Neutron-star tidal deformability and equation-of-state constraints

DOI10.1007/S10714-020-02754-3zbMath1465.83015arXiv2006.03168OpenAlexW3104504237MaRDI QIDQ828792

Katerina Chatziioannou

Publication date: 5 May 2021

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2006.03168

zbMATH Keywords

coalescencebinary neutron starstidal deformation

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15) Equations of motion in general relativity and gravitational theory (83C10) Gravitational waves (83C35)

Related Items (9)

Astrophysical constraints on compact objects in 4D Einstein-Gauss-Bonnet gravity ⋮ Approximate perfect fluid solutions with quadrupole moment ⋮ Thermal effects on tidal deformability in the last orbits of an inspiraling binary neutron star system ⋮ Gravitational waves from binary neutron stars ⋮ Scalar Love numbers and Love symmetries of 5-dimensional Myers-Perry black holes ⋮ Love symmetry ⋮ Gravitoelectric dynamical tides at second post-Newtonian order ⋮ Anisotropic compact stars: constraining model parameters to account for physical features of tidal love numbers ⋮ Leading nonlinear tidal effects and scattering amplitudes

Cites Work

• Holographic compact stars meet gravitational wave constraints
• Approximate universal relations for neutron stars and quark stars
• Gravity
• Gravitational Radiation from Point Masses in a Keplerian Orbit
• Gravitational radiation from post-Newtonian sources and inspiralling compact binaries

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