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Literature DB >> 30003183

GW170817, general relativistic magnetohydrodynamic simulations, and the neutron star maximum mass.

Milton Ruiz¹, Stuart L Shapiro^1,2, Antonios Tsokaros¹.

Abstract

Recent numerical simulations in general relativistic magnetohydrodynamics (GRMHD) provide useful constraints for the interpretation of the GW170817 discovery. Combining the observed data with these simulations leads to a bound on the maximum mass of a cold, spherical neutron star (the TOV limit): Mmaxsph≲2.74/β , where β is the ratio of the maximum mass of a uniformly rotating neutron star (the supramassive limit) over the maximum mass of a nonrotating star. Causality arguments allow β to be as high as 1.27, while most realistic candidate equations of state predict β to be closer to 1.2, yielding Mmaxsph in the range 2.16-2.28M⊙. A minimal set of assumptions based on these simulations distinguishes this analysis from previous ones, but leads a to similar estimate. There are caveats, however, and they are enumerated and discussed. The caveats can be removed by further simulations and analysis to firm up the basic argument.

Entities: Chemical

Year: 2018 PMID： 30003183 PMCID： PMC6036631 DOI： 10.1103/PhysRevD.97.021501

Source DB: PubMed Journal: Phys Rev D ISSN： 2470-0010 Impact factor: 5.296

14 in total

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Journal: Astrophys J Date: 2000-01-01 Impact factor: 5.874

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Authors: P B Demorest; T Pennucci; S M Ransom; M S E Roberts; J W T Hessels
Journal: Nature Date: 2010-10-28 Impact factor: 49.962

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Authors: D B Fox; D A Frail; P A Price; S R Kulkarni; E Berger; T Piran; A M Soderberg; S B Cenko; P B Cameron; A Gal-Yam; M M Kasliwal; D-S Moon; F A Harrison; E Nakar; B P Schmidt; B Penprase; R A Chevalier; P Kumar; K Roth; D Watson; B L Lee; S Shectman; M M Phillips; M Roth; P J McCarthy; M Rauch; L Cowie; B A Peterson; J Rich; N Kawai; K Aoki; G Kosugi; T Totani; H-S Park; A MacFadyen; K C Hurley
Journal: Nature Date: 2005-10-06 Impact factor: 49.962

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Authors: Masaru Shibata
Journal: Phys Rev Lett Date: 2005-05-25 Impact factor: 9.161

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Journal: Phys Rev Lett Date: 2013-09-25 Impact factor: 9.161

6. Binary neutron star mergers: a review of Einstein's richest laboratory.

Authors: Luca Baiotti; Luciano Rezzolla
Journal: Rep Prog Phys Date: 2017-03-20

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Authors: Milton Ruiz; Ryan N Lang; Vasileios Paschalidis; Stuart L Shapiro
Journal: Astrophys J Lett Date: 2016-06-03 Impact factor: 7.413

8. A massive pulsar in a compact relativistic binary.

Authors: John Antoniadis; Paulo C C Freire; Norbert Wex; Thomas M Tauris; Ryan S Lynch; Marten H van Kerkwijk; Michael Kramer; Cees Bassa; Vik S Dhillon; Thomas Driebe; Jason W T Hessels; Victoria M Kaspi; Vladislav I Kondratiev; Norbert Langer; Thomas R Marsh; Maura A McLaughlin; Timothy T Pennucci; Scott M Ransom; Ingrid H Stairs; Joeri van Leeuwen; Joris P W Verbiest; David G Whelan
Journal: Science Date: 2013-04-26 Impact factor: 47.728

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10. The afterglow and elliptical host galaxy of the short gamma-ray burst GRB 050724.

Authors: E Berger; P A Price; S B Cenko; A Gal-Yam; A M Soderberg; M Kasliwal; D C Leonard; P B Cameron; D A Frail; S R Kulkarni; D C Murphy; W Krzeminski; T Piran; B L Lee; K C Roth; D-S Moon; D B Fox; F A Harrison; S E Persson; B P Schmidt; B E Penprase; J Rich; B A Peterson; L L Cowie
Journal: Nature Date: 2005-12-15 Impact factor: 49.962

8 in total

1. Neutron stars harboring a primordial black hole: Maximum survival time.

Authors: Thomas W Baumgarte; Stuart L Shapiro
Journal: Phys Rev D Date: 2021-04-22 Impact factor: 5.296

2. Black hole-neutron star coalescence: Effects of the neutron star spin on jet launching and dynamical ejecta mass.

Authors: Milton Ruiz; Vasileios Paschalidis; Antonios Tsokaros; Stuart L Shapiro
Journal: Phys Rev D Date: 2020-12-20 Impact factor: 5.296

3. Relativistic Bondi accretion for stiff equations of state.

Authors: Chloe B Richards; Thomas W Baumgarte; Stuart L Shapiro
Journal: Mon Not R Astron Soc Date: 2021-01-20 Impact factor: 5.287

Review 4. Kilonovae.

Authors: Brian D Metzger
Journal: Living Rev Relativ Date: 2019-12-16 Impact factor: 40.429