Tensor-multi-scalar theories: relativistic stars and 3 + 1 decomposition

DOI10.1088/0264-9381/32/20/204001zbMath1327.83027arXiv1505.07462OpenAlexW1913183818WikidataQ59942238 ScholiaQ59942238MaRDI QIDQ3453152

Paolo Pani, Leonardo Gualtieri, Emanuele Berti, Ulrich Sperhake, Hector O. Silva, Michael Horbatsch, Davide Gerosa

Publication date: 20 November 2015

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

Full work available at URL: https://arxiv.org/abs/1505.07462

zbMATH Keywords

gravityblack holesneutron starsmodified theories

Mathematics Subject Classification ID

Geometrodynamics and the holographic principle (83E05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Galactic and stellar structure (85A15) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (8)

Stellar structure models in modified theories of gravity: lessons and challenges ⋮ Static neutron stars perspective of quadratic and induced inflationary attractor scalar-tensor theories ⋮ Neutron stars in scalar-tensor gravity with quartic order scalar potential ⋮ Extreme gravity tests with gravitational waves from compact binary coalescences. I: Inspiral-merger ⋮ Dynamics of test particles around hairy black holes in Horndeski's theory ⋮ Inverse-chirp signals and spontaneous scalarisation with self-interacting potentials in stellar collapse ⋮ Universal inflationary attractors implications on static neutron stars ⋮ Invariant quantities in the multiscalar-tensor theories of gravitation

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