Matches in SemOpenAlex for { <https://semopenalex.org/work/W2610725191> ?p ?o ?g. }
- W2610725191 endingPage "L19" @default.
- W2610725191 startingPage "L19" @default.
- W2610725191 abstract "Following merger, a neutron star (NS) binary can produce roughly one of three different outcomes: (1) a stable NS, (2) a black hole (BH), or (3) a supramassive, rotationally supported NS, which then collapses to a BH following angular momentum losses. Which of these fates occur and in what proportion has important implications for the electromagnetic transient associated with the mergers and the expected gravitational wave (GW) signatures, which in turn depend on the high density equation of state (EOS). Here we combine relativistic calculations of NS masses using realistic EOSs with Monte Carlo population synthesis based on the mass distribution of NS binaries in our Galaxy to predict the distribution of fates expected. For many EOSs, a significant fraction of the remnants are NSs or supramassive NSs. This lends support to scenarios in which a quickly spinning, highly magnetized NS may be powering an electromagnetic transient. This also indicates that it will be important for future GW observatories to focus on high frequencies to study the post-merger GW emission. Even in cases where individual GW events are too low in signal to noise to study the post merger signature in detail, the statistics of how many mergers produce NSs versus BHs can be compared with our work to constrain the EOS. To match short gamma-ray-burst (SGRB) X-ray afterglow statistics, we find that the stiffest EOSs are ruled out. Furthermore, many popular EOSs require a significant fraction of ∼60%–70% of SGRBs to be from NS–BH mergers rather than just binary NSs." @default.
- W2610725191 created "2017-05-12" @default.
- W2610725191 creator A5037828745 @default.
- W2610725191 creator A5061358030 @default.
- W2610725191 creator A5064913713 @default.
- W2610725191 date "2017-07-27" @default.
- W2610725191 modified "2023-10-02" @default.
- W2610725191 title "The Fate of Neutron Star Binary Mergers" @default.
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