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 language | English |
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Title of host publication | Proceedings of the 50th Rencontres de Moriond - 2015 Gravitation |
Subtitle of host publication | 100 years after GR |
Editors | Etienne Auge, Jacques Dumarchez, Jean Tran Thanh Van |
Publisher | The Gioi Publishers |
Pages | 375-376 |
Number of pages | 2 |
ISBN (Electronic) | 9782954640068 |
State | Published - 2015 |
Event | 50th Rencontres de Moriond on Gravitation 2015: 100 years after GR - La Thuile, Italy Duration: Mar 21 2015 → Mar 28 2015 |
Publication series
Name | Proceedings of the 50th Rencontres de Moriond - 2015 Gravitation: 100 years after GR |
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Conference
Conference | 50th Rencontres de Moriond on Gravitation 2015: 100 years after GR |
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Country/Territory | Italy |
City | La Thuile |
Period | 03/21/15 → 03/28/15 |
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.