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Soma Mukherjee

Researcher at University of Texas at Austin

Publications -  280
Citations -  72580

Soma Mukherjee is an academic researcher from University of Texas at Austin. The author has contributed to research in topics: LIGO & Gravitational wave. The author has an hindex of 95, co-authored 266 publications receiving 59549 citations. Previous affiliations of Soma Mukherjee include The University of Texas Rio Grande Valley & Saha Institute of Nuclear Physics.

Papers
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Journal ArticleDOI

Population Properties of Compact Objects from the Second LIGO-Virgo Gravitational-Wave Transient Catalog

Richard J. Abbott, +1431 more
TL;DR: In this article, the population of 47 compact binary mergers detected with a false-alarm rate of 0.614 were dynamically assembled, and the authors found that the BBH rate likely increases with redshift, but not faster than the star formation rate.
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Binary Black Hole Population Properties Inferred from the First and Second Observing Runs of Advanced LIGO and Advanced Virgo

B. P. Abbott, +1218 more
TL;DR: In this paper, the mass, spin, and redshift distributions of binary black hole (BBH) mergers with LIGO and Advanced Virgo observations were analyzed using phenomenological population models.
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Tests of General Relativity with GW170817

B. P. Abbott, +1240 more
TL;DR: In this paper, the authors place constraints on the dipole radiation and possible deviations from GR in the post-Newtonian coefficients that govern the inspiral regime of a binary neutron star inspiral.
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GW150914: First results from the search for binary black hole coalescence with Advanced LIGO

B. P. Abbott, +980 more
- 07 Jun 2016 - 
TL;DR: In this paper, the results of a matched-filter search using relativistic models of compact-object binaries that recovered GW150914 as the most significant event during the coincident observations between the two LIGO detectors were reported.
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Observation of Gravitational Waves from Two Neutron Star–Black Hole Coalescences

Richard J. Abbott, +1695 more
TL;DR: In this article, the authors reported the observation of gravitational waves from two compact binary coalescences in LIGO's and Virgo's third observing run with properties consistent with neutron star-black hole (NSBH) binaries.