Tidal deformability of neutron and hyperon star with relativistic mean field equations of state
arXiv:1609.08863 · doi:10.1103/PhysRevC.95.015801
Abstract
We systematically study the tidal deformability for neutron and hyperon stars using relativistic mean field (RMF) equations of state (EOSs). The tidal effect plays an important role during the early part of the evolution of compact binaries. Although, the deformability associated with the EOSs has a small correction, it gives a clean gravitational wave signature in binary inspiral. These are characterized by various love numbers kl (l=2, 3, 4), that depend on the EOS of a star for a given mass and radius. The tidal effect of star could be efficiently measured through advanced LIGO detector from the final stages of inspiraling binary neutron star (BNS) merger.
References in corpus (16)
- Shapiro delay measurement of a two solar mass neutron star
- A Massive Pulsar in a Compact Relativistic Binary
- Chiral effective field theory and nuclear forces
- Tidal Love numbers of neutron stars
- Constraining neutron star tidal Love numbers with gravitational wave detectors
- Relativistic theory of tidal Love numbers
- Neutron-Rich Nuclei in Heaven and Earth
- Post-1-Newtonian tidal effects in the gravitational waveform from binary inspirals
- Building relativistic mean field models for finite nuclei and neutron stars
- Using Neutron Star Observations to Determine Crust Thicknesses, Moments of Inertia, and Tidal Deformabilities
- Constraining the High-Density Behavior of Nuclear Symmetry Energy with the Tidal Polarizability of Neutron Stars
- Analytic modelling of tidal effects in the relativistic inspiral of binary neutron stars
- Relativistic theory of surficial Love numbers
- Phase transition and properties of compact star
- Quark-Pauli effects in three octet-baryons
- Ground states and excited states of hypernuclei in Relativistic Mean Field approach
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- Constraints on Nuclear Saturation Properties from Terrestrial Experiments and Astrophysical Observations of Neutron Stars
- Compact star merger events with stars composed of interacting strange quark matter
- Role of dense matter in tidal deformations of inspiralling neutron stars and in gravitational waveform with unified equations of state
- Effect of Scalar Boson on Fermionic Dark Star
- Constraining the parameterized neutron star equation of state with astronomical observations
- Systematic study for the surface properties of neutron star