Multiple physical elements to determine the gravitational-wave signatures of core-collapse supernovae

Abstract

We review recent progress in the theoretical predictions of gravitational waves (GWs) of core-collapse supernovae. Following a brief summary of the methods in the numerical modeling, we summarize multiple physical elements that determine the GW signatures which have been considered to be important in extracting the information of the long-veiled explosion mechanism from the observation of the GWs. We conclude with a summary of the most urgent tasks to make the dream come true.

48 pages, 16 figures, to appear in a special issue of Comptes Rendus Physique "Gravitational Waves (from detectors to astrophysics)"

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Cited by in corpus (78)

• Three-dimensional Hydrodynamic Core-Collapse Supernova Simulations for an $11.2M_{\odot }$ Star with Spectral Neutrino Transport
• Characterizing the Gravitational Wave Signal from Core-Collapse Supernovae
• Hydrodynamics of core-collapse supernovae and their progenitors
• General-Relativistic Simulations of Three-Dimensional Core-Collapse Supernovae
• The gravitational wave signal from core-collapse supernovae
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• Observing Gravitational Waves from Core-Collapse Supernovae in the Advanced Detector Era
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• Equation of State Effects on Gravitational Waves from Rotating Core Collapse
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