Compassion Predictors in Undergraduates: A Catholic College Example

Compassion is sorely needed in contemporary society, including within faith-based colleges. Past research has examined the prevention of compassion fatigue in healthcare professions, but relatively little research exists on the predictors of compassion, particularly among student populations. This study examines the factors associated with higher compassion levels in graduating college seniors, revealing demographic, experiential, and beliefrelated factors contributing to compassion. Results suggest that the general profile of a highly compassionate graduating college senior is a student who is female, politically liberal, religious, studying the natural or social sciences, actively involved in community service or volunteering, and who has undergone workshops on racial/cultural awareness and sensitivity

Compassion development in higher education

Many schools of psychology and religious studies intend to promote the cultivation of compassion. Compassion is currently an integral area of study in psychology, religious studies, and higher education, specifically in faith-based higher education. While secular universities in the United States strive to generate disciplinary-based knowledge through scholarship, their ability to promote students\u27 use of the information they are learning to create positive social change has typically lagged. Conscious of the magnitude of today\u27s global issues and dissatisfied with the current disparity between the world\u27s reality and university curricula, scholars have begun to re-imagine the role of higher education in forming the leaders who will face our most exigent problems. The present article reviews how compassion can be integrated into university curriculum, specifically in faith-based institutions. The article also discusses how compassion can be measured throughout the course of undergraduates\u27 careers

Search for intermediate-mass black hole binaries in the third observing run of Advanced LIGO and Advanced Virgo

International audienceIntermediate-mass black holes (IMBHs) span the approximate mass range 100−105 M⊙, between black holes (BHs) that formed by stellar collapse and the supermassive BHs at the centers of galaxies. Mergers of IMBH binaries are the most energetic gravitational-wave sources accessible by the terrestrial detector network. Searches of the first two observing runs of Advanced LIGO and Advanced Virgo did not yield any significant IMBH binary signals. In the third observing run (O3), the increased network sensitivity enabled the detection of GW190521, a signal consistent with a binary merger of mass ∼150 M⊙ providing direct evidence of IMBH formation. Here, we report on a dedicated search of O3 data for further IMBH binary mergers, combining both modeled (matched filter) and model-independent search methods. We find some marginal candidates, but none are sufficiently significant to indicate detection of further IMBH mergers. We quantify the sensitivity of the individual search methods and of the combined search using a suite of IMBH binary signals obtained via numerical relativity, including the effects of spins misaligned with the binary orbital axis, and present the resulting upper limits on astrophysical merger rates. Our most stringent limit is for equal mass and aligned spin BH binary of total mass 200 M⊙ and effective aligned spin 0.8 at 0.056 Gpc−3 yr−1 (90% confidence), a factor of 3.5 more constraining than previous LIGO-Virgo limits. We also update the estimated rate of mergers similar to GW190521 to 0.08 Gpc−3 yr−1.Key words: gravitational waves / stars: black holes / black hole physicsCorresponding author: W. Del Pozzo, e-mail: [email protected]† Deceased, August 2020