On the ambiguity in relativistic tidal deformability

DOI10.1088/1361-6382/aab186zbMath1409.83044arXiv1710.11096OpenAlexW2767087979WikidataQ130202843 ScholiaQ130202843MaRDI QIDQ3119746

Samuel E. Gralla

Publication date: 12 March 2019

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1710.11096

zbMATH Keywords

black holesgravitational wavesneutron starstidal deformability

Mathematics Subject Classification ID

Black holes (83C57) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15) Gravitational waves (83C35)

Related Items (5)

Scalar Love numbers and Love symmetries of 5-dimensional Myers-Perry black holes ⋮ On the vanishing of Love numbers for Kerr black holes ⋮ Interpreting binary neutron star mergers: describing the binary neutron star dynamics, modelling gravitational waveforms, and analyzing detections ⋮ Ladder symmetries of black holes. Implications for love numbers and no-hair theorems ⋮ Static response and Love numbers of Schwarzschild black holes

Cites Work

• Multipole moments for stationary systems: The equivalence of the Geroch- Hansen formulation and the Thorne formulation
• Proof of a multiple conjecture due to Geroch
• Black hole stereotyping: induced gravito-static polarization
• The tune of love and thenature(ness)of spacetime
• Multipole Moments. II. Curved Space
• Multipole moments of stationary space-times
• Perspective on gravitational self-force analyses
• A rigorous derivation of gravitational self-force

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