Gravitational wave signals from multi-dimensional core-collapse supernova explosion simulations

In this work we report briefly on the gravitational wave (GW) signal computed in the context of a self-consistent, 3D simulation of a core-collapse supernova (CCSN) explosion of a 15M\(_\odot\) progenitor star. We present a short overview of the GW signal, including signal amplitude, frequency distr...

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Bibliographic Details
Published in:arXiv.org 2017-10
Main Authors: Yakunin, K N, Endeve, E, Mezzacappa, A, Szczpanczyk, M, Zanolin, M, Marronetti, P, Lentz, E J, Bruenn, S W, Hix, W R, Messer, O E B, Blondin, J M, Harris, J A
Format: Article
Language:English
Subjects:
Computer simulation
Energy distribution
Explosions
Frequency distribution
Gravitation
Gravitational collapse
Gravitational waves
Neutrinos
Online Access:Get full text
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Summary:In this work we report briefly on the gravitational wave (GW) signal computed in the context of a self-consistent, 3D simulation of a core-collapse supernova (CCSN) explosion of a 15M\(_\odot\) progenitor star. We present a short overview of the GW signal, including signal amplitude, frequency distribution, and the energy emitted in the form of GWs for each phase of explosion, along with neutrino luminosities, and discuss correlations between them.
ISSN:2331-8422