Los Alamos National Laboratory

Los Alamos National Laboratory

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Fate of the Compact Remnant in Neutron Star Mergers

NASA illustration of a binary neutron star system

Illustration of a binary neutron star system in the process of merging. The remnant formed by this merger could be either a neutron star or a black hole, determining whether it launches a gamma-ray burst. [NASA]

What Do You Get When Two Neutron Stars Merge?

Neutron star (binary neutron star and neutron star–black hole) mergers are believed to produce short-duration gamma-ray bursts (GRBs). They are also believed to be the dominant source of gravitational waves to be detected by the advanced LIGO and advanced VIRGO 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). We've combined the results of Newtonian 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 GRBs, LIGO/Virgo observed rates compared to GRB rates could be used to constrain the equation of state for dense nuclear matter.

American Astronomical Society journal article


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