Dynamical tidal response of neutron stars as a probe of dense-matter properties
Abhishek Hegade K. R., Yumu Yang, Mauricio Hippert, Jacquelyn Noronha-Hostler, Jorge Noronha, Nicolás Yunes
gr-qc, astro-ph.HE, nucl-th
Submitted: 2026-08-17
Updated: 2026-08-18
Comments: 18 pages + appendices, 9 figures. Supplementary notebook in the source file
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Tidal deformability of neutron stars with realistic equations of state and their gravitational wave signatures in binary inspiral
- Hybrid stars in the light of GW170817
- Nonparametric Inference of Neutron Star Composition, Equation of State, and Maximum Mass with GW170817
- Extreme Matter meets Extreme Gravity: Ultra-heavy neutron stars with crossovers and first-order phase transitions
- Neutron star tidal deformability and equation of state constraints
- The slope, the hill, the drop, and the swoosh: Learning about the nuclear matter equation of state from the binary Love relations
- Nonparametric extensions of nuclear equations of state: probing the breakdown scale of relativistic mean-field theory
- Constraining neutron star tidal Love numbers with gravitational wave detectors
- GW170817: Measurements of Neutron Star Radii and Equation of State
- Tidal Love numbers of neutron stars
- Relativistic theory of tidal Love numbers
- Relativistic tidal properties of neutron stars
- Properties of the binary neutron star merger GW170817
- Dynamical Tides in General Relativity: Effective Action and Effective-One-Body Hamiltonian
- Resonant Oscillations and Tidal Heating in Coalescing Binary Neutron Stars
- Neutron-star seismology with realistic, finite-temperature nuclear matter
- Interface modes in inspiralling neutron stars: A gravitational-wave probe of first-order phase transitions
- Probing internal dissipative processes of neutron stars with gravitational waves during the inspiral of neutron star binaries
- Gravitational radiation from a particle in circular orbit around a black hole. V. Black-hole absorption and tail corrections
- Post-Newtonian Expansion of Gravitational Waves from a Particle in Circular Orbits around a Rotating Black Hole :Effects of Black Hole Absorption
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