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The Gravitational Wave Signal of a Core Collapse Supernova Explosion of a 15M$_\odot$ Star

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arxiv 1701.07325 v1 pith:PXO7TXA7 submitted 2017-01-25 astro-ph.HE

Konstantin N. Yakunin , Anthony Mezzacappa , Pedro Marronetti , Eric J. Lentz , Stephen W. Bruenn , W. Raphael Hix , O. E. Bronson Messer , Eirik Endeve
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John M. Blondin J. Austin Harris
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keywords gravitationalsignalwavecollapsecoreexplosionodotsimulation
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abstract

In this Letter, we report on the gravitational wave signal computed in the context of an $ab$ $initio$, three-dimensional simulation of a core collapse supernova explosion, beginning with a 15M$_\odot$ star and using state-of-the-art weak interactions. The simulation was performed with our neutrino hydrodynamics code Chimera. We discuss the potential for detection of our predicted gravitational signal by the current generation of gravitational wave detectors.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Phenomenological gravitational waveforms for core-collapse supernovae

    astro-ph.HE 2025-01 conditional novelty 5.0 of 10

    ccphen v4 quickly generates stochastic, polarized gravitational waveforms for non-rotating core-collapse supernovae, calibrated to 33 numerical simulations.

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