Although much research examines how physicians perceive their patients, here we study how patients perceive physicians. We propose patients consider their physicians like personally emotionless “empty vessels”: The higher is individuals’ need for care, the less they value physicians’ traits related to their personal lives (e.g., self-focused emotions), but the more they value physicians’ traits related to patients (e.g., patient-focused emotions). In an initial study, participants recalled fewer personal facts (e.g., marital status) about physicians who seemed more important to their health. In subsequent experiments, participants in higher need for care believed physicians have less personal emotions. Although higher need individuals, such as patients in a clinic, perceived their physicians to be personally emotionless, they wanted the clinic to hire physicians who displayed patient-focused emotion. We discuss implications of perceiving physicians as empty vessels for health care.

To achieve goals, individuals and organizations must understand how to effectively motivate themselves and others. We review three broad strategies that people employ to increase motivation: giving feedback, setting goal targets, and applying incentives. Although each of these strategies can effectively motivate action under certain circumstances and among certain people, they can also result in unintended consequences: not helping or even hurting motivation. For example, employers may give positive feedback that leads employees to relax their effort or negative feedback that undermines employees' commitment, organizations may set goals that are overly ambitious and consequently reduce motivation, and certain incentives might appear attractive before pursuing an action but uncertain incentives better motivate action during goal pursuit. By identifying when and how these common motivational strategies work versus fail, we are able to prescribe a specific set of guidelines that will help people understand how to motivate themselves and others.

Intimacy is often motivated by love, but sometimes it is merely functional. For example, disrobing and being touched at an airport security check serves the goal of catching a flight, not building a relationship. We propose that this functional intimacy induces discomfort, making people prefer greater social distance from their interaction partner. Supporting this prediction, participants who considered (Experiments 1 and 2) or experienced (Experiment 3) more physically intimate medical procedures preferred a health provider who is less social. Increased psychological intimacy also led people to prefer social distance from cleaning and health providers (Experiments 4-5), a preference revealed by nonverbal behavior (e.g., turning away and looking away, Experiments 6-7). These patterns of distancing are unique to functional (vs. romantic) intimacy (Experiment 7). Although creating social distance may be an effective strategy for coping with functional intimacy, it may have costs for service providers.

Intimacy is often motivated by love, but sometimes it is merely functional. For example, disrobing and being touched at an airport security check serves the goal of catching a flight, not building a relationship. We propose that this functional intimacy induces discomfort, making people prefer greater social distance from their interaction partner. Supporting this prediction, participants who considered (Experiments 1 and 2) or experienced (Experiment 3) more physically intimate medical procedures preferred a health provider who is less social. Increased psychological intimacy also led people to prefer social distance from cleaning and health providers (Experiments 4-5), a preference revealed by nonverbal behavior (e.g., turning away and looking away, Experiments 6-7). These patterns of distancing are unique to functional (vs. romantic) intimacy (Experiment 7). Although creating social distance may be an effective strategy for coping with functional intimacy, it may have costs for service providers. (PsycINFO Database Record

We present a search for continuous gravitational waves from five radio pulsars, comprising three recycled pulsars (PSR J0437-4715, PSR J0711-6830, and PSR J0737-3039A) and two young pulsars: the Crab pulsar (J0534+2200) and the Vela pulsar (J0835-4510). We use data from the third observing run of Advanced LIGO and Virgo combined with data from their first and second observing runs. For the first time, we are able to match (for PSR J0437-4715) or surpass (for PSR J0711-6830) the indirect limits on gravitational-wave emission from recycled pulsars inferred from their observed spin-downs, and constrain their equatorial ellipticities to be less than 10-8. For each of the five pulsars, we perform targeted searches that assume a tight coupling between the gravitational-wave and electromagnetic signal phase evolution. We also present constraints on PSR J0711-6830, the Crab pulsar, and the Vela pulsar from a search that relaxes this assumption, allowing the gravitational-wave signal to vary from the electromagnetic expectation within a narrow band of frequencies and frequency derivatives.

We present a search for quasi-monochromatic gravitational-wave signals from the young, energetic X-ray pulsar PSR J0537-6910 using data from the second and third observing runs of LIGO and Virgo. The search is enabled by a contemporaneous timing ephemeris obtained using Neutron star Interior Composition Explorer (NICER) data. The NICER ephemeris has also been extended through 2020 October and includes three new glitches. PSR J0537-6910 has the largest spin-down luminosity of any pulsar and exhibits fRequent and strong glitches. Analyses of its long-term and interglitch braking indices provide intriguing evidence that its spin-down energy budget may include gravitational-wave emission from a time-varying mass quadrupole moment. Its 62 Hz rotation frequency also puts its possible gravitational-wave emission in the most sensitive band of the LIGO/Virgo detectors. Motivated by these considerations, we search for gravitational-wave emission at both once and twice the rotation frequency from PSR J0537-6910. We find no signal, however, and report upper limits. Assuming a rigidly rotating triaxial star, our constraints reach below the gravitational-wave spin-down limit for this star for the first time by more than a factor of 2 and limit gravitational waves from the l = m = 2 mode to account for less than 14% of the spin-down energy budget. The fiducial equatorial ellipticity is constrained to less than about 3 ×10-5, which is the third best constraint for any young pulsar.