Gravitational Waves from Core-Collapse Supernovae

Bernhard Müller

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arXiv · 1703.04633

Gravitational Waves from Core-Collapse Supernovae

Bernhard Müller

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Abstract

Gravitational waves are a potential direct probe for the multi-dimensional flow during the first second of core-collapse supernova explosions. Here we outline the structure of the predicted gravitational wave signal from neutrino-driven supernovae of non-rotating progenitors from recent 2D and 3D simulations. We sketch some quantitative dependencies that govern the amplitudes of this signal and its evolution in the time-frequency domain.

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Bernhard Müller. 2017-03-14. Gravitational Waves from Core-Collapse Supernovae. https://arxiv.org/abs/1703.04633

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