The Fate of the Compact Remnant in Neutron Star Mergers

Fryer, Chris L.; Belczynski, Krzysztoff; Ramirez-Ruiz, Enrico; Rosswog, Stephan; Shen, Gang; Steiner, Andrew W.

doi:10.1088/0004-637X/812/1/24

The Fate of the Compact Remnant in Neutron Star Mergers

Journal Article · Tue Oct 06 00:00:00 EDT 2015 · The Astrophysical Journal (Online)

DOI:https://doi.org/10.1088/0004-637X/812/1/24· OSTI ID:1265719

Fryer, Chris L. ^[1]; Belczynski, Krzysztoff ^[2]; Ramirez-Ruiz, Enrico ^[3]; Rosswog, Stephan ^[4]; Shen, Gang ^[5]; Steiner, Andrew W. ^[6]

Univ. of Arizona, Tucson, AZ (United States); Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
Univ. of Warsaw (Poland)
Univ. of California, Santa Cruz, CA (United States)
Stockholm Univ. (Sweden)
Univ. of Washington, Seattle, WA (United States)
Univ. of Tennessee, Knoxville, TN (United States); Oak Ridge National Lab. (ORNL), Oak Ridge, TN (United States)

Neutron star (binary neutron star and neutron star - black hole) mergers are believed to produce short-duration gamma-ray bursts. They are also believed to be the dominant source of gravitational waves to be detected by the advanced LIGO and the dominant source of the heavy r-process elements in the universe. Whether or not these mergers produce short-duration GRBs depends sensitively on the fate of the core of the remnant (whether, and how quickly, it forms a black hole). In this paper, we combine the results of merger calculations and equation of state studies to determine the fate of the cores of neutron star mergers. Using population studies, we can determine the distribution of these fates to compare to observations. We find that black hole cores form quickly only for equations of state that predict maximum non-rotating neutron star masses below 2.3-2.4 solar masses. If quick black hole formation is essential in producing gamma-ray bursts, LIGO observed rates compared to GRB rates could be used to constrain the equation of state for dense nuclear matter.

View Accepted Manuscript (DOE)

Research Organization:: Los Alamos National Lab. (LANL), Los Alamos, NM (United States); Oak Ridge National Laboratory (ORNL), Oak Ridge, TN (United States). Joint Institute for Computational Sciences (JICS)

Sponsoring Organization:: USDOE; USDOE Office of Science (SC)

Grant/Contract Number:: AC05-00OR22725; AC52-06NA25396

OSTI ID:: 1265719

Alternate ID(s):: OSTI ID: 1324567
OSTI ID: 22518864

Report Number(s):: LA-UR--15-22916; KB0301020; ERKBP05

Journal Information:: The Astrophysical Journal (Online), Journal Name: The Astrophysical Journal (Online) Journal Issue: 1 Vol. 812; ISSN 1538-4357

Publisher:: Institute of Physics (IOP)Copyright Statement

Country of Publication:: United States

Language:: English

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