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

K.N. Yakunin
(
- Tennessee U.
)
,
E. Endeve
(
- Tennessee U. and
- Oak Ridge
)
,
A. Mezzacappa
(
- Tennessee U. and
- Oak Ridge
)
,
M. Szczpanczyk
(
- Embry-Riddle Aeronautical U.
)
,
M. Zanolin
(
- Embry-Riddle Aeronautical U.
)

Oct 23, 2017

5 pages

Part of Proceedings, 52nd Rencontres de Moriond on Gravitation (Moriond Gravitation 2017) : La Thuile, Italy, March 25-April 1, 2017, 37-42

Contribution to:

- Moriond Gravitation 2017
, 37-42

e-Print:

1710.08372 [astro-ph.HE]

View in:

ADS Abstract Service

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Abstract: (arXiv)

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.

Note:

5 pages, 2 figures, submitted in the proceedings of the 52nd Rencontres de Moriond

neutrino: luminosity
energy: emission
gravitational radiation
gravitational radiation detector
gravitational radiation: emission
supernova
higher-dimensional
correlation
star: collapse
numerical methods

References(14)

Figures(5)

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(
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)
,
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(
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- Oak Ridge
)
,
Pedro Marronetti
(
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)
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