Numerical simulations of stellar collapse in scalar-tensor theories of gravity

DOI10.1088/0264-9381/33/13/135002zbMath1346.83021arXiv1602.06952OpenAlexW3102479383MaRDI QIDQ3188376

Ulrich Sperhake, Davide Gerosa, Christian D. Ott

Publication date: 19 August 2016

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

Full work available at URL: https://arxiv.org/abs/1602.06952

zbMATH Keywords

gravitational wavessupernovaemodified theories of gravity

Mathematics Subject Classification ID

Space-time singularities, cosmic censorship, etc. (83C75) 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) Computational methods for problems pertaining to relativity and gravitational theory (83-08) Gravitational waves (83C35)

Related Items (3)

Orbiting naked singularities in large-\(\omega \) Brans-Dicke gravity ⋮ Inverse-chirp signals and spontaneous scalarisation with self-interacting potentials in stellar collapse ⋮ Scalar gravitational wave signals from core collapse in massive scalar–tensor gravity with triple-scalar interactions

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