Equation of state constraints from the threshold binary mass for prompt collapse of neutron star mergers

Using hydrodynamical simulations for a large set of high-density matter equations of state (EoSs) we systematically determine the threshold mass M_thres for prompt black-hole formation in equal-mass and asymmetric neutron star (NS) mergers. We devise the so far most direct, general and accurate meth...

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Main Authors Bauswein, Andreas, Blacker, Sebastian, Vijayan, Vimal, Stergioulas, Nikolaos, Chatziioannou, Katerina, Clark, James A, Bastian, Niels-Uwe F, Blaschke, David B, Cierniak, Mateusz, Fischer, Tobias
Format Paper Journal Article
LanguageEnglish
Published Ithaca Cornell University Library, arXiv.org 06.10.2020
Subjects
Binary stars
Black holes
Equations of state
Gravitational collapse
Gravitational waves
Neutron stars
Phase transitions
Physics - High Energy Astrophysical Phenomena
Physics - High Energy Physics - Phenomenology
Physics - Nuclear Theory
Quarks
Star mergers
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Abstract Using hydrodynamical simulations for a large set of high-density matter equations of state (EoSs) we systematically determine the threshold mass M_thres for prompt black-hole formation in equal-mass and asymmetric neutron star (NS) mergers. We devise the so far most direct, general and accurate method to determine the unknown maximum mass of nonrotating NSs from merger observations revealing M_thres. Considering hybrid EoSs with hadron-quark phase transition, we identify a new, observable signature of quark matter in NS mergers. Furthermore, our findings have direct applications in gravitational wave searches, kilonova interpretations and multi-messenger constraints on NS properties.
AbstractList Using hydrodynamical simulations for a large set of high-density matter equations of state (EoSs) we systematically determine the threshold mass M_thres for prompt black-hole formation in equal-mass and asymmetric neutron star (NS) mergers. We devise the so far most direct, general and accurate method to determine the unknown maximum mass of nonrotating NSs from merger observations revealing M_thres. Considering hybrid EoSs with hadron-quark phase transition, we identify a new, observable signature of quark matter in NS mergers. Furthermore, our findings have direct applications in gravitational wave searches, kilonova interpretations and multi-messenger constraints on NS properties.
Phys. Rev. Lett. 125, 141103 (2020) Using hydrodynamical simulations for a large set of high-density matter equations of state (EoSs) we systematically determine the threshold mass M_thres for prompt black-hole formation in equal-mass and asymmetric neutron star (NS) mergers. We devise the so far most direct, general and accurate method to determine the unknown maximum mass of nonrotating NSs from merger observations revealing M_thres. Considering hybrid EoSs with hadron-quark phase transition, we identify a new, observable signature of quark matter in NS mergers. Furthermore, our findings have direct applications in gravitational wave searches, kilonova interpretations and multi-messenger constraints on NS properties.
Author Vijayan, Vimal
Blaschke, David B
Chatziioannou, Katerina
Stergioulas, Nikolaos
Bauswein, Andreas
Clark, James A
Fischer, Tobias
Blacker, Sebastian
Cierniak, Mateusz
Bastian, Niels-Uwe F
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BackLink https://doi.org/10.1103/PhysRevLett.125.141103$$DView published paper (Access to full text may be restricted)
https://doi.org/10.48550/arXiv.2004.00846$$DView paper in arXiv
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Snippet Using hydrodynamical simulations for a large set of high-density matter equations of state (EoSs) we systematically determine the threshold mass M_thres for...
Phys. Rev. Lett. 125, 141103 (2020) Using hydrodynamical simulations for a large set of high-density matter equations of state (EoSs) we systematically...
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SubjectTerms Binary stars
Black holes
Equations of state
Gravitational collapse
Gravitational waves
Neutron stars
Phase transitions
Physics - High Energy Astrophysical Phenomena
Physics - High Energy Physics - Phenomenology
Physics - Nuclear Theory
Quarks
Star mergers
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Title Equation of state constraints from the threshold binary mass for prompt collapse of neutron star mergers
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