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

K. N. Yakunin; E. Endeve; A. Mezzacappa; M. Szczpanczyk; M. Zanolin; P. Marronetti; E. J. Lentz; S. W. Bruenn; W. R. Hix; O. E.B. Messer; J. M. Blondin; J. A. Harris

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

K. N. Yakunin, E. Endeve, A. Mezzacappa, M. Szczpanczyk, M. Zanolin, P. Marronetti, E. J. Lentz, S. W. Bruenn, W. R. Hix, O. E.B. Messer, J. M. Blondin, J. A. Harris

Research output: Contribution to conference › Paper › peer-review

Abstract

In this work we report briefly on the gravitational wave (GW) signal computed in the context of a self-consistent, three-dimensional (3D) simulation of a core-collapse supernova (CCSN) explosion of a 15 M☉ 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.

Original language	English
Pages	37-41
Number of pages	5
State	Published - 2017
Event	52nd Rencontres de Moriond on Gravitation 2017 - La Thuile, Italy Duration: Mar 25 2017 → Apr 1 2017

Conference

Conference	52nd Rencontres de Moriond on Gravitation 2017
Country/Territory	Italy
City	La Thuile
Period	03/25/17 → 04/1/17

Funding

This research was supported by the U.S. Department of Energy Offices of Nuclear Physics and Advanced Scientific Computing Research, the NASA Astrophysics Theory and Fundamental Physics Program (grants NNH08AH71I and NNH11AQ72I), and the National Science Foundation PetaApps Program (grants OCI-0749242, OCI-0749204, and OCI-0749248) and Gravitational Physics Program (grant GP-1505933).

Cite this

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. (2017). Gravitational wave signals from multi-dimensional core-collapse supernova explosion simulations. 37-41. Paper presented at 52nd Rencontres de Moriond on Gravitation 2017, La Thuile, Italy.

@conference{19cb9a6ac96547b5b588312c09e0d8be,

title = "Gravitational wave signals from multi-dimensional core-collapse supernova explosion simulations",

abstract = "In this work we report briefly on the gravitational wave (GW) signal computed in the context of a self-consistent, three-dimensional (3D) simulation of a core-collapse supernova (CCSN) explosion of a 15 M☉ 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.",

author = "Yakunin, {K. N.} and E. Endeve and A. Mezzacappa and M. Szczpanczyk and M. Zanolin and P. Marronetti and Lentz, {E. J.} and Bruenn, {S. W.} and Hix, {W. R.} and Messer, {O. E.B.} and Blondin, {J. M.} and Harris, {J. A.}",

note = "Publisher Copyright: {\textcopyright} Proceedings of the 52nd Rencontres de Moriond - 2017 Gravitation.; 52nd Rencontres de Moriond on Gravitation 2017 ; Conference date: 25-03-2017 Through 01-04-2017",

year = "2017",

language = "English",

pages = "37--41",

}

Yakunin, KN, Endeve, E, Mezzacappa, A, Szczpanczyk, M, Zanolin, M, Marronetti, P, Lentz, EJ, Bruenn, SW, Hix, WR , Messer, OEB, Blondin, JM & Harris, JA 2017, 'Gravitational wave signals from multi-dimensional core-collapse supernova explosion simulations', Paper presented at 52nd Rencontres de Moriond on Gravitation 2017, La Thuile, Italy, 03/25/17 - 04/1/17 pp. 37-41.

TY - CONF

T1 - Gravitational wave signals from multi-dimensional core-collapse supernova explosion simulations

AU - Yakunin, K. N.

AU - Endeve, E.

AU - Mezzacappa, A.

AU - Szczpanczyk, M.

AU - Zanolin, M.

AU - Marronetti, P.

AU - Lentz, E. J.

AU - Bruenn, S. W.

AU - Hix, W. R.

AU - Messer, O. E.B.

AU - Blondin, J. M.

AU - Harris, J. A.

PY - 2017

Y1 - 2017

N2 - In this work we report briefly on the gravitational wave (GW) signal computed in the context of a self-consistent, three-dimensional (3D) simulation of a core-collapse supernova (CCSN) explosion of a 15 M☉ 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.

AB - In this work we report briefly on the gravitational wave (GW) signal computed in the context of a self-consistent, three-dimensional (3D) simulation of a core-collapse supernova (CCSN) explosion of a 15 M☉ 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.

UR - http://www.scopus.com/inward/record.url?scp=85091327228&partnerID=8YFLogxK

M3 - Paper

AN - SCOPUS:85091327228

SP - 37

EP - 41

T2 - 52nd Rencontres de Moriond on Gravitation 2017

Y2 - 25 March 2017 through 1 April 2017

ER -

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

Abstract

Conference

Funding

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