Multimessengers from 3D core-collapse supernovae

K. N. Yakunin, P. Marronetti, A. Mezzacappa, O. E.B. Messer, E. Lentz, S. Bruenn, W. Raphael Hix, J. A. Harris

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

Abstract

We present gravitational wave and neutrino signatures obtained in our ab initio 3D core-collapse supernova simulation of a 15 M☉ non-rotating progenitor with the Chimera code. Observations of neutrinos emitted by the forming neutron star and the gravitational waves produced by hydrodynamic instabilities are the most promising channel of direct information about the supernova engine. Both signals show different phases of the supernova evolution.

Original languageEnglish
Title of host publicationProceedings of the 50th Rencontres de Moriond - 2015 Gravitation
Subtitle of host publication100 years after GR
EditorsEtienne Auge, Jacques Dumarchez, Jean Tran Thanh Van
PublisherThe Gioi Publishers
Pages375-376
Number of pages2
ISBN (Electronic)9782954640068
StatePublished - 2015
Event50th Rencontres de Moriond on Gravitation 2015: 100 years after GR - La Thuile, Italy
Duration: Mar 21 2015Mar 28 2015

Publication series

NameProceedings of the 50th Rencontres de Moriond - 2015 Gravitation: 100 years after GR

Conference

Conference50th Rencontres de Moriond on Gravitation 2015: 100 years after GR
Country/TerritoryItaly
CityLa Thuile
Period03/21/1503/28/15

Funding

This research was supported by the U.S. Department of Energy Offices of Nuclear Physics and Advanced Scientific Computing Research and the NASA Astrophysics Theory and Fundamental Physics Program (NNH11AQ72I). PM is supported by the National Science Foundation through its employee IR/D program. The opinions and conclusions expressed herein are those of the authors and do not represent the National Science Foundation.

FundersFunder number
Nuclear Physics and Advanced Scientific Computing Research
National Science Foundation
National Aeronautics and Space AdministrationNNH11AQ72I

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