Hyperonic neutron star matter in light of GW170817
Sign Up to like & getrecommendations! Published in 2019 at "Astronomische Nachrichten"
DOI: 10.1002/asna.201913579
Abstract: Since 2013 the mass of pulsar PSR J0348+0432 ($M = 2.01\,M_{\odot}$) has provided a tight constraint on neutron star equation of state. However, a number of different analyses of the recently detected BNS merger (GW170817)… read more here.
Keywords: matter light; mass; neutron star; star matter ... See more keywords
Constraints on the equation of state of neutron star matter based on observations
Sign Up to like & getrecommendations! Published in 2017 at "Modern Physics Letters A"
DOI: 10.1142/s0217732317501905
Abstract: Many calculations of the neutron star (NS) equation of state (EOS) have been performed over the years. Recent observations of NSs have begun to play an important role in finding the realistic EOS. In this… read more here.
Keywords: state neutron; constraints equation; equation state; neutron star ... See more keywords