Impact of the neutron-star deformability on equation of state parameters
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DOI: 10.1103/physrevc.102.045808
Abstract: We use a Bayesian inference analysis to explore the sensitivity of Taylor expansion parameters of the nuclear equation of state (EOS) to the neutron star dimensionless tidal deformability ($\mathrm{\ensuremath{\Lambda}}$) on 1- to 2-solar-mass neutron stars.… read more here.
Keywords: text sym; equation state; neutron star; deformability ... See more keywords
Upper limit set by causality on the tidal deformability of a neutron star
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DOI: 10.1103/physrevd.95.083014
Abstract: A principal goal of gravitational-wave astronomy is to constrain the neutron star equation of state (EOS) by measuring the tidal deformability of neutron stars. The tidally induced departure of the waveform from that of point-particle… read more here.
Keywords: tidal deformability; neutron star; limit; upper limit ... See more keywords
Two-layer compact stars with crystalline quark matter: Screening effect on the tidal deformability
Sign Up to like & getrecommendations! Published in 2019 at "Physical Review D"
DOI: 10.1103/physrevd.99.023018
Abstract: (Abridged) It is well known that the tidal deformability of a compact star carries important information about the interior equation-of-state (EOS) of the star. The first gravitational-wave event GW170817 from a binary compact star merger… read more here.
Keywords: tidal deformability; quark matter; deformability; star ... See more keywords