Spectral properties of the post-merger gravitational-wave signal from binary neutron stars
Kentaro TakamiInstitut für Theoretische Physik, Max-von-Laue-Straße 1, 60438 Frankfurt, GermanyLuciano RezzollaInstitut für Theoretische Physik, Max-von-Laue-Straße 1, 60438 Frankfurt, GermanyLuca BaiottiGraduate School of Science, Osaka University, 560-0043 Toyonaka, Japan
2015en
ABI
Аннотация
Can gravitational waves from merging neutron star binaries be used to determine characteristics of neutron stars? Extensive numerical relativity simulations reported here show that these signals can be used to set constraints on the equation of state and other features of merging neutron stars.
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