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I -Love- Q relations: from compact stars to black holes

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Publication:2814635
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DOI10.1088/0264-9381/33/9/095005zbMath1338.83163arXiv1601.02171OpenAlexW3102855289MaRDI QIDQ2814635

Kent Yagi, Nicolás Yunes

Publication date: 22 June 2016

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

Full work available at URL: https://arxiv.org/abs/1601.02171


zbMATH Keywords

relativityblack holesneutron starsmodified theories of gravity


Mathematics Subject Classification ID

Black holes (83C57) Strong interaction, including quantum chromodynamics (81V05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Galactic and stellar structure (85A15)


Related Items (7)

Approximate universal relations for neutron stars and quark stars ⋮ Slowly rotating Tolman VII solution ⋮ Flavored anisotropic black holes ⋮ Gravitoelectric dynamical tides at second post-Newtonian order ⋮ Extreme gravity tests with gravitational waves from compact binary coalescences: II: Ringdown ⋮ Interpreting binary neutron star mergers: describing the binary neutron star dynamics, modelling gravitational waveforms, and analyzing detections ⋮ Holographic spontaneous anisotropy







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