Constraining the neutron-matter equation of state with gravitational waves

We show how observations of gravitational waves from binary neutron star (BNS) mergers over the next few years can be combined with insights from nuclear physics to obtain useful constraints on the equation of state (EoS) of dense matter. In particular, the neutron-matter EoS between 1 and 2 times t...

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Veröffentlicht in:	Physical review. D 2019-10, Vol.100 (8), Article 083010
Hauptverfasser:	Forbes, Michael McNeil, Bose, Sukanta, Reddy, Sanjay, Zhou, Dake, Mukherjee, Arunava, De, Soumi
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy & Astrophysics ASTRONOMY AND ASTROPHYSICS Binary stars Computer simulation Constraint modelling Equations of state Gravitation Gravitational waves Neutron stars Neutrons Nuclear matter Nuclear physics Parameter identification Parameter sensitivity Phase transitions Physics Principal components analysis Sensitivity X-ray astronomy
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