Nuclear Science
Parent: Physical Sciences
eScholarship stats: Breakdown by Item for May through August, 2024
| Item | Title | Total requests | Download | View-only | %Dnld |
|---|---|---|---|---|---|
| 8833b038 | Review of Particle Physics | 180 | 52 | 128 | 28.9% |
| 16m3r325 | Search for exotic decays of the Higgs boson to a pair of pseudoscalars in the μμbb and ττbb final states. | 145 | 42 | 103 | 29.0% |
| 9vg4k6g6 | Higher-order correlations between different moments of two flow amplitudes in Pb-Pb collisions at sNN=5.02 TeV | 122 | 21 | 101 | 17.2% |
| 11k10948 | The Physics of the B Factories | 121 | 7 | 114 | 5.8% |
| 1s79s9bj | Thermal conductivity measurements of PTFE and Al2O3 ceramic at sub-Kelvin temperatures | 114 | 15 | 99 | 13.2% |
| 9sw1s6k8 | Search for lepton-flavor-violating decays D0→X0e±μ∓ | 105 | 20 | 85 | 19.0% |
| 92z0x9td | Modeling backward-angle (u-channel) virtual Compton scattering at the future Electron-Ion Collider | 104 | 20 | 84 | 19.2% |
| 9fb704x9 | Comparative scintillation performance of EJ-309, EJ-276, and a novel organic glass | 104 | 24 | 80 | 23.1% |
| 7dj1d5sr | Design of the Superconducting Magnet System for a 45 GHz ECR Ion Source | 101 | 18 | 83 | 17.8% |
| 8bd7v3bb | KamLAND’s search for correlated low-energy electron antineutrinos with astrophysical neutrinos from IceCube | 98 | 25 | 73 | 25.5% |
| 70w6x41n | The BABAR detector | 97 | 67 | 30 | 69.1% |
| 3k1843rw | Bulk properties of the system formed in Au+Au collisions at sNN=14.5 GeV at the BNL STAR detector | 96 | 26 | 70 | 27.1% |
| 4bg298ms | Search for neutrino lines from dark matter annihilation and decay with IceCube | 94 | 32 | 62 | 34.0% |
| 6831d5df | Spectroscopic study of a possible Λnn resonance and a pair of ΣNN states using the (e,e′K+) reaction with a tritium target | 94 | 21 | 73 | 22.3% |
| 45r822p9 | Polaris-LAMP: Multi-Modal 3-D Image Reconstruction With a Commercial Gamma-Ray Imager | 92 | 12 | 80 | 13.0% |
| 58r3c4sx | Can We Detect the Quantum Nature of Weak Gravitational Fields? | 92 | 20 | 72 | 21.7% |
| 8r37x6z9 | Constraints on neutrino emission from nearby galaxies using the 2MASS redshift survey and IceCube | 92 | 29 | 63 | 31.5% |
| 79g6x7k4 | Characterization of cubic Li2100MoO4 crystals for the CUPID experiment | 91 | 18 | 73 | 19.8% |
| 7sr999w8 | Machine Learning Techniques for Pile-Up Rejection in Cryogenic Calorimeters | 91 | 20 | 71 | 22.0% |
| 0mx946m8 | Search for GeV-scale dark matter annihilation in the Sun with IceCube DeepCore | 90 | 25 | 65 | 27.8% |
| 82p3s3qf | Real-Time Free-Moving Active Coded Mask 3D Gamma-Ray Imaging | 90 | 11 | 79 | 12.2% |
| 8mm255dc | Excitation functions for (p,x) reactions of niobium in the energy range of Ep = 40–90 MeV | 90 | 18 | 72 | 20.0% |
| 5m605672 | Detailed analysis of excited state systematics in a lattice QCD calculation of $g_A$ | 88 | 19 | 69 | 21.6% |
| 82x5v66c | ADC Nonlinearity Correction for the Majorana Demonstrator | 88 | 17 | 71 | 19.3% |
| 9cr1b30s | Modification of Z 0 leptonic invariant mass in ultrarelativistic heavy ion collisions as a measure of the electromagnetic field | 88 | 16 | 72 | 18.2% |
| 9q3550m0 | Three-pion Hanbury-Brown-Twiss correlations in relativistic heavy-ion collisions from the STAR experiment | 88 | 3 | 85 | 3.4% |
| 1pp29372 | Multihadronic events at Ec.m.=29 GeV and predictions of QCD models from Ec.m.=29 GeV to Ec.m.=93 GeV | 87 | 13 | 74 | 14.9% |
| 8rq0t2fp | CUORE opens the door to tonne-scale cryogenics experiments | 87 | 16 | 71 | 18.4% |
| 2qm3f1tr | Lattice determination of I=0 and 2 ππ scattering phase shifts with a physical pion mass | 85 | 24 | 61 | 28.2% |
| 68g1b51r | Measurement of transverse single-spin asymmetries of π0 and electromagnetic jets at forward rapidity in 200 and 500 GeV transversely polarized proton-proton collisions | 85 | 10 | 75 | 11.8% |
| 8pp9z5bd | Precise measurement of 2νββ decay of 100Mo with the CUPID-Mo detection technology | 85 | 13 | 72 | 15.3% |
| 6j8510dj | Initial performance of the CUORE-0 experiment | 84 | 16 | 68 | 19.0% |
| 79f5x4p5 | Strange hadron production in Au+Au collisions at sNN=7.7, 11.5, 19.6, 27, and 39 GeV | 84 | 20 | 64 | 23.8% |
| 5p28d02g | Measurement of R=σL/σT and the separated longitudinal and transverse structure functions in the nucleon-resonance region | 83 | 22 | 61 | 26.5% |
| 61v5b2r5 | Probing criticality with deep learning in relativistic heavy-ion collisions | 83 | 21 | 62 | 25.3% |
| 8r63g6j5 | Observation of Decays B0→Ds(*)+π- and B0→Ds(*)-K+ | 83 | 5 | 78 | 6.0% |
| 0h90n84d | Follow-up of Astrophysical Transients in Real Time with the IceCube Neutrino Observatory | 82 | 18 | 64 | 22.0% |
| 7sg6q500 | Search for decays of stopped long-lived particles produced in proton-proton collisions at [Formula: see text]. | 82 | 10 | 72 | 12.2% |
| 9sm0m9bx | Classification and asymptotic scaling of the light-cone wave-function amplitudes of hadrons | 82 | 6 | 76 | 7.3% |
| 3fs0d0q3 | Status and prospects for CUORE | 81 | 19 | 62 | 23.5% |
| 3tr0t9cz | Differential measurements of jet substructure and partonic energy loss in Au + Au collisions at sNN=200 GeV | 81 | 22 | 59 | 27.2% |
| 0qs49185 | The Majorana Demonstrator Status and Preliminary Results | 80 | 16 | 64 | 20.0% |
| 127666wd | Search for annihilating dark matter in the Sun with 3 years of IceCube data | 80 | 53 | 27 | 66.3% |
| 7k08x5t6 | Smeared quasidistributions in perturbation theory | 80 | 11 | 69 | 13.8% |
| 7s653698 | Amplitude analysis of the decay B±→π±π±π∓ | 79 | 6 | 73 | 7.6% |
| 93h2g9hr | Measurement of |Vcb| and the Form-Factor Slope in B¯→Dℓ-ν¯ℓ Decays in Events Tagged by a Fully Reconstructed B Meson | 79 | 4 | 75 | 5.1% |
| 09v3h754 | Effect of event selection on jetlike correlation measurement in d+Au collisions at sNN=200 GeV | 78 | 5 | 73 | 6.4% |
| 49z6k2v9 | Search for Long-Lived Particles in e+e- Collisions | 78 | 8 | 70 | 10.3% |
| 07d4s18x | Studies of jet production rates ine+e− annihilation atEcm=29 GeV | 77 | 8 | 69 | 10.4% |
| 996843fd | Erratum to: Dispersive corrections in elastic electron-nucleus scattering: an investigation in the intermediate energy regime and their impact on the nuclear matter | 77 | 6 | 71 | 7.8% |
Note: Due to the evolving nature of web traffic, the data presented here should be considered approximate and subject to revision. Learn more.