Inverse-chirp signals and spontaneous scalarisation with self-interacting potentials in stellar collapse

DOI10.1088/1361-6382/AB256FzbMath1477.83022arXiv1903.09704OpenAlexW3098407840WikidataQ121434735 ScholiaQ121434735MaRDI QIDQ5159872

Roxana Rosca-Mead, Christopher J. Moore, Ulrich Sperhake, Michalis Agathos

Publication date: 28 October 2021

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

Full work available at URL: https://arxiv.org/abs/1903.09704

zbMATH Keywords

gravitational wavesmodified gravitynumerical relativitystellar collapse

Mathematics Subject Classification ID

Black holes (83C57) Lattice gravity, Regge calculus and other discrete methods in general relativity and gravitational theory (83C27) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Galactic and stellar structure (85A15) Gravitational waves (83C35) Radiative transfer in astronomy and astrophysics (85A25)

Related Items (1)

Scalar gravitational wave signals from core collapse in massive scalar–tensor gravity with triple-scalar interactions

Uses Software

• GR1D

Cites Work

• Probes and tests of strong-field gravity with observations in the electromagnetic spectrum
• Numerical simulations of stellar collapse in scalar-tensor theories of gravity
• Towards the nonlinear regime in extensions to GR: assessing possible options
• Tensor-multi-scalar theories: relativistic stars and 3 + 1 decomposition
• A new open-source code for spherically symmetric stellar collapse to neutron stars and black holes
• The Scalar-Tensor Theory of Gravitation
• Tensor-multi-scalar theories of gravitation
• The Cauchy problem of scalar–tensor theories of gravity
• The motion of point particles in curved spacetime
• The confrontation between general relativity and experiment

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