Multimessengers from Core-Collapse Supernovae: Multidimensionality as a Key to Bridge Theory and Observation
Core-collapse supernovae are dramatic explosions marking the catastrophic end of massive stars. The only means to get direct information about the supernova engine is from observations of neutrinos emitted by the forming neutron star, and through gravitational waves which are produced when the hydro...
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Format: | Article |
Language: | English |
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Wiley
2012-01-01
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Series: | Advances in Astronomy |
Online Access: | http://dx.doi.org/10.1155/2012/428757 |
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author | Kei Kotake Tomoya Takiwaki Yudai Suwa Wakana Iwakami Nakano Shio Kawagoe Youhei Masada Shin-ichiro Fujimoto |
author_facet | Kei Kotake Tomoya Takiwaki Yudai Suwa Wakana Iwakami Nakano Shio Kawagoe Youhei Masada Shin-ichiro Fujimoto |
author_sort | Kei Kotake |
collection | DOAJ |
description | Core-collapse supernovae are dramatic explosions marking the catastrophic end of massive stars. The only means to get direct information about the supernova engine is from observations of neutrinos emitted by the forming neutron star, and through gravitational waves which are produced when the hydrodynamic flow or the neutrino flux is not perfectly spherically symmetric. The multidimensionality of the supernova engine, which breaks the sphericity of the central core such as convection, rotation, magnetic fields, and hydrodynamic instabilities of the supernova shock, is attracting great attention as the most important ingredient to understand the long-veiled explosion mechanism. Based on our recent work, we summarize properties of gravitational waves, neutrinos, and explosive nucleosynthesis obtained in a series of our multidimensional hydrodynamic simulations and discuss how the mystery of the central engines can be unraveled by deciphering these multimessengers produced under the thick veils of massive stars. |
format | Article |
id | doaj-art-dd0c4ef38c3e465faf46864a45a5d539 |
institution | Kabale University |
issn | 1687-7969 1687-7977 |
language | English |
publishDate | 2012-01-01 |
publisher | Wiley |
record_format | Article |
series | Advances in Astronomy |
spelling | doaj-art-dd0c4ef38c3e465faf46864a45a5d5392025-02-03T07:26:14ZengWileyAdvances in Astronomy1687-79691687-79772012-01-01201210.1155/2012/428757428757Multimessengers from Core-Collapse Supernovae: Multidimensionality as a Key to Bridge Theory and ObservationKei Kotake0Tomoya Takiwaki1Yudai Suwa2Wakana Iwakami Nakano3Shio Kawagoe4Youhei Masada5Shin-ichiro Fujimoto6Division of Theoretical Astronomy, National Astronomical Observatory of Japan, 2-21-1, Osawa, Mitaka, Tokyo 181-8588, JapanCenter for Computational Astrophysics, National Astronomical Observatory of Japan, Mitaka, Tokyo 181-8588, JapanYukawa Institute for Theoretical Physics, Kyoto University, Oiwake-cho, Kitashirakawa, Sakyo-ku, Kyoto 606-8502, JapanDepartment of Aerospace Engineering, Tohoku University, 6-6-01 Aramaki-Aza-Aoba, Aoba-ku, Sendai 980-8579, JapanKnowledge Dissemination Unit, Oshima Lab, Institute of Industrial Science, The University of Tokyo, 4-6-1 Komaba, Meguro-ku, Tokyo 153-8505, JapanDepartment of Computational Science, Graduate School of System Informatics, Kobe University, Nada, Kobe 657-8501, JapanKumamoto National College of Technology, 2659-2 Suya, Goshi, Kumamoto 861-1102, JapanCore-collapse supernovae are dramatic explosions marking the catastrophic end of massive stars. The only means to get direct information about the supernova engine is from observations of neutrinos emitted by the forming neutron star, and through gravitational waves which are produced when the hydrodynamic flow or the neutrino flux is not perfectly spherically symmetric. The multidimensionality of the supernova engine, which breaks the sphericity of the central core such as convection, rotation, magnetic fields, and hydrodynamic instabilities of the supernova shock, is attracting great attention as the most important ingredient to understand the long-veiled explosion mechanism. Based on our recent work, we summarize properties of gravitational waves, neutrinos, and explosive nucleosynthesis obtained in a series of our multidimensional hydrodynamic simulations and discuss how the mystery of the central engines can be unraveled by deciphering these multimessengers produced under the thick veils of massive stars.http://dx.doi.org/10.1155/2012/428757 |
spellingShingle | Kei Kotake Tomoya Takiwaki Yudai Suwa Wakana Iwakami Nakano Shio Kawagoe Youhei Masada Shin-ichiro Fujimoto Multimessengers from Core-Collapse Supernovae: Multidimensionality as a Key to Bridge Theory and Observation Advances in Astronomy |
title | Multimessengers from Core-Collapse Supernovae: Multidimensionality as a Key to Bridge Theory and Observation |
title_full | Multimessengers from Core-Collapse Supernovae: Multidimensionality as a Key to Bridge Theory and Observation |
title_fullStr | Multimessengers from Core-Collapse Supernovae: Multidimensionality as a Key to Bridge Theory and Observation |
title_full_unstemmed | Multimessengers from Core-Collapse Supernovae: Multidimensionality as a Key to Bridge Theory and Observation |
title_short | Multimessengers from Core-Collapse Supernovae: Multidimensionality as a Key to Bridge Theory and Observation |
title_sort | multimessengers from core collapse supernovae multidimensionality as a key to bridge theory and observation |
url | http://dx.doi.org/10.1155/2012/428757 |
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