Multiple physical elements to determine the gravitational-wave signatures of core-collapse supernovae

被引:77
|
作者
Kotake, Kei [1 ,2 ]
机构
[1] Natl Inst Nat Sci, Natl Astron Observ Japan, Div Theoret Astron, Mitaka, Tokyo 1818588, Japan
[2] Natl Inst Nat Sci, Natl Astron Observ Japan, Ctr Computat Astrophys, Mitaka, Tokyo 1818588, Japan
关键词
Supernovae; Radiation-hydrodynamics; Gravitational wave physics; Neutrino physics; ACCRETION SHOCK INSTABILITY; GAMMA-RAY BURSTS; EQUATION-OF-STATE; ANISOTROPIC NEUTRINO RADIATION; ARMED SPIRAL INSTABILITY; FULL GENERAL-RELATIVITY; ROTATING MASSIVE STARS; CIRCLE-DOT STAR; DRIVEN SUPERNOVA; DYNAMICAL INSTABILITIES;
D O I
10.1016/j.crhy.2013.01.008
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We review recent progress in the theoretical predictions of gravitational waves (GWs) of core-collapse supernovae. Following a brief summary of the methods in the numerical modeling, we summarize multiple physical elements that determine the GW signatures which have been considered to be important in extracting the information of the long-veiled explosion mechanism from the observation of the GWs. We conclude with a summary of the most urgent tasks to make the dream come true. (C) 2013 Academie des sciences. Published by Elsevier Masson SAS. All rights reserved.
引用
收藏
页码:318 / 351
页数:34
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