement induced by periodic charging and discharging of the electrical double layer (EDL) inhibits both heterogeneous and homogeneous nucleation (and crystal growth) of CaCO3. Titanium sheets (meant to simulate metallic heat exchanger surfaces) are immersed in super-saturated CaCO3 solutions with a saturation index &amp;gt;11. We show that at relatively high AC frequencies, incomplete EDL formation leads to an alternating electric field that propagates far into the bulk solution, inducing rapid ion migration that overwhelms the Brownian motion of ions. Electrochemical characterization reveals EDL charging/discharging under AC conditions that greatly inhibits precipitation. Operating at 4 Vpp,...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/7x65t4q4</guid>
      <pubDate>Mon, 20 Jan 2025 00:00:00 +0000</pubDate>
      <author>
        <name>Liu, Yiming</name>
      </author>
      <author>
        <name>Xiao, Minhao</name>
      </author>
      <author>
        <name>Huang, Xiaochuan</name>
      </author>
      <author>
        <name>Park, Jane</name>
      </author>
      <author>
        <name>Hoffman, Matthew E</name>
      </author>
      <author>
        <name>Feng, Yuren</name>
      </author>
      <author>
        <name>An, Alicia Kyoungjin</name>
      </author>
      <author>
        <name>Li, Qilin</name>
      </author>
      <author>
        <name>Hoek, Eric MV</name>
        <uri>https://orcid.org/0000-0002-9674-1916</uri>
      </author>
      <author>
        <name>Jassby, David</name>
      </author>
    </item>
    <item>
      <title>An Integrated Framework for Infectious Disease Control Using Mathematical Modeling and Deep Learning</title>
      <link>https://escholarship.org/uc/item/3cr2m7kz</link>
      <description>Infectious diseases are a major global public health concern. Precise modeling and prediction methods are essential to develop effective strategies for disease control. However, data imbalance and the presence of noise and intensity inhomogeneity make disease detection more challenging. &lt;i&gt;Goal:&lt;/i&gt; In this article, a novel infectious disease pattern prediction system is proposed by integrating deterministic and stochastic model benefits with the benefits of the deep learning model. &lt;i&gt;Results:&lt;/i&gt; The combined benefits yield improvement in the performance of solution prediction. Moreover, the objective is also to investigate the influence of time delay on infection rates and rates associated with vaccination. &lt;i&gt;Conclusions:&lt;/i&gt; In this proposed framework, at first, the global stability at disease free equilibrium is effectively analysed using Routh-Haurwitz criteria and Lyapunov method, and the endemic equilibrium is analysed using non-linear Volterra integral equations in the...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/3cr2m7kz</guid>
      <pubDate>Mon, 16 Dec 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Salman, Mohammed</name>
      </author>
      <author>
        <name>Das, Pradeep Kumar</name>
      </author>
      <author>
        <name>Mohanty, Sanjay Kumar</name>
      </author>
    </item>
    <item>
      <title>NUMOSIM: A Synthetic Mobility Dataset with Anomaly Detection Benchmarks</title>
      <link>https://escholarship.org/uc/item/7h88t1wf</link>
      <description>NUMOSIM: A Synthetic Mobility Dataset with Anomaly Detection Benchmarks</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/7h88t1wf</guid>
      <pubDate>Thu, 5 Dec 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Stanford, Chris</name>
      </author>
      <author>
        <name>Adari, Suman</name>
      </author>
      <author>
        <name>Liao, Xishun</name>
        <uri>https://orcid.org/0000-0002-7219-8971</uri>
      </author>
      <author>
        <name>He, Yueshuai</name>
      </author>
      <author>
        <name>Jiang, Qinhua</name>
      </author>
      <author>
        <name>Kuai, Chenchen</name>
      </author>
      <author>
        <name>Ma, Jiaqi</name>
        <uri>https://orcid.org/0000-0002-8184-5157</uri>
      </author>
      <author>
        <name>Tung, Emmanuel</name>
      </author>
      <author>
        <name>Qian, Yinlong</name>
      </author>
      <author>
        <name>Zhao, Lingyi</name>
      </author>
      <author>
        <name>Zhou, Zihao</name>
      </author>
      <author>
        <name>Rasheed, Zeeshan</name>
      </author>
      <author>
        <name>Shafique, Khurram</name>
      </author>
    </item>
    <item>
      <title>ZeroCAL: Eliminating Carbon Dioxide Emissions from Limestone’s Decomposition to Decarbonize Cement Production</title>
      <link>https://escholarship.org/uc/item/2qk5w2r8</link>
      <description>Limestone (calcite, CaCO&lt;sub&gt;3&lt;/sub&gt;) is an abundant and cost-effective source of calcium oxide (CaO) for cement and lime production. However, the thermochemical decomposition of limestone (∼800 °C, 1 bar) to produce lime (CaO) results in substantial carbon dioxide (CO&lt;sub&gt;2(g)&lt;/sub&gt;) emissions and energy use, i.e., ∼1 tonne [t] of CO&lt;sub&gt;2&lt;/sub&gt; and ∼1.4 MWh per t of CaO produced. Here, we describe a new pathway to use CaCO&lt;sub&gt;3&lt;/sub&gt; as a Ca source to make hydrated lime (portlandite, Ca(OH)&lt;sub&gt;2&lt;/sub&gt;) at ambient conditions (&lt;i&gt;p&lt;/i&gt;, &lt;i&gt;T&lt;/i&gt;)-while nearly eliminating process CO&lt;sub&gt;2(g)&lt;/sub&gt; emissions (as low as 1.5 mol. % of the CO&lt;sub&gt;2&lt;/sub&gt; in the precursor CaCO&lt;sub&gt;3&lt;/sub&gt;, equivalent to 9 kg of CO&lt;sub&gt;2(g)&lt;/sub&gt; per t of Ca(OH)&lt;sub&gt;2&lt;/sub&gt;)-within an aqueous flow-electrolysis/pH-swing process that coproduces hydrogen (H&lt;sub&gt;2(g)&lt;/sub&gt;) and oxygen (O&lt;sub&gt;2(g)&lt;/sub&gt;). Because Ca(OH)&lt;sub&gt;2&lt;/sub&gt; is a zero-carbon precursor for cement and lime production, this approach...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/2qk5w2r8</guid>
      <pubDate>Mon, 11 Nov 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Leão, Adriano</name>
      </author>
      <author>
        <name>Collin, Marie</name>
      </author>
      <author>
        <name>Ghodkhande, Swarali</name>
      </author>
      <author>
        <name>Bouissonnié, Arnaud</name>
      </author>
      <author>
        <name>Chen, Xin</name>
      </author>
      <author>
        <name>Malin, Benjamin</name>
      </author>
      <author>
        <name>Liu, Yiming</name>
      </author>
      <author>
        <name>Hovey, Geanna</name>
      </author>
      <author>
        <name>Govindhakannan, Jagannathan</name>
      </author>
      <author>
        <name>La Plante, Erika</name>
        <uri>https://orcid.org/0000-0002-5273-9523</uri>
      </author>
      <author>
        <name>Jassby, David</name>
      </author>
      <author>
        <name>Gädt, Torben</name>
      </author>
      <author>
        <name>Corsini, Lorenzo</name>
      </author>
      <author>
        <name>Simonetti, Dante</name>
      </author>
      <author>
        <name>Rosner, Fabian</name>
      </author>
      <author>
        <name>Sant, Gaurav</name>
      </author>
    </item>
    <item>
      <title>The multi-scale damage evolution of nano-modified concrete under the cold region tunnel environment based on micromechanical model</title>
      <link>https://escholarship.org/uc/item/5rt430c7</link>
      <description>The multi-scale damage evolution of nano-modified concrete under the cold region tunnel environment based on micromechanical model</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/5rt430c7</guid>
      <pubDate>Thu, 7 Nov 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Xia, Wei</name>
      </author>
      <author>
        <name>Li, Wei-kang</name>
      </author>
      <author>
        <name>Rao, Jia-rui</name>
      </author>
      <author>
        <name>Jiang, Zong-quan</name>
      </author>
      <author>
        <name>Ju, Jiann-wen Woody</name>
      </author>
      <author>
        <name>Cui, Sheng-ai</name>
      </author>
    </item>
    <item>
      <title>Topological controls on the dissolution kinetics of glassy aluminosilicates</title>
      <link>https://escholarship.org/uc/item/6g30d4sc</link>
      <description>Fly ash which encompasses a mixture of glassy and crystalline aluminosilicates is an abundant supplementary cementitious material (SCM), valuable for replacing ordinary portland cement (OPC) in the binder fraction in concrete. Because higher OPC replacement levels are desired, it is critically important to better understand and quantify fly ash reactivity. By combining molecular dynamics (MD) simulations and vertical scanning interferometry (VSI), this study establishes that the reactivity of the glassy fractions in a fly ash with water (i.e., their aqueous dissolution rate) is controlled by the number of constraints placed on atoms within the disordered aluminosilicate network. More precisely, an Arrhenius-like dependence of dissolution rates on the atomic network topology is observed. Such &lt;i&gt;topological controls&lt;/i&gt; on fly ash reactivity are highlighted for a range of U.S. commercial fly ashes spanning CaO-enriched and SiO&lt;sub&gt;2&lt;/sub&gt;-enriched compositions. The structure-property...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/6g30d4sc</guid>
      <pubDate>Mon, 4 Nov 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Oey, Tandré</name>
      </author>
      <author>
        <name>Kumar, Aditya</name>
      </author>
      <author>
        <name>Pignatelli, Isabella</name>
      </author>
      <author>
        <name>Yu, Yingtian</name>
      </author>
      <author>
        <name>Neithalath, Narayanan</name>
      </author>
      <author>
        <name>Bullard, Jeffrey W</name>
      </author>
      <author>
        <name>Bauchy, Mathieu</name>
        <uri>https://orcid.org/0000-0003-4600-0631</uri>
      </author>
      <author>
        <name>Sant, Gaurav</name>
      </author>
    </item>
    <item>
      <title>Monolithic Polyepoxide Membranes for Nanofiltration Applications and Sustainable Membrane Manufacture</title>
      <link>https://escholarship.org/uc/item/0254j5c7</link>
      <description>The present work details the development of carbon fiber-reinforced epoxy membranes with excellent rejection of small-molecule dyes. It is a proof-of-concept for a more sustainable membrane design incorporating carbon fibers, and their recycling and reuse. 4,4'-methylenebis(cyclohexylamine) (MBCHA) polymerized with either bisphenol-A-diglycidyl ether (BADGE) or tetraphenolethane tetraglycidylether (EPON Resin 1031) in polyethylene glycol (PEG) were used to make monolithic membranes reinforced by nonwoven carbon fibers. Membrane pore sizes were tuned by adjusting the molecular weight of the PEG used in the initial polymerization. Membranes made of BADGE-MBCHA showed rejection of Rose Bengal approaching 100%, while tuning the pore sizes substantially increased the rejection of Methylene Blue from ~65% to nearly 100%. The membrane with the best permselectivity was made of EPON-MBCHA polymerized in PEG 300. It has an average DI flux of 4.48 LMH/bar and an average rejection of 99.6%...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/0254j5c7</guid>
      <pubDate>Wed, 30 Oct 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Anderson, Mackenzie Babetta</name>
      </author>
      <author>
        <name>Danna, Riley A</name>
      </author>
      <author>
        <name>French, Clayton</name>
      </author>
      <author>
        <name>Wu, Jishan</name>
      </author>
      <author>
        <name>Thiel, Markus N</name>
      </author>
      <author>
        <name>Yang, Zhiyin</name>
      </author>
      <author>
        <name>Hoek, Eric MV</name>
        <uri>https://orcid.org/0000-0002-9674-1916</uri>
      </author>
      <author>
        <name>Kaner, Richard B</name>
        <uri>https://orcid.org/0000-0003-0345-4924</uri>
      </author>
    </item>
    <item>
      <title>CEERS: 7.7 μm PAH Star Formation Rate Calibration with JWST MIRI</title>
      <link>https://escholarship.org/uc/item/153092z2</link>
      <description>We test the relationship between UV-derived star formation rates (SFRs) and the 7.7 μm polycyclic aromatic hydrocarbon luminosities from the integrated emission of galaxies at z ∼ 0-2. We utilize multiband photometry covering 0.2-160 μm from the Hubble Space Telescope, CFHT, JWST, Spitzer, and Herschel for galaxies in the Cosmic Evolution Early Release Science (CEERS) Survey. We perform spectral energy distribution (SED) modeling of these data to measure dust-corrected far-UV (FUV) luminosities, L FUV, and UV-derived SFRs. We then fit SED models to the JWST/MIRI 7.7-21 μm CEERS data to derive rest-frame 7.7 μm luminosities, L 770, using the average flux density in the rest-frame MIRI F770W bandpass. We observe a correlation between L 770 and L FUV, where log L 770 ∝ ( 1.27 ± 0.04 ) log L FUV . L 770 diverges from this relation for galaxies at lower metallicities, lower dust obscuration, and for galaxies dominated by evolved stellar populations. We derive a “single-wavelength”...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/153092z2</guid>
      <pubDate>Mon, 28 Oct 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Ronayne, Kaila</name>
      </author>
      <author>
        <name>Papovich, Casey</name>
      </author>
      <author>
        <name>Yang, Guang</name>
      </author>
      <author>
        <name>Shen, Lu</name>
      </author>
      <author>
        <name>Dickinson, Mark</name>
      </author>
      <author>
        <name>Kennicutt, Robert</name>
      </author>
      <author>
        <name>Alavi, Anahita</name>
      </author>
      <author>
        <name>Haro, Pablo Arrabal</name>
      </author>
      <author>
        <name>Bagley, Micaela B</name>
      </author>
      <author>
        <name>Burgarella, Denis</name>
      </author>
      <author>
        <name>Le Bail, Aurélien</name>
        <uri>https://orcid.org/0000-0002-9466-2763</uri>
      </author>
      <author>
        <name>Bell, Eric F</name>
      </author>
      <author>
        <name>Cleri, Nikko J</name>
      </author>
      <author>
        <name>Cole, Justin</name>
      </author>
      <author>
        <name>Costantin, Luca</name>
      </author>
      <author>
        <name>de la Vega, Alexander</name>
      </author>
      <author>
        <name>Daddi, Emanuele</name>
      </author>
      <author>
        <name>Elbaz, David</name>
      </author>
      <author>
        <name>Finkelstein, Steven L</name>
      </author>
      <author>
        <name>Grogin, Norman A</name>
      </author>
      <author>
        <name>Holwerda, Benne W</name>
      </author>
      <author>
        <name>Kartaltepe, Jeyhan S</name>
      </author>
      <author>
        <name>Kirkpatrick, Allison</name>
      </author>
      <author>
        <name>Koekemoer, Anton M</name>
      </author>
      <author>
        <name>Lucas, Ray A</name>
      </author>
      <author>
        <name>Magnelli, Benjamin</name>
      </author>
      <author>
        <name>Mobasher, Bahram</name>
      </author>
      <author>
        <name>Pérez-González, Pablo G</name>
      </author>
      <author>
        <name>Prichard, Laura</name>
      </author>
      <author>
        <name>Rafelski, Marc</name>
      </author>
      <author>
        <name>Rodighiero, Giulia</name>
      </author>
      <author>
        <name>Sunnquist, Ben</name>
      </author>
      <author>
        <name>Teplitz, Harry I</name>
      </author>
      <author>
        <name>Wang, Xin</name>
        <uri>https://orcid.org/0009-0006-8812-5175</uri>
      </author>
      <author>
        <name>Windhorst, Rogier A</name>
      </author>
      <author>
        <name>Yung, LY Aaron</name>
      </author>
    </item>
    <item>
      <title>Proteomics insights into the fungal-mediated bioremediation of environmental contaminants</title>
      <link>https://escholarship.org/uc/item/1913054g</link>
      <description>As anthropogenic activities continue to introduce various contaminants into the environment, the need for effective monitoring and bioremediation strategies is critical. Fungi, with their diverse enzymatic arsenal, offer promising solutions for the biotransformation of many pollutants. While conventional research reports on ligninolytic, oxidoreductive, and cytochrome P450 (CYP) enzymes, the vast potential of fungi, with approximately 10 345 protein sequences per species, remains largely untapped. This review describes recent advancements in fungal proteomics instruments as well as software and highlights their detoxification mechanisms and biochemical pathways. Additionally, it highlights lesser-known fungal enzymes with potential applications in environmental biotechnology. By reviewing the benefits and challenges associated with proteomics tools, we hope to summarize and promote the studies of fungi and fungal proteins relevant in the environment.</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/1913054g</guid>
      <pubDate>Thu, 24 Oct 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Shah, Kshitija</name>
        <uri>https://orcid.org/0009-0003-8509-5714</uri>
      </author>
      <author>
        <name>Ray, Soham</name>
        <uri>https://orcid.org/0009-0006-4443-4822</uri>
      </author>
      <author>
        <name>Bose, Himadri</name>
      </author>
      <author>
        <name>Pandey, Vijaya</name>
        <uri>https://orcid.org/0000-0002-5675-5504</uri>
      </author>
      <author>
        <name>Wohlschlegel, James A</name>
        <uri>https://orcid.org/0000-0001-8289-2222</uri>
      </author>
      <author>
        <name>Mahendra, Shaily</name>
        <uri>https://orcid.org/0000-0003-3298-9602</uri>
      </author>
    </item>
    <item>
      <title>Implications of mHVSR Spatial Variability on Site Response Predictability</title>
      <link>https://escholarship.org/uc/item/90b2c6w9</link>
      <description>One-dimensional ground response analyses (GRA) can introduce model error to site response estimates when wave propagation is not dominated by vertically propagating shear waves. We identify sites suitable for GRA based on microtremor horizontal-to-vertical spectral ratios (mHVSRs). We analyzed 300 microtremor recordings from 17 vertical array sites in California, comparing mHVSRs at varying spatial separations. We find that low mHVSR spatial correlation, as measured using Longest Common Subsequence, tends to occur at vertical array sites that are poorly modeled by GRA. Conversely, stronger mHVSR correlations tend to occur at sites where GRA is relatively effective.</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/90b2c6w9</guid>
      <pubDate>Mon, 21 Oct 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Ornelas, Francisco Javier</name>
      </author>
      <author>
        <name>de la Torre, Christopher A</name>
      </author>
      <author>
        <name>Stewart, Jonathan P</name>
        <uri>https://orcid.org/0000-0003-3602-3629</uri>
      </author>
    </item>
    <item>
      <title>Deciphering the controlling factors for phase transitions in zeolitic imidazolate frameworks</title>
      <link>https://escholarship.org/uc/item/5gt753k0</link>
      <description>Zeolitic imidazolate frameworks (ZIFs) feature complex phase transitions, including polymorphism, melting, vitrification, and polyamorphism. Experimentally probing their structural evolution during transitions involving amorphous phases is a significant challenge, especially at the medium-range length scale. To overcome this challenge, here we first train a deep learning-based force field to identify the structural characteristics of both crystalline and non-crystalline ZIF phases. This allows us to reproduce the structural evolution trend during the melting of crystals and formation of ZIF glasses at various length scales with an accuracy comparable to that of &lt;i&gt;ab initio&lt;/i&gt; molecular dynamics, yet at a much lower computational cost. Based on this approach, we propose a new structural descriptor, namely, the ring orientation index, to capture the propensity for crystallization of ZIF-4 (Zn(Im)&lt;sub&gt;2&lt;/sub&gt;, Im&amp;nbsp;=&amp;nbsp;C&lt;sub&gt;3&lt;/sub&gt;H&lt;sub&gt;3&lt;/sub&gt;N&lt;sub&gt;2&lt;/sub&gt;&lt;sup&gt;-&lt;/sup&gt;)...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/5gt753k0</guid>
      <pubDate>Tue, 10 Sep 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Du, Tao</name>
      </author>
      <author>
        <name>Li, Shanwu</name>
      </author>
      <author>
        <name>Ganisetti, Sudheer</name>
      </author>
      <author>
        <name>Bauchy, Mathieu</name>
        <uri>https://orcid.org/0000-0003-4600-0631</uri>
      </author>
      <author>
        <name>Yue, Yuanzheng</name>
      </author>
      <author>
        <name>Smedskjaer, Morten M</name>
      </author>
    </item>
    <item>
      <title>Edge-based graph neural network for ranking critical road segments in a network</title>
      <link>https://escholarship.org/uc/item/4j80v0bn</link>
      <description>Transportation networks play a crucial role in society by enabling the smooth movement of people and goods during regular times and acting as arteries for evacuations during catastrophes and natural disasters. Identifying the critical road segments in a large and complex network is essential for planners and emergency managers to enhance the network's efficiency, robustness, and resilience to such stressors. We propose a novel approach to rapidly identify critical and vital network components (road segments in a transportation network) for resilience improvement or post-disaster recovery. We pose the transportation network as a graph with roads as edges and intersections as nodes and deploy a Graph Neural Network (GNN) trained on a broad range of network parameter changes and disruption events to rank the importance of road segments. The trained GNN model can rapidly estimate the criticality rank of individual road segments in the modified network resulting from an interruption....</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/4j80v0bn</guid>
      <pubDate>Thu, 29 Aug 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Jana, Debasish</name>
        <uri>https://orcid.org/0000-0003-2368-6394</uri>
      </author>
      <author>
        <name>Malama, Sven</name>
      </author>
      <author>
        <name>Narasimhan, Sriram</name>
      </author>
      <author>
        <name>Taciroglu, Ertugrul</name>
        <uri>https://orcid.org/0000-0001-9618-1210</uri>
      </author>
    </item>
    <item>
      <title>Cultivating climate resilience in California agriculture: Adaptations to an increasingly volatile water future</title>
      <link>https://escholarship.org/uc/item/1fg4v5tf</link>
      <description>California agriculture will undergo significant transformations over the next few decades in response to climate extremes, environmental regulation and policy encouraging environmental justice, and economic pressures that have long driven agricultural changes. With several local climates suited to a variety of crops, periodically abundant nearby precipitation, and public investments that facilitated abundant low-priced irrigation water, California hosts one of the most diverse and productive agroecosystems in the world. California farms supply nearly half of the high-nutrient fruit, tree nut, and vegetable production in the United States. Climate change impacts on productivity and profitability of California agriculture are increasing and forebode problems for standard agricultural practices, especially water use norms. We highlight many challenges California agriculture confronts under climate change through the direct and indirect impacts on the biophysical conditions and ecosystem...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/1fg4v5tf</guid>
      <pubDate>Thu, 22 Aug 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Medellín-Azuara, Josué</name>
      </author>
      <author>
        <name>Escriva-Bou, Alvar</name>
      </author>
      <author>
        <name>Gaudin, Amélie CM</name>
      </author>
      <author>
        <name>Schwabe, Kurt A</name>
        <uri>https://orcid.org/0000-0002-3402-1411</uri>
      </author>
      <author>
        <name>Sumner, Daniel A</name>
      </author>
    </item>
    <item>
      <title>User-interaction with a web-served global ground motion relational database</title>
      <link>https://escholarship.org/uc/item/9tw6k14c</link>
      <description>We present an application programming interface (API) which facilitates public access to a global relational database of earthquake ground motion intensity measures, associated metadata, and time-series data. Next Generation Attenuation (NGA)-East and NGA-West2 project spreadsheets have been adapted into a relational database format composed of multiple tables through a series of primary and foreign keys. The combined dataset has been expanded to include contributions from earthquakes, generally with magnitudes greater than M3.9, that have occurred since the conclusion of the data synthesis component of both projects in 2011. Currently the database includes 62,449 ground motions recorded at 9,092 stations for 899 events. The database is accessible through an API, which allows users to interact with and query the database directly without detailed knowledge of structure query language (SQL). Simple queries are constructed by appending relatively straightforward query string parameters...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/9tw6k14c</guid>
      <pubDate>Sun, 7 Jul 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Buckreis, Tristan</name>
      </author>
      <author>
        <name>Nweke, CC</name>
      </author>
      <author>
        <name>Wang, Pangfei</name>
      </author>
      <author>
        <name>Brandenberg, scott</name>
      </author>
      <author>
        <name>Shams, Rashid</name>
      </author>
      <author>
        <name>Ramos-Sepulveda, Maria</name>
      </author>
      <author>
        <name>Pretell, Renmin</name>
      </author>
      <author>
        <name>Mazzoni, Silvia</name>
      </author>
      <author>
        <name>Stewart, Jonathan P</name>
        <uri>https://orcid.org/0000-0003-3602-3629</uri>
      </author>
    </item>
    <item>
      <title>Reliability of low frequency mHVSR ordinates</title>
      <link>https://escholarship.org/uc/item/9731j6bz</link>
      <description>Microtremor horizontal-to-vertical spectral ratios (mHVSR) are frequency-dependent ratios of Fourier amplitude spectra of the horizontal to vertical components of a 3-component recording of ambient ground motions from microtremors. Results from mHVSR tests can identify the frequencies associated with site resonances at sites with large impedance contrasts, and hence have potential to provide useful parameters for predicting seismic site response. Site measurements are made by recording ground vibrations either from a temporarily deployed seismometer, typically recording for a relatively short period of time (~1-2 hrs.), or from a permanently-installed broadband seismometer. In this paper, we discuss ongoing work investigating the reliability of low frequency (&amp;lt; ∼0.1 Hz) mHVSR ordinates. Such low frequency ordinates are potentially useful for sites that are known to have deep basins (e.g., LA Basin, Imperial Valley, Great Salt Lake basin), where fundamental frequencies may fall...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/9731j6bz</guid>
      <pubDate>Sun, 7 Jul 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Ornelas, Francesco Javier</name>
      </author>
      <author>
        <name>Nweke, CC</name>
      </author>
      <author>
        <name>de la Torre, Christopher A</name>
      </author>
      <author>
        <name>Wang, Pengfe9</name>
      </author>
      <author>
        <name>Mai, TD</name>
      </author>
      <author>
        <name>Cox, Brady R</name>
      </author>
      <author>
        <name>Brandenberg, Scott J</name>
      </author>
      <author>
        <name>Stewart, Jonathan P</name>
        <uri>https://orcid.org/0000-0003-3602-3629</uri>
      </author>
    </item>
    <item>
      <title>A general framework for modeling subregional path effects</title>
      <link>https://escholarship.org/uc/item/7c5870pf</link>
      <description>Next Generation Attenuation (NGA) West2 ground motion models (GMMs) include regional path adjustments for broad jurisdictional regions, which necessarily averages spatially variable path effects within those regions. We extend that framework to account for systematic variations in attenuation within subregions defined in consideration of geologic differences. In recent years, cell-based methods which systematically account for spatial variations by summing the attenuation effects over a fine discretization of uniform-rectangular cells (e.g., Dawood and Rodriquez-Marek 2013; Kuehn et al. 2019) have been shown to be an effective alternative to regionalization and a step towards modelling non-ergodic path effects. The main drawbacks of these models, however, are their increased computational complexity, poorly informed coefficients for cells in which few paths travel, and unoptimized boundaries that may span across the limits of geologic domains. The framework presented here considers...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/7c5870pf</guid>
      <pubDate>Sun, 7 Jul 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Buckreis, Tristan</name>
      </author>
      <author>
        <name>Wang, Pengfei</name>
      </author>
      <author>
        <name>Brandenberg, scott</name>
      </author>
      <author>
        <name>Stewart, Jonathan P</name>
        <uri>https://orcid.org/0000-0003-3602-3629</uri>
      </author>
    </item>
    <item>
      <title>Empirical site response of Mexico City through regionalization of global subduction GMMs</title>
      <link>https://escholarship.org/uc/item/6f7990md</link>
      <description>We assemble a dataset which enhances existing Central America and Mexico data for the NGASubduction (NGA-Sub) project, including now additional earthquake ground motions and site parameters from Mexico. This data has been used to provide regional customization of NGA-Sub global Ground Motion Models (GMMs) for application in Mexico, paying particular attention to the site response of Mexico City (CDMX). The expanded database for Mexico incorporates smaller magnitude earthquakes (M &amp;lt; 6) and three significant events (M 7.2-8.3) that occurred in 2017 and 2018. These latter events are particularly important, because they are well recorded over a broad distance range and apply for hazard-critical conditions. Our focus here is on presenting the observed site response in CDMX, which we model based on the time-averaged shear wave
velocity in the upper 30 meters (VS30) and the Peak Ground Acceleration at a reference rock site (PGAr). The
empirical model we propose is different from previous...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/6f7990md</guid>
      <pubDate>Sun, 7 Jul 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Contreras, Victor</name>
      </author>
      <author>
        <name>Stewart, Jonathan P</name>
        <uri>https://orcid.org/0000-0003-3602-3629</uri>
      </author>
      <author>
        <name>Pérez-Campos, Xyoli</name>
      </author>
      <author>
        <name>Mayoral, Juan</name>
      </author>
      <author>
        <name>De La Rosa, D</name>
      </author>
    </item>
    <item>
      <title>Findings from a decade of ground motion simulation validation research and a path forward</title>
      <link>https://escholarship.org/uc/item/3wm8s4pg</link>
      <description>Simulated ground motions can advance seismic hazard assessments and structural response analyses, particularly for conditions with limited recorded ground motions such as large magnitude earthquakes at short source-to-site distances. Rigorous validation of simulated ground motions is required before hazard analysts, practicing engineers, or regulatory bodies can be confident in their use. A decade ago, validation exercises were mainly limited to comparisons of simulated-to-observed waveforms and median values of spectral accelerations for selected earthquakes. The Southern California Earthquake Center (SCEC) Ground Motion Simulation Validation (GMSV) group was formed to increase coordination between simulation modelers and research engineers with the aim of devising and applying more effective methods for simulation validation.

In this presentation, we summarize what has been learned in over a decade of GMSV activities. We categorize different validation methods according to...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/3wm8s4pg</guid>
      <pubDate>Sun, 7 Jul 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Rezaeian, Sanaz</name>
      </author>
      <author>
        <name>Stewart, Jonathan</name>
        <uri>https://orcid.org/0000-0003-3602-3629</uri>
      </author>
      <author>
        <name>Luco, Nico</name>
      </author>
      <author>
        <name>Goulet, Christine A</name>
      </author>
    </item>
    <item>
      <title>Relative contributions of different sources of epistemic uncertainty on seismic hazard in California</title>
      <link>https://escholarship.org/uc/item/20q0x2hf</link>
      <description>We evaluate the relative impact of three sources of epistemic uncertainty on probabilistic seismic hazard analyses in California: source model uncertainty, ground motion model (GMM) uncertainty, and site parameter uncertainty. Seismic source model uncertainty is inherently contained in the source model framework applied by the USGS in the 2023 National Seismic Hazard Model (NSHM23); we have added tools to extract this uncertainty for California sites in the open-source seismic hazard software OpenSHA. GMM uncertainty is generally accounted for using alternative models in PSHA or a single backbone model with a defined uncertainty. Site parameter uncertainty refers to uncertainty in the shear wave velocity of the upper 30 meters of the site profile (VS30) and potentially other independent site parameters.

We demonstrate the impacts of these major sources of epistemic uncertainty at the sites of two UC campuses, Berkeley, which is located near the active Hayward fault, and Davis,...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/20q0x2hf</guid>
      <pubDate>Sun, 7 Jul 2024 00:00:00 +0000</pubDate>
      <author>
        <name>O'Donnell, Timothy</name>
      </author>
      <author>
        <name>Stewart, Jonathan P</name>
        <uri>https://orcid.org/0000-0003-3602-3629</uri>
      </author>
      <author>
        <name>Milner, Kevin R</name>
      </author>
    </item>
    <item>
      <title>Recommendations on best available science for the United States National Seismic Hazard Model</title>
      <link>https://escholarship.org/uc/item/1x6139kd</link>
      <description>The 50 state update to the 2023 United States National Seismic Hazard Model (NSHM) is the latest in a sequence published by the U. S. Geological Survey (USGS). The 2023 NSHM is intended for use in building codes and similar applications at return periods of 475 years (corresponding to exceedance probabilities of 10% in 50 years) or longer. In reviewing the model, the NSHM Program Steering Committee, consisting of the authors of this paper, considered the characteristics of “best available science” that are applicable to the NSHM. Best available science must perform better than the previous NSHM, and there should be no available alternatives that could improve the models. The following are suggested characteristics of “best available science”:

A) Clear objectives
B) Rigorous conceptual model
C) Timely, relevant and inclusive
D) Verified and reproducible
E) Validated intermediate and final models
F) Replicable within uncertainties
G) Peer reviewed
H) Permanent documentation

This...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/1x6139kd</guid>
      <pubDate>Sun, 7 Jul 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Anderson, John G</name>
      </author>
      <author>
        <name>Atkinson, Gail M</name>
      </author>
      <author>
        <name>Baker, Jack W</name>
      </author>
      <author>
        <name>Campbell, Kenneth W</name>
      </author>
      <author>
        <name>DeShon, Heather R</name>
      </author>
      <author>
        <name>Jordan, Thomas H</name>
      </author>
      <author>
        <name>Kelson, Keith I</name>
      </author>
      <author>
        <name>Shome, Nilesh</name>
      </author>
      <author>
        <name>Stewart, Jonathan P</name>
        <uri>https://orcid.org/0000-0003-3602-3629</uri>
      </author>
    </item>
    <item>
      <title>A maching learning-based analysis of liquefaction input factors using the Next Generation Liquefaction database</title>
      <link>https://escholarship.org/uc/item/0vz1x69b</link>
      <description>Liquefaction triggering is typically predicted using fully-empirical and/or semi-empirical models. Hence, such models are heavily reliant upon available liquefaction (and/or lack thereof) case history data. These predictive models are based on a variety of factors, describing the demand (i.e., the cyclic stress ratio, CSR in existing legacy models) and the capacity (i.e., the cyclic resistance ratio, CRR). However, the degree to which these factors truly affect models’ performance is unknown. To explore this aspect and quantitatively rank the importance of liquefaction input model parameters, we leverage a Random Forest Machine Learning (ML) approach using two methods: (1) a feature importance metric based on the Gini impurity index, and (2) a SHapley Additive exPlanations (SHAP)-based approach. Both approaches were employed using typical input factors used in legacy liquefaction triggering models based on cone penetration test (CPT) data. Such analyses were performed using all...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/0vz1x69b</guid>
      <pubDate>Sun, 7 Jul 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Zimmaro, Paolo</name>
      </author>
      <author>
        <name>Hudson, Kenneth</name>
      </author>
      <author>
        <name>Ulmer, Kristin</name>
      </author>
      <author>
        <name>Brandenberg, Scott</name>
      </author>
      <author>
        <name>Stewart, Jonathan P</name>
        <uri>https://orcid.org/0000-0003-3602-3629</uri>
      </author>
      <author>
        <name>Kramer, Steven L</name>
      </author>
    </item>
    <item>
      <title>Revealing hidden medium-range order in amorphous materials using topological data analysis</title>
      <link>https://escholarship.org/uc/item/0h4758n9</link>
      <description>Despite the numerous technological applications of amorphous materials, such as glasses, the understanding of their medium-range order (MRO) structure-and particularly the origin of the first sharp diffraction peak (FSDP) in the structure factor-remains elusive. Here, we use persistent homology, an emergent type of topological data analysis, to understand MRO structure in sodium silicate glasses. To enable this analysis, we introduce a self-consistent categorization of rings with rigorous geometrical definitions of the structural entities. Furthermore, we enable quantitative comparison of the persistence diagrams by computing the cumulative sum of all points weighted by their lifetime. On the basis of these analysis methods, we show that the approach can be used to deconvolute the contributions of various MRO features to the FSDP. More generally, the developed methodology can be applied to analyze and categorize molecular dynamics data and understand MRO structure in any class...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/0h4758n9</guid>
      <pubDate>Fri, 5 Jul 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Sørensen, Søren S</name>
      </author>
      <author>
        <name>Biscio, Christophe AN</name>
      </author>
      <author>
        <name>Bauchy, Mathieu</name>
        <uri>https://orcid.org/0000-0003-4600-0631</uri>
      </author>
      <author>
        <name>Fajstrup, Lisbeth</name>
      </author>
      <author>
        <name>Smedskjaer, Morten M</name>
      </author>
    </item>
    <item>
      <title>Reconnaissance of 2020 M 7.0 Samos Island (Aegean Sea) earthquake</title>
      <link>https://escholarship.org/uc/item/5m73x8c0</link>
      <description>The Samos Island (Aegean Sea) Earthquake occurred on 30 October 2020. It produced a tsunami that impacted coastal communities, ground shaking that was locally amplified in some areas and that led to collapse of structures with 118 fatalities in both Greece and Turkey, and wide-ranging geotechnical effects including rockfalls, landsliding, and liquefaction. As a result of the global COVID-19 pandemic, the reconnaissance of this event did not involve the deployment of international teams, as would be typical for an event of this size. Instead, following initial deployments of separate Greek and Turkish teams, the reconnaissance and documentation efforts were managed in a coordinated manner with the assistance of international partners. This coordination ultimately produced a multi-agency joint report published on the 2-month anniversary of the earthquake, and this special issue. This paper provides an overview of the reconnaissance activities undertaken to document the effects of...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/5m73x8c0</guid>
      <pubDate>Thu, 13 Jun 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Cetin, K Onder</name>
      </author>
      <author>
        <name>Mylonakis, George</name>
      </author>
      <author>
        <name>Sextos, Anastasios</name>
      </author>
      <author>
        <name>Stewart, Jonathan P</name>
        <uri>https://orcid.org/0000-0003-3602-3629</uri>
      </author>
    </item>
    <item>
      <title>Foundation Settlement and Tilt of Millennium Tower in San Francisco, California</title>
      <link>https://escholarship.org/uc/item/45x3x28x</link>
      <description>Foundation Settlement and Tilt of Millennium Tower in San Francisco, California</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/45x3x28x</guid>
      <pubDate>Wed, 12 Jun 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Stewart, Jonathan P</name>
        <uri>https://orcid.org/0000-0003-3602-3629</uri>
      </author>
      <author>
        <name>Wagner, Nathaniel</name>
      </author>
      <author>
        <name>Murphy, Debra</name>
      </author>
      <author>
        <name>Butkovich, Jeremy</name>
      </author>
      <author>
        <name>Largent, Micaela</name>
      </author>
      <author>
        <name>Nouri, Hamid</name>
      </author>
      <author>
        <name>Curran, Hannah</name>
      </author>
      <author>
        <name>Maffioli, Darcie</name>
      </author>
      <author>
        <name>Egan, John A</name>
      </author>
    </item>
    <item>
      <title>Preliminary observations of an ergodic site response model in California conditioned on Vs30 and HVSR Parameters</title>
      <link>https://escholarship.org/uc/item/3527w1wb</link>
      <description>Traditional ergodic models are derived based on time-averaged shear-wave velocity in the upper 30 m of the site. These models are not able to account for site resonances, the presence and frequency of which can be established from microtremor HVSR surveys. Not all California sites exhibit such resonances, but knowledge that peaks are or are not present affects site response over a wide range of frequencies, with the former producing a response spectral peak near the HVSR peak. Research is underway to develop a model using microtremor HVSR data, which will be novel relative to previous models that are based on earthquake HVSR data. Our model is being formulated as modification to a global VS30 and z1.0 relationship. This paper explains the model development approach and findings of a systematic assessment of how HVSR curves relate to features of site-specific (or non-ergodic) response, which is informing model development.</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/3527w1wb</guid>
      <pubDate>Fri, 10 May 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Ornelas, Francisco-Javier</name>
      </author>
      <author>
        <name>Buckreis, Tristan</name>
      </author>
      <author>
        <name>Nweke, Chukwuebuka C</name>
      </author>
      <author>
        <name>Wang, Pengfei</name>
      </author>
      <author>
        <name>de Torre, Christopher</name>
      </author>
      <author>
        <name>Brandenberg, Scott J</name>
      </author>
      <author>
        <name>Stewart, Jonathan P</name>
        <uri>https://orcid.org/0000-0003-3602-3629</uri>
      </author>
    </item>
    <item>
      <title>February 6, 2023 Türkiye Earthquakes: Ground Motions</title>
      <link>https://escholarship.org/uc/item/2pf5n7vp</link>
      <description>The 2023 Türkiye/Syria earthquake sequence includes the February 6 M7.8 mainshock followed approximately nine hours later by a M7.7 aftershock, and many smaller aftershocks including a M6.8 and M6.3 on February 6 and 20, respectively. These events occurred in a region near the plate boundary of the East Anatolian Fault, in the proximity of which numerous ground motion recordings sites had been installed north of the Türkiye/Syria border. As a result, the events were well recorded both near the fault and at rupture distances up to 570 km. We describe the available recordings and component-specific data processing performed with the aim of optimizing usable bandwidth. The resulting database includes 310, 351, 291, and 229 usable three-component recordings from the M7.8, M7.7, M6.8, and M6.3 events, respectively. We also present source, path, and site metadata that was compiled according to uniform protocols. Comparisons to a global ground motion model (GMM) for active tectonic regions...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/2pf5n7vp</guid>
      <pubDate>Fri, 10 May 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Buckreis, Tristan E</name>
      </author>
      <author>
        <name>Pretell, Renmin</name>
      </author>
      <author>
        <name>Sandikkaya, Abdullah</name>
      </author>
      <author>
        <name>Kale, Özkan</name>
      </author>
      <author>
        <name>Askan, Aysegul</name>
      </author>
      <author>
        <name>Brandenberg, Scott J</name>
      </author>
      <author>
        <name>Stewart, Jonathan P</name>
        <uri>https://orcid.org/0000-0003-3602-3629</uri>
      </author>
    </item>
    <item>
      <title>Application of Non-Ergodic Site Response for High Velocity Contrast Sites in the San Francisco Bay Area</title>
      <link>https://escholarship.org/uc/item/2h54r2tk</link>
      <description>Seismic-hazard analysis (SHA) is typically performed using ergodic ground-motion models (GMMs), wherein the site response component is derived from global data and conditioned on the time-averaged shear-wave velocity in the upper 30 meters (VS30) and a “basin depth” term (e.g., Z1.0 or Z2.5). In the ergodic GMMs, for a given VS30, there is an implicit shear-wave velocity (VS) profile associated with the site response prediction that has smooth increases of velocity with depth. When a site-specific VS profile is characterized by abrupt velocity contrasts, for example at the rock-soil interface, the site response is likely to differ significantly from ergodic model predictions. This limitation of the ergodic models can be overcome by incorporating non-ergodic site response in the SHA. This approach involves customizing the site response for site-specific conditions, which has the effect of decreasing overall model uncertainty.In this paper, we describe results from ergodic SHA and...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/2h54r2tk</guid>
      <pubDate>Fri, 10 May 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Teague, David</name>
      </author>
      <author>
        <name>Vahdani, Shahriar</name>
      </author>
      <author>
        <name>Stewart, Jonathan</name>
        <uri>https://orcid.org/0000-0003-3602-3629</uri>
      </author>
      <author>
        <name>Khoshkbari, Parham</name>
      </author>
      <author>
        <name>Eliahu, Uri</name>
      </author>
    </item>
    <item>
      <title>De Novo Atomistic Discovery of Disordered Mechanical Metamaterials by Machine Learning</title>
      <link>https://escholarship.org/uc/item/5dd5320s</link>
      <description>Architected materials design across orders of magnitude length scale intrigues exceptional mechanical responses nonexistent in their natural bulk state. However, the so-termed mechanical metamaterials, when scaling bottom down to the atomistic or microparticle level, remain largely unexplored and conventionally fall out of their coarse-resolution, ordered-pattern design space. Here, combining high-throughput molecular dynamics (MD) simulations and machine learning (ML) strategies, some intriguing atomistic families of disordered mechanical metamaterials are discovered, as fabricated by melt quenching and exemplified herein by lightweight-yet-stiff cellular materials featuring a theoretical limit of linear stiffness-density scaling, whose structural disorder-rather than order-is key to reduce the scaling exponent and is simply controlled by the bonding interactions and their directionality that enable flexible tunability experimentally. Importantly, a systematic navigation in the...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/5dd5320s</guid>
      <pubDate>Tue, 9 Apr 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Liu, Han</name>
      </author>
      <author>
        <name>Li, Liantang</name>
      </author>
      <author>
        <name>Wei, Zhenhua</name>
      </author>
      <author>
        <name>Smedskjaer, Morten M</name>
      </author>
      <author>
        <name>Zheng, Xiaoyu Rayne</name>
      </author>
      <author>
        <name>Bauchy, Mathieu</name>
        <uri>https://orcid.org/0000-0003-4600-0631</uri>
      </author>
    </item>
    <item>
      <title>State-of-the-Science Data and Methods Need to Guide Place-Based Efforts to Reduce Air Pollution Inequity</title>
      <link>https://escholarship.org/uc/item/4bt2s7mj</link>
      <description>BACKGROUND: Recently enacted environmental justice policies in the United States at the state and federal level emphasize addressing place-based inequities, including persistent disparities in air pollution exposure and associated health impacts. Advances in air quality measurement, models, and analytic methods have demonstrated the importance of finer-scale data and analysis in accurately quantifying the extent of inequity in intraurban pollution exposure, although the necessary degree of spatial resolution remains a complex and context-dependent question.
OBJECTIVE: The objectives of this commentary were to &lt;i&gt;a&lt;/i&gt;) discuss ways to maximize and evaluate the effectiveness of efforts to reduce air pollution disparities, and &lt;i&gt;b&lt;/i&gt;) argue that environmental regulators must employ improved methods to project, measure, and track the distributional impacts of new policies at finer geographic and temporal scales.
DISCUSSION: The historic federal investments from the Inflation Reduction...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/4bt2s7mj</guid>
      <pubDate>Thu, 28 Mar 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Gohlke, Julia M</name>
      </author>
      <author>
        <name>Harris, Maria H</name>
      </author>
      <author>
        <name>Roy, Ananya</name>
      </author>
      <author>
        <name>Thompson, Tammy M</name>
      </author>
      <author>
        <name>DePaola, Mindi</name>
      </author>
      <author>
        <name>Alvarez, Ramón A</name>
      </author>
      <author>
        <name>Anenberg, Susan C</name>
      </author>
      <author>
        <name>Apte, Joshua S</name>
        <uri>https://orcid.org/0000-0002-2796-3478</uri>
      </author>
      <author>
        <name>Demetillo, Mary Angelique G</name>
      </author>
      <author>
        <name>Dressel, Isabella M</name>
      </author>
      <author>
        <name>Kerr, Gaige H</name>
      </author>
      <author>
        <name>Marshall, Julian D</name>
      </author>
      <author>
        <name>Nowlan, Aileen E</name>
      </author>
      <author>
        <name>Patterson, Regan F</name>
      </author>
      <author>
        <name>Pusede, Sally E</name>
      </author>
      <author>
        <name>Southerland, Veronica A</name>
      </author>
      <author>
        <name>Vogel, Sarah A</name>
      </author>
    </item>
    <item>
      <title>Advancements in conventional and 3D printed feed spacers in membrane modules</title>
      <link>https://escholarship.org/uc/item/5wv5692p</link>
      <description>Plate &amp;amp; frame and spiral-wound modules are used for gas separation, pervaporation, reverse osmosis, nanofiltration, ultrafiltration, microfiltration, electro-dialysis, electro-deionization, membrane distillation and forward osmosis membrane processes. Feed channel spacers are an integral part of both module types – providing mechanical support for a cross-flow channel through the module and, in most cases, promoting mixing to enhance mass transfer to reduce concentration polarization and fouling. However, enhanced mass transfer comes at a cost of increased hydraulic pressure losses and stagnant zones wherever a spacer filament touches a membrane surface. These stagnant zones exacerbate membrane fouling and make cleaning more difficult. Efforts to improve feed spacer performance largely focus on adjusting the chemistry or geometry of the spacer to mitigate these challenges. Additive manufacturing (i.e. 3D printing) offers new degrees of freedom in feed spacer design and production,...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/5wv5692p</guid>
      <pubDate>Thu, 21 Mar 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Qian, Xin</name>
      </author>
      <author>
        <name>Anvari, Arezou</name>
      </author>
      <author>
        <name>Hoek, Eric MV</name>
        <uri>https://orcid.org/0000-0002-9674-1916</uri>
      </author>
      <author>
        <name>McCutcheon, Jeffrey R</name>
      </author>
    </item>
    <item>
      <title>A reverse-selective ion exchange membrane for the selective transport of phosphates via an outer-sphere complexation–diffusion pathway</title>
      <link>https://escholarship.org/uc/item/6g64x0rs</link>
      <description>Specific-ion selectivity is a highly desirable feature for the next generation of membranes. However, existing membranes rely on differences in charge, size and hydration energy, which limits their ability to target individual ion species. Here we demonstrate a nanocomposite ion-exchange membrane material that enables a reverse-selective transport mechanism that can selectively pass a single ion species. We demonstrate this transport mechanism with phosphate ions selectively transporting across negatively charged cation exchange membranes. Selective transport is enabled by the in situ growth of hydrous manganese oxide nanoparticles throughout a cation exchange membrane that provide a diffusion pathway via phosphate-specific, reversible outer-sphere interactions. On incorporating the hydrous manganese oxide nanoparticles, the membrane’s phosphate flux increased by a factor of 27 over an unmodified cation exchange membrane, and the selectivity of phosphorous over sulfate, nitrate...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/6g64x0rs</guid>
      <pubDate>Wed, 20 Mar 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Iddya, Arpita</name>
      </author>
      <author>
        <name>Zarzycki, Piotr</name>
        <uri>https://orcid.org/0000-0003-3891-7159</uri>
      </author>
      <author>
        <name>Kingsbury, Ryan</name>
      </author>
      <author>
        <name>Khor, Chia Miang</name>
      </author>
      <author>
        <name>Ma, Shengcun</name>
      </author>
      <author>
        <name>Wang, Jingbo</name>
      </author>
      <author>
        <name>Wheeldon, Ian</name>
        <uri>https://orcid.org/0000-0002-3492-7539</uri>
      </author>
      <author>
        <name>Ren, Zhiyong Jason</name>
      </author>
      <author>
        <name>Hoek, Eric MV</name>
      </author>
      <author>
        <name>Jassby, David</name>
      </author>
    </item>
    <item>
      <title>Molecular mechanisms of thickness-dependent water desalination in polyamide reverse-osmosis membranes</title>
      <link>https://escholarship.org/uc/item/44c450q3</link>
      <description>Using non-equilibrium molecular simulations, we systematically elaborate the relationships among synthesis (membrane's thickness and morphology), atomic-scale transport mechanism, and separation performance (permeability and selectivity) for 3D-printed polyamide (PA) membranes. Results indicated that water diffusion, swelling ratio, water flux, and water permeance proportionally decrease with increasing membrane thickness (4.0–32.5&amp;nbsp;nm). PA membranes with different thicknesses can achieve almost 100% salt rejection over the simulation time. Importantly, water permeability exponentially decreases with increasing thickness, and 15&amp;nbsp;nm is identified as the critical membrane thickness for efficient water transport. The discontinuous water-available space spreads all over PA membranes with thicknesses greater than 5&amp;nbsp;nm, allowing water molecules to jump by way of the temporary open-and-close pores. However, the connected water-useable space exists in PA membranes with thicknesses...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/44c450q3</guid>
      <pubDate>Thu, 14 Mar 2024 00:00:00 +0000</pubDate>
      <author>
        <name>He, Jinlong</name>
      </author>
      <author>
        <name>Arbaugh, Tom</name>
      </author>
      <author>
        <name>Nguyen, Danh</name>
      </author>
      <author>
        <name>Xian, Weikang</name>
      </author>
      <author>
        <name>Hoek, Eric MV</name>
        <uri>https://orcid.org/0000-0002-9674-1916</uri>
      </author>
      <author>
        <name>McCutcheon, Jeffrey R</name>
      </author>
      <author>
        <name>Li, Ying</name>
      </author>
    </item>
    <item>
      <title>A Framework for Probabilistic Assessment of Liquefaction Manifestation</title>
      <link>https://escholarship.org/uc/item/4f481648</link>
      <description>As part of the next generation liquefaction (NGL) project, we are developing probabilistic triggering and manifestation models using laboratory data and cone penetration test (CPT) case histories in the NGL database. The case histories are used to develop probabilistic models for surface manifestation conditional on susceptibility, liquefaction triggering, soil properties, stratigraphic details, and other features. Susceptibility is interpreted as a sole function of soil composition and is expressed as a probabilistic function of soil behavior type index, Ic, obtained from CPT. A triggering model is derived based on laboratory tests on high-quality specimens from literature; this model captures mean responses and uncertainty reflective of data dispersion and is considered as a Bayesian prior that will subsequently be updated by field observation data. A manifestation model is then regressed from field case histories where surface manifestation was or was not observed, information...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/4f481648</guid>
      <pubDate>Sun, 3 Mar 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Hudson, Kenneth S</name>
      </author>
      <author>
        <name>Ulmer, Kristin</name>
      </author>
      <author>
        <name>Brandenberg, Scott J</name>
      </author>
      <author>
        <name>Zimmaro, Paolo</name>
      </author>
      <author>
        <name>Kramer, Steven L</name>
      </author>
      <author>
        <name>Stewart, Jonathan P</name>
        <uri>https://orcid.org/0000-0003-3602-3629</uri>
      </author>
    </item>
    <item>
      <title>Fly Ash–Ca(OH)2 Reactivity in Hypersaline NaCl and CaCl2 Brines</title>
      <link>https://escholarship.org/uc/item/9jj9j7dc</link>
      <description>The disposal of highly concentrated brines from coal power generation can be effectively accomplished by physical solidification and chemical stabilization (S&amp;amp;S) processes that utilize fly ashes as a reactant. Herein, pozzolanic fly ashes are typically combined with calcium-based additives to achieve S&amp;amp;S. While the reactions of fly ash-(cement)-water systems have been extensively studied, the reactivity of fly ashes in hypersaline brines (ionic strength, Im &amp;gt; 1 mol/L) is comparatively less understood. Therefore, the interactions of a Class C (Ca-rich) fly ash and a Class F (Ca-poor) fly ash were examined in the presence of Ca(OH)2, and their thermodynamic phase equilibria were modeled on contact with NaCl or CaCl2 brines for 0 ≤ Im ≤ 7.5 mol/L. At low ionic strengths (&amp;lt;0.3 mol/L), reactivity and stable phase assemblages remain effectively unaltered. However, at high(er) ionic strengths (&amp;gt;0.5 mol/L), the phase assemblage shows a particular abundance of Cl-AFm compounds...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/9jj9j7dc</guid>
      <pubDate>Wed, 28 Feb 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Collin, Marie</name>
        <uri>https://orcid.org/0000-0002-0571-5019</uri>
      </author>
      <author>
        <name>Prentice, Dale P</name>
        <uri>https://orcid.org/0000-0002-4980-8751</uri>
      </author>
      <author>
        <name>Arnold, Ross A</name>
      </author>
      <author>
        <name>Ellison, Kirk</name>
      </author>
      <author>
        <name>Simonetti, Dante A</name>
      </author>
      <author>
        <name>Sant, Gaurav N</name>
      </author>
    </item>
    <item>
      <title>Fly ash degree of reaction in hypersaline NaCl and CaCl2 brines: Effects of calcium-based additives</title>
      <link>https://escholarship.org/uc/item/8sh191qf</link>
      <description>The pozzolanic reaction of fly ashes with calcium-based additives can be effectively used to solidify and chemically stabilize (S&amp;amp;S process) highly concentrated brines inside a cementitious matrix. However, complex interactions between the fly ash, the additive, and the brine typically affect the phases formed at equilibrium, and the resulting solid capacity to successfully encapsulate the brine and its contaminants. Here, the performances of two types of fly ash (a Class C and Class F fly ash) are assessed when combined with different additives (two types of cement, or lime with and without NaAlO&lt;sub&gt;2&lt;/sub&gt;), and two types of brine (NaCl or CaCl&lt;sub&gt;2&lt;/sub&gt;) over a range of concentrations (0&amp;nbsp;≤&amp;nbsp;[Cl&lt;sup&gt;-&lt;/sup&gt;]&amp;nbsp;≤&amp;nbsp;2&amp;nbsp;M). The best performing matrices - i.e., the matrices with the highest Cl-containing phases content - were identified using XRD and TGA. The experimental results were then combined with thermodynamic modeling to dissociate the contribution...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/8sh191qf</guid>
      <pubDate>Wed, 28 Feb 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Collin, Marie</name>
        <uri>https://orcid.org/0000-0002-0571-5019</uri>
      </author>
      <author>
        <name>Song, Yu</name>
      </author>
      <author>
        <name>Prentice, Dale P</name>
        <uri>https://orcid.org/0000-0002-4980-8751</uri>
      </author>
      <author>
        <name>Arnold, Ross A</name>
      </author>
      <author>
        <name>Ellison, Kirk</name>
      </author>
      <author>
        <name>Simonetti, Dante A</name>
      </author>
      <author>
        <name>Bauchy, Mathieu</name>
        <uri>https://orcid.org/0000-0003-4600-0631</uri>
      </author>
      <author>
        <name>Sant, Gaurav N</name>
      </author>
    </item>
    <item>
      <title>Solubility behavior and thermodynamic modeling of sodium monosulfoaluminate (“U‐phase”) in cementitious systems</title>
      <link>https://escholarship.org/uc/item/8js3981j</link>
      <description>The “U-phase,” a sodium-containing (alumino-ferrite-monosubstituent) AFm phase, has been observed to form in sodium-enriched highly alkaline cementitious systems, for example, of relevance to nuclear waste, and saline industrial brine management. But, minimal information is available of the U-phase's (e.g., solubility or thermodynamic properties) due to its limited stability and its tendency to transform into ettringite or monosulfoaluminate. Herein, the U-phase was systematically synthesized at four temperatures (5, 15, 25, and 50°C) and fully characterized in terms of its thermochemical properties. The average composition of the synthesized U-phase (4CaO·Al2O3·1.85SO3·0.85Na2O·12H2O) deviates slightly from typical disclosures in the literature. The solubility product of the U-phase formation was measured from conditions of oversaturation. The measured thermodynamic data accurately predicted experimental observations of U-phase formation in cementitious environments. In general,...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/8js3981j</guid>
      <pubDate>Wed, 28 Feb 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Collin, Marie</name>
        <uri>https://orcid.org/0000-0002-0571-5019</uri>
      </author>
      <author>
        <name>Prentice, Dale P</name>
        <uri>https://orcid.org/0000-0002-4980-8751</uri>
      </author>
      <author>
        <name>Arnold, Ross R</name>
      </author>
      <author>
        <name>Ellison, Kirk</name>
      </author>
      <author>
        <name>Balonis, Magdalena</name>
      </author>
      <author>
        <name>Simonetti, Dante</name>
      </author>
      <author>
        <name>Sant, Gaurav N</name>
      </author>
    </item>
    <item>
      <title>The role of delay in vaccination rate on Covid-19</title>
      <link>https://escholarship.org/uc/item/7763m29r</link>
      <description>The role of vaccination in tackling Covid-19 and the potential consequences of a time delay in vaccination rate are discussed. This study presents a mathematical model that incorporates the rate of vaccination and parameters related to the presence and absence of time delay in the context of Covid-19. We conducted a study on the global dynamics of a Covid-19 outbreak model, which incorporates a vaccinated population and a time delay parameter. Our findings demonstrate the global stability of these models. Our observation indicates that lower vaccination rates are associated with an increase in the overall number of infected individuals. The stability of the corresponding time delay model is determined by the value of the time delay parameter. If the time delay parameter is less than the critical value at which the Hopf bifurcation occurs, the model is stable. The results are supported by numerical illustrations that have epidemiological relevance.</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/7763m29r</guid>
      <pubDate>Wed, 28 Feb 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Salman, Mohammed</name>
      </author>
      <author>
        <name>Mohanty, Sanjay Kumar</name>
      </author>
      <author>
        <name>Nayak, Chittaranjan</name>
      </author>
      <author>
        <name>Kumar, Sachin</name>
      </author>
    </item>
    <item>
      <title>How Brine Composition Affects Fly Ash Reactions: The Influence of (Cat-, An-)ion Type</title>
      <link>https://escholarship.org/uc/item/2t939172</link>
      <description>Hypersaline brines can be solidified and stabilized via the hydraulic and pozzolanic reactions between fly ash(es) and calcium-based additives. Although recent work has examined fly ash reactivity in single-salt ("simple") hypersaline brines (ionic strength, Im &amp;gt; 1 mol/L), the effects of mixed-salt solutions on fly ash reactivity remain unclear. Herein, the reactivity of a Class C (calcium oxide [CaO]-rich) or Class F (CaO-poor) fly ash mixture with calcium hydroxide is reacted in solutions bearing sodium chloride (NaCl), calcium chloride (CaCl2), magnesium chloride (MgCl2), sodium sulfate (Na2SO4), or combinations thereof for 1.5 ≤ Im ≤ 2.25 mol/L, from 1 week until 24 weeks. Expectedly, sulfate anions promote the formation of sulfate phases (i.e., ettringite, monosulfoaluminate, U-phase), while chloride anions induce the formation of Cl-AFm compounds (i.e., Kuzel's and Friedel's salt). Although the Class C fly ash's reactivity is similar across different anions (for a fixed...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/2t939172</guid>
      <pubDate>Wed, 28 Feb 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Collin, Marie</name>
        <uri>https://orcid.org/0000-0002-0571-5019</uri>
      </author>
      <author>
        <name>Prentice, Dale P</name>
        <uri>https://orcid.org/0000-0002-4980-8751</uri>
      </author>
      <author>
        <name>Arnold, Ross A</name>
      </author>
      <author>
        <name>Ellison, Kirk</name>
      </author>
      <author>
        <name>Simonetti, Dante A</name>
      </author>
      <author>
        <name>Sant, Gaurav N</name>
      </author>
    </item>
    <item>
      <title>Thermochemical data and phase equilibria of halide (Cl−, Br−, I−) containing AFm and hydrotalcite compounds</title>
      <link>https://escholarship.org/uc/item/0bv6j43p</link>
      <description>Layered double hydroxide (LDH) phases that form during cement hydration can incorporate a variety of interlayer anions in their interlayer positions. Here, a range of phases of general formula [MII(1−x)MIII(x)(OH)2][An−]x/n·zH2O were synthesized, where MII&amp;nbsp;=&amp;nbsp;Mg2+ (hydrotalcite) or Ca2+ (AFm), MIII&amp;nbsp;=&amp;nbsp;Al3+ such that [MII/Al]&amp;nbsp;=&amp;nbsp;2 (Ca and Mg, atomic units) or 3 (Mg only), and A&amp;nbsp;=&amp;nbsp;Cl−, Br−, or I−. All the synthesized phases were characterized to assess their composition, density, and crystal structure. By approach from undersaturation, the solubility data of these compounds was measured at 5, 25, and 60°C. This thermochemical data was used to successfully model their formation using thermodynamic modeling and to infer the fields of stability of these compounds for conditions of relevance to cementitious systems. It is seen that halide-containing hydrotalcite phases strongly compete with hydroxide-containing hydrotalcite, with the latter prevailing...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/0bv6j43p</guid>
      <pubDate>Wed, 28 Feb 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Collin, Marie</name>
        <uri>https://orcid.org/0000-0002-0571-5019</uri>
      </author>
      <author>
        <name>Prentice, Dale P</name>
        <uri>https://orcid.org/0000-0002-4980-8751</uri>
      </author>
      <author>
        <name>Geddes, Dan</name>
      </author>
      <author>
        <name>Provis, John L</name>
      </author>
      <author>
        <name>Ellison, Kirk</name>
      </author>
      <author>
        <name>Balonis, Magdalena</name>
      </author>
      <author>
        <name>Simonetti, Dante</name>
      </author>
      <author>
        <name>Sant, Gaurav N</name>
      </author>
    </item>
    <item>
      <title>The pore structure and water absorption in Portland/slag blended hardened cement paste determined by synchrotron X-ray microtomography and neutron radiography</title>
      <link>https://escholarship.org/uc/item/7gr7c7qg</link>
      <description>The pore structures of hardened Portland/slag cement pastes (&amp;gt;75 wt% slag content), and the initial capillary absorption of moisture through these pores, were monitored using &lt;i&gt;ex situ&lt;/i&gt; synchrotron X-ray computerised microtomography and &lt;i&gt;in situ&lt;/i&gt; quantitative neutron radiography. The pore structure becomes more constricted as the cement hydrates and its microstructure develops. This mechanism was effective even at a slag content as high as 90 wt% in the cementitious blend, where the lowest total porosity and a significant pore refinement were identified at extended curing ages (360 d). By combining this information with neutron radiographic imaging, and directly quantifying both depth and mass of water uptake, it was observed that 90 wt% slag cement outperformed the 75 wt% slag blend at 90 days in terms of resistance to capillary water uptake, although the higher-slag blend had not yet developed such a refined microstructure at 28 days of curing. The assumptions associated...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/7gr7c7qg</guid>
      <pubDate>Thu, 15 Feb 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Vigor, James E</name>
      </author>
      <author>
        <name>Prentice, Dale P</name>
        <uri>https://orcid.org/0000-0002-4980-8751</uri>
      </author>
      <author>
        <name>Xiao, Xianghui</name>
      </author>
      <author>
        <name>Bernal, Susan A</name>
      </author>
      <author>
        <name>Provis, John L</name>
      </author>
    </item>
    <item>
      <title>California’s zero-emission vehicle adoption brings air quality benefits yet equity gaps persist</title>
      <link>https://escholarship.org/uc/item/50w1s0f1</link>
      <description>Zero-emission vehicle (ZEV) adoption is a key climate mitigation tool, but its environmental justice implications remain unclear. Here, we quantify ZEV adoption at the census tract level in California from 2015 to 2020 and project it to 2035 when all new passenger vehicles sold are expected to be ZEVs. We then apply an integrated traffic model together with a dispersion model to simulate air quality changes near roads in the Greater Los Angeles. We found that per capita ZEV ownership in non-disadvantaged communities (non-DACs) as defined by the state of California is 3.8 times of that in DACs. Racial and ethnic minorities owned fewer ZEVs regardless of DAC designation. While DAC residents receive 40% more pollutant reduction than non-DACs due to intercommunity ZEV trips in 2020, they remain disproportionately exposed to higher levels of traffic-related air pollution. With more ZEVs in 2035, the exposure disparity narrows. However, to further reduce disparities, the focus must...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/50w1s0f1</guid>
      <pubDate>Mon, 5 Feb 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Yu, Qiao</name>
        <uri>https://orcid.org/0000-0002-1774-0860</uri>
      </author>
      <author>
        <name>He, Brian Yueshuai</name>
      </author>
      <author>
        <name>Ma, Jiaqi</name>
        <uri>https://orcid.org/0000-0002-8184-5157</uri>
      </author>
      <author>
        <name>Zhu, Yifang</name>
        <uri>https://orcid.org/0000-0002-0591-3322</uri>
      </author>
    </item>
    <item>
      <title>A general method to synthesize and sinter bulk ceramics in seconds</title>
      <link>https://escholarship.org/uc/item/7zq911jz</link>
      <description>Ceramics are an important class of materials with widespread applications because of their high thermal, mechanical, and chemical stability. Computational predictions based on first principles methods can be a valuable tool in accelerating materials discovery to develop improved ceramics. It is essential to experimentally confirm the material properties of such predictions. However, materials screening rates are limited by the long processing times and the poor compositional control from volatile element loss in conventional ceramic sintering techniques. To overcome these limitations, we developed an ultrafast high-temperature sintering (UHS) process for the fabrication of ceramic materials by radiative heating under an inert atmosphere. We provide several examples of the UHS process to demonstrate its potential utility and applications, including advancements in solid-state electrolytes, multicomponent structures, and high-throughput materials screening.</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/7zq911jz</guid>
      <pubDate>Wed, 3 Jan 2024 00:00:00 +0000</pubDate>
      <author>
        <name>Wang, Chengwei</name>
      </author>
      <author>
        <name>Ping, Weiwei</name>
      </author>
      <author>
        <name>Bai, Qiang</name>
      </author>
      <author>
        <name>Cui, Huachen</name>
      </author>
      <author>
        <name>Hensleigh, Ryan</name>
      </author>
      <author>
        <name>Wang, Ruiliu</name>
      </author>
      <author>
        <name>Brozena, Alexandra H</name>
      </author>
      <author>
        <name>Xu, Zhenpeng</name>
      </author>
      <author>
        <name>Dai, Jiaqi</name>
      </author>
      <author>
        <name>Pei, Yong</name>
      </author>
      <author>
        <name>Zheng, Chaolun</name>
      </author>
      <author>
        <name>Pastel, Glenn</name>
      </author>
      <author>
        <name>Gao, Jinlong</name>
      </author>
      <author>
        <name>Wang, Xizheng</name>
        <uri>https://orcid.org/0000-0003-4390-1733</uri>
      </author>
      <author>
        <name>Wang, Howard</name>
      </author>
      <author>
        <name>Zhao, Ji-Cheng</name>
      </author>
      <author>
        <name>Yang, Bao</name>
      </author>
      <author>
        <name>Zheng, Xiaoyu Rayne</name>
      </author>
      <author>
        <name>Luo, Jian</name>
        <uri>https://orcid.org/0000-0002-5424-0216</uri>
      </author>
      <author>
        <name>Mo, Yifei</name>
      </author>
      <author>
        <name>Dunn, Bruce</name>
      </author>
      <author>
        <name>Hu, Liangbing</name>
      </author>
    </item>
    <item>
      <title>Combinatorial molecular optimization of cement hydrates</title>
      <link>https://escholarship.org/uc/item/6r6275nz</link>
      <description>Despite its ubiquitous presence in the built environment, concrete’s molecular-level properties are only recently being explored using experimental and simulation studies. Increasing societal concerns about concrete’s environmental footprint have provided strong motivation to develop new concrete with greater specific stiffness or strength (for structures with less material). Herein, a combinatorial approach is described to optimize properties of cement hydrates. The method entails screening a computationally generated database of atomic structures of calcium-silicate-hydrate, the binding phase of concrete, against a set of three defect attributes: calcium-to-silicon ratio as compositional index and two correlation distances describing medium-range silicon-oxygen and calcium-oxygen environments. Although structural and mechanical properties correlate well with calcium-to-silicon ratio, the cross-correlation between all three defect attributes reveals an indentation modulus-to-hardness...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/6r6275nz</guid>
      <pubDate>Sun, 24 Dec 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Abdolhosseini Qomi, MJ</name>
      </author>
      <author>
        <name>Krakowiak, KJ</name>
      </author>
      <author>
        <name>Bauchy, M</name>
        <uri>https://orcid.org/0000-0003-4600-0631</uri>
      </author>
      <author>
        <name>Stewart, KL</name>
      </author>
      <author>
        <name>Shahsavari, R</name>
      </author>
      <author>
        <name>Jagannathan, D</name>
      </author>
      <author>
        <name>Brommer, DB</name>
      </author>
      <author>
        <name>Baronnet, A</name>
      </author>
      <author>
        <name>Buehler, MJ</name>
      </author>
      <author>
        <name>Yip, S</name>
      </author>
      <author>
        <name>Ulm, F-J</name>
      </author>
      <author>
        <name>Van Vliet, KJ</name>
      </author>
      <author>
        <name>Pellenq, RJ-M</name>
      </author>
    </item>
    <item>
      <title>Comparison of Ground Motions from CSN Instruments and Proximate Sensors from Other Networks</title>
      <link>https://escholarship.org/uc/item/72p42461</link>
      <description>The Community Seismic Network (CSN) is a low-cost, MEMS-sensor seismic network with smaller average station-to-station spacing than stations for other networks. We have downloaded and processed CSN data for 29 earthquakes with M &amp;gt; 4 from 2012 to 2023 using NGA procedures. Visual checks of data useability were applied to distinguish rejected records form records with clear seismic signals. We compare recordings from proximate (within 3 km) CSN and non-CSN (generally SCSN or CSMIP) stations with usable signals. Results show no systematic differences for peak acceleration and similar spectra when the CSN motions have large usable bandwidths.</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/72p42461</guid>
      <pubDate>Mon, 11 Dec 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Stewart, Jonathan P</name>
        <uri>https://orcid.org/0000-0003-3602-3629</uri>
      </author>
      <author>
        <name>Mohammed, Shako</name>
      </author>
      <author>
        <name>Nweke, Chukwuebuka C</name>
      </author>
      <author>
        <name>Shams, Rashid</name>
      </author>
      <author>
        <name>Buckreis, Tristan E</name>
      </author>
      <author>
        <name>Kohler, Monica D</name>
      </author>
      <author>
        <name>Bozorgnia, Yousef</name>
      </author>
    </item>
    <item>
      <title>Panel Review of Ground Motion Characterization Model in 2023 NSHM</title>
      <link>https://escholarship.org/uc/item/2546f8hw</link>
      <description>The 2023 National Seismic Hazard Model (NSHM; Petersen et al., 2023) has two major components – a seismic source characterization (SSC) model and a ground motion characterization (GMC) model. The US Geological Survey (USGS) established separate panels to review and provide input on these two models. Both panels are advisory, meaning that they provide input on technical issues for consideration by the USGS NSHM team, but they do not have decision making authority. Here, we report on the activities and recommendations of the Ground Motion Characterization Panel, made up of the authors of this review. Final modeling decisions are presented in separate USGS documents, including Petersen et al., (2023) and Moschetti et al., (2023). Where modeling decisions depart from our recommendations, the rationale is explained in those publications.</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/2546f8hw</guid>
      <pubDate>Mon, 11 Dec 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Stewart, Jonathan</name>
        <uri>https://orcid.org/0000-0003-3602-3629</uri>
      </author>
      <author>
        <name>Abrahamson, Norman A</name>
      </author>
      <author>
        <name>Atkinson, Gail M</name>
      </author>
      <author>
        <name>Anderson, John G</name>
      </author>
      <author>
        <name>Campbell, Kenneth W</name>
      </author>
      <author>
        <name>Cramer, Chris</name>
      </author>
      <author>
        <name>Kolaj, Michal</name>
      </author>
      <author>
        <name>Parker, Grace A</name>
      </author>
    </item>
    <item>
      <title>Graph-based structural joint pose estimation in non-line-of-sight conditions</title>
      <link>https://escholarship.org/uc/item/40z8z2d0</link>
      <description>Graph-based structural joint pose estimation in non-line-of-sight conditions</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/40z8z2d0</guid>
      <pubDate>Wed, 8 Nov 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Thoms, Alexander</name>
      </author>
      <author>
        <name>Al-Sabbag, Zaid</name>
      </author>
      <author>
        <name>Narasimhan, Sriram</name>
      </author>
    </item>
    <item>
      <title>Use of expanded shale, clay, and slate aggregates and biochar in the clear zone of road infrastructures for sustainable treatment of stormwater</title>
      <link>https://escholarship.org/uc/item/3bd9t73h</link>
      <description>A Clear Zone (CZ), the unobstructed roadside area with highly compacted soil, naturally accumulates high concentrations of pollutants from traffic activities. These pollutants are washed off by road runoff and enter waterways. In situ, treatment of polluted runoff from the CZ could not only protect water resources but also provide an opportunity to recharge groundwater. However, the soil in the CZ requires compaction, which limits the natural infiltration and treatment of road runoff. In this study, we examine whether and how amending the soil in the CZ with sand, a common bulking agent used in road design, and Expanded Shale, Clay, and Slate (ESCS) aggregates, a novel light-weight engineered bulking agent, could help treat stormwater in situ. ESCS-amended soil media infiltrated 220% more water than sand-amended soil under compaction, indicating that the addition of ESCS would make the CZ better at treating road runoff generated during high-intensity rainfall. Compared to sand-amended...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/3bd9t73h</guid>
      <pubDate>Wed, 8 Nov 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Das, Tonoy K</name>
      </author>
      <author>
        <name>Raoelison, Onja D</name>
      </author>
      <author>
        <name>Rehman, Hamid</name>
      </author>
      <author>
        <name>Zhang, Yuhui</name>
      </author>
      <author>
        <name>Chau, Wendy</name>
      </author>
      <author>
        <name>Thamiz, Lisa</name>
      </author>
      <author>
        <name>Stenstrom, Michael K</name>
      </author>
      <author>
        <name>Mohanty, Sanjay K</name>
      </author>
    </item>
    <item>
      <title>Full-Field Vibration Response Estimation from Sparse Multi-Agent Automatic Mobile Sensors Using Formation Control Algorithm</title>
      <link>https://escholarship.org/uc/item/2f09b53v</link>
      <description>In structural vibration response sensing, mobile sensors offer outstanding benefits as they are not dedicated to a certain structure; they also possess the ability to acquire dense spatial information. Currently, most of the existing literature concerning mobile sensing involves human drivers manually driving through the bridges multiple times. While self-driving automated vehicles could serve for such studies, they might entail substantial costs when applied to structural health monitoring tasks. Therefore, in order to tackle this challenge, we introduce a formation control framework that facilitates automatic multi-agent mobile sensing. Notably, our findings demonstrate that the proposed formation control algorithm can effectively control the behavior of the multi-agent systems for structural response sensing purposes based on user choice. We leverage vibration data collected by these mobile sensors to estimate the full-field vibration response of the structure, utilizing a...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/2f09b53v</guid>
      <pubDate>Thu, 26 Oct 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Jana, Debasish</name>
        <uri>https://orcid.org/0000-0003-2368-6394</uri>
      </author>
      <author>
        <name>Nagarajaiah, Satish</name>
      </author>
    </item>
    <item>
      <title>Techno-Economic Analysis of Solid Oxide Fuel Cell-Gas Turbine Hybrid Systems for Stationary Power Applications Using Renewable Hydrogen</title>
      <link>https://escholarship.org/uc/item/2xx7z0g4</link>
      <description>Solid oxide fuel cell (SOFC)–gas turbine (GT) hybrid systems can produce power at high electrical efficiencies while emitting virtually zero criteria pollutants (e.g., ozone, carbon monoxide, oxides of nitrogen and sulfur, and particulate matters). This study presents new insights into renewable hydrogen (RH2)-powered SOFC–GT hybrid systems with respect to their system configuration and techno-economic analysis motivated by the need for clean on-demand power. First, three system configurations are thermodynamically assessed: (I) a reference case with no SOFC off-gas recirculation, (II) a case with cathode off-gas recirculation, and (III) a case with anode off-gas recirculation. While these configurations have been studied in isolation, here we provide a detailed performance comparison. Moreover, a techno-economic analysis is conducted to study the economic competitiveness of RH2-fueled hybrid systems and the economies of scale by offering a comparison to natural gas (NG)-fueled...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/2xx7z0g4</guid>
      <pubDate>Wed, 4 Oct 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Chan, Chun Yin</name>
      </author>
      <author>
        <name>Rosner, Fabian</name>
      </author>
      <author>
        <name>Samuelsen, Scott</name>
      </author>
    </item>
    <item>
      <title>Rapid inverse design of metamaterials based on prescribed mechanical behavior through machine learning</title>
      <link>https://escholarship.org/uc/item/4q53q0fs</link>
      <description>Designing and printing metamaterials with customizable architectures enables the realization of unprecedented mechanical behaviors that transcend those of their constituent materials. These behaviors are recorded in the form of response curves, with stress-strain curves describing their quasi-static footprint. However, existing inverse design approaches are yet matured to capture the full desired behaviors due to challenges stemmed from multiple design objectives, nonlinear behavior, and process-dependent manufacturing errors. Here, we report a rapid inverse design methodology, leveraging generative machine learning and desktop additive manufacturing, which enables the creation of nearly all possible uniaxial compressive stress‒strain curve cases while accounting for process-dependent errors from printing. Results show that mechanical behavior with full tailorability can be achieved with nearly 90% fidelity between target and experimentally measured results. Our approach represents...</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/4q53q0fs</guid>
      <pubDate>Thu, 21 Sep 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Ha, Chan Soo</name>
      </author>
      <author>
        <name>Yao, Desheng</name>
      </author>
      <author>
        <name>Xu, Zhenpeng</name>
      </author>
      <author>
        <name>Liu, Chenang</name>
      </author>
      <author>
        <name>Liu, Han</name>
      </author>
      <author>
        <name>Elkins, Daniel</name>
      </author>
      <author>
        <name>Kile, Matthew</name>
      </author>
      <author>
        <name>Deshpande, Vikram</name>
      </author>
      <author>
        <name>Kong, Zhenyu</name>
      </author>
      <author>
        <name>Bauchy, Mathieu</name>
        <uri>https://orcid.org/0000-0003-4600-0631</uri>
      </author>
      <author>
        <name>Zheng, Xiaoyu Rayne</name>
      </author>
    </item>
    <item>
      <title>The Crystallization of Disordered Materials under Shock Is Governed by Their Network Topology</title>
      <link>https://escholarship.org/uc/item/9jt8d2b6</link>
      <description>When the shock load is applied, materials experience incredibly high temperature and pressure conditions on picosecond timescales, usually accompanied by remarkable physical or chemical phenomena. Understanding the underlying physics that governs the kinetics of shocked materials is of great importance for both physics and materials science. Here, combining experiment and large-scale molecular dynamics simulation, the ultrafast nanoscale crystal nucleation process in shocked soda-lime silicate glass is investigated. By adopting topological constraints theory, this study finds that the propensity of nucleation is governed by the connectivity of the atomic network. The densification of local networks, which appears once the crystal starts to grow, results in the underconstrained shell around the crystal and prevents further crystallization. These results shed light on the nanoscale crystallization mechanism of shocked materials from the viewpoint of topological constraint theory.</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/9jt8d2b6</guid>
      <pubDate>Thu, 14 Sep 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Tang, Longwen</name>
        <uri>https://orcid.org/0000-0001-7809-8720</uri>
      </author>
      <author>
        <name>Srivastava, Pratyush</name>
      </author>
      <author>
        <name>Gupta, Vijay</name>
      </author>
      <author>
        <name>Bauchy, Mathieu</name>
        <uri>https://orcid.org/0000-0003-4600-0631</uri>
      </author>
    </item>
    <item>
      <title>UV exposure to PET microplastics increases their downward mobility in stormwater biofilters undergoing freeze–thaw cycles</title>
      <link>https://escholarship.org/uc/item/8092q930</link>
      <description>An increase in microplastic weathering under UV lights decreases their surface hydrophilicity by the formation of polar groups and increases their mobility in the stormwater biofilter under freeze–thaw cycles.</description>
      <guid isPermaLink="true">https://escholarship.org/uc/item/8092q930</guid>
      <pubDate>Wed, 13 Sep 2023 00:00:00 +0000</pubDate>
      <author>
        <name>Gunther, Haley J</name>
      </author>
      <author>
        <name>Das, Tonoy K</name>
      </author>
      <author>
        <name>Leonard, Jamie</name>
      </author>
      <author>
        <name>Koutnik, Vera S</name>
      </author>
      <author>
        <name>Rassi, Lea A El</name>
      </author>
      <author>
        <name>Tang, Zilong</name>
      </author>
      <author>
        <name>Mohanty, Sanjay K</name>
      </author>
    </item>
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