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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.

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Journal ArticleDOI

Model Comparison from LIGO-Virgo Data on GW170817's Binary Components and Consequences for the Merger Remnant

B. P. Abbott, +1280 more
TL;DR: In this paper, the authors perform Bayesian model selection on a wide range of theoretical predictions for the neutron star equation of state, and find that all scenarios from prompt collapse to long-lived or even stable remnants are possible.
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Einstein@Home all-sky search for periodic gravitational waves in LIGO S5 data

J. Aasi, +888 more
- 13 Feb 2013 - 
TL;DR: In this paper, the results of an all-sky search for periodic gravitational waves in the frequency range [50, 1190] Hz and with frequency derivative range of similar to [-20, 1.1] x 10(-10) Hz s(-1) for the fifth LIGO science run (S5) are presented.
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Improved Analysis of GW150914 Using a Fully Spin-Precessing Waveform Model

B. P. Abbott, +1001 more
- 21 Oct 2016 - 
TL;DR: In this paper, a 15-dimensional precessing-spin waveform model (precessing EOBNR) was developed within the EOB formalism for GW150914.
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Search for gravitational-wave bursts in the first year of the fifth LIGO science run

B. P. Abbott, +501 more
- 11 Nov 2009 - 
TL;DR: In this paper, the results obtained from an all-sky search for gravitational-wave (GW) bursts in the 64 −======2000 Hz frequency range in data collected by the LIGO detectors during the first year (November 2005-======November 2006) of their fifth science run were presented.
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Directional limits on persistent gravitational waves using LIGO S5 science data

J. Abadie, +720 more
TL;DR: Two directional searches for persistent GWs using data from the LIGO S5 science run are performed: one optimized for pointlike sources and one for arbitrary extended sources, finding no evidence to support the detection of GWs.