Explosion mechanism, neutrino burst and gravitational wave in core-collapse supernovae
@article{Kotake2005ExplosionMN,
title={Explosion mechanism, neutrino burst and gravitational wave in core-collapse supernovae},
author={Kei Kotake and Katsuhiko Sato and Keitaro Takahashi},
journal={Reports on Progress in Physics},
year={2005},
volume={69},
pages={971-1143}
}Core-collapse supernovae are among the most energetic explosions in the universe marking the catastrophic end of massive stars. In spite of rigorous studies for several decades, we still do not understand the explosion mechanism completely. Since they are related to many astrophysical phenomena such as nucleosynthesis, gamma-ray bursts and acceleration of cosmic rays, understanding of their physics has been of wide interest to the astrophysical community.In this paper, we review recent progress…
Figures and Tables from this paper
figure 1 
table 1 
figure 2 
table 2 
figure 3 
table 3 
figure 4 
table 4 
figure 5 
table 5 
figure 6 
table 6 
figure 7 
table 7 
figure 8 
table 8 
figure 9 
table 9 
table 10 
figure 11 
figure 12 
figure 13 
figure 14 
figure 15 
figure 16 
figure 19 
figure 21 
figure 23 
figure 24 
figure 25 
figure 26 
figure 27 
figure 28 
figure 29 
figure 30 
figure 31 
figure 32 
figure 33 
figure 34 
figure 35 
figure 36 
figure 37 
figure 38 
figure 40 
figure 42 
figure 43 
figure 44 
figure 45 
figure 46 
figure 47 
figure 48 
figure 50 
figure 51 
figure 52 
figure 54 
figure 55 
figure 56 
figure 57 
figure 58 
figure 59 
figure 60 
figure 61 
figure 62 
figure 63 
figure 64 
figure 65 
figure 66 
figure 68 
figure 69 
figure 70 
figure 71 
figure 72 
figure 73 
figure 74 
figure 75 
figure 76 
figure 77 
figure 78 
figure 79 
figure 80 
figure 81 
figure 82 
figure 83 
figure 84 
figure 85 
figure 86 
figure 87 
figure 88 
figure 89 
figure 90 
figure 91 
figure 92 
figure 93 
figure 94 
figure 95 
figure 96 
figure 97 
figure 98 
figure 99 
figure 100 
figure 101 
figure 102 
figure 103 
figure 104 
figure 105 
figure 106 
figure 107 
figure 108 
figure 109 
figure 110 
figure 111 
figure 112 
figure 113 
figure 114 
figure 115 
figure 116 
figure 117 
figure 118 
figure 119 
figure 120 
figure 121 
figure 122 
figure 123 
figure 124 
figure 125 
figure 126 
figure 127 
figure 128 
figure 129 
figure 130 
figure 131 
figure 132 
figure 133 
figure 134 
figure 135 
figure 136 
figure 137 
figure 138 
figure 139
216 Citations
A numerical challenge on the core-collapse supernovae: physics of neutrino and matter at extreme conditions
- Physics
- 2011
Core-collapse supernovae are the explosive phenomena, which occur at the end of the life of massive stars. Despite the importance of these astrophysical events, the mechanism of supernova explosion…
Gravitational waves from 3D MHD core-collapse supernova simulations with neutrino transport
- Physics
- 2011
Core-collapse supernovae (CCSNe) are among the most energetic explosions in the universe, liberating the prodigious amount of ~ 1053 erg, the binding energy of their compact remnants, neutron stars…
Towards gravitational-wave astronomy of core-collapse supernova explosion
- Physics
- 2010
We study properties of gravitational waves based on the three-dimensional (3D) simulations, which demonstrate the neutrino-driven explosions aided by the standing accretion shock instability (SASI).…
Explosion Mechanisms of Core-Collapse Supernovae
- Physics
- 2012
Supernova theory, numerical and analytic, has made remarkable progress in the past decade. This progress was made possible by more sophisticated simulation tools, especially for neutrino transport,…
Neutrino oscillations in magnetically driven supernova explosions
- Physics
- 2009
We investigate neutrino oscillations from core-collapse supernovae that produce magnetohydrodynamic (MHD) explosions. By calculating numerically the flavor conversion of neutrinos in the highly…
Gravitational waves from core-collapse supernovae and their related compact objects
- Physics
- 2008
Core-collapse supernovae have been supposed to be one of the most plausible sources of gravitational waves. Based on a series of our magnetohydrodynamic core-collapse simulations, we find that the…
Gravitational-wave signatures in successful vs. failed core-collapse supernovae
- Physics
- 2011
In this contribution, we discuss possible gravitational-wave (GWs) signatures emitted from core-collapse supernovae that do or do not produce explosions. For the former case, we study properties of…
STOCHASTIC NATURE OF GRAVITATIONAL WAVES FROM SUPERNOVA EXPLOSIONS WITH STANDING ACCRETION SHOCK INSTABILITY
- Physics
- 2009
We study the properties of gravitational waves (GWs) based on three-dimensional (3D) simulations, which demonstrate neutrino-driven explosions aided by standing accretion shock instability (SASI).…
Anisotropic neutrinos and gravitational waves from black hole neutrino-dominated accretion flows in fallback core-collapse supernovae
- Physics
- 2021
Fallback in core-collapse supernovae (CCSNe) plays an important role in determining the properties of the central compact remnants, which might produce a black hole (BH) hyperaccretion system in the…
References
SHOWING 1-10 OF 452 REFERENCES
Explosion Mechanisms of Massive Stars
- Physics
- 2002
One of the central problems in supernova theory is the question how massive stars explode. Understanding the physical processes that drive the explosion is crucial for linking the stellar progenitors…
Gravitational radiation from supernova neutrino bursts
- PhysicsNature
- 1978
SUPERNOVAE, the violent collapses of massive stars into neutron stars, are considered to be the strongest known sources of gravitational radiation. The quadrupole (and higher) moments of the…
Effect of Anisotropic Neutrino Radiation on Supernova Explosion Energy
- Physics
- 2001
Since SN 1987A, many observations have indicated that supernova explosions are not spherical. The cause of the asymmetric explosion is still controversial (e.g., asymmetry in the envelope, the…
On the nature of core-collapse supernova explosions
- Physics
- 1995
We investigate in this paper the core-collapse supernova explosion mechanism in both one and two dimensions. We verify the usefulness of neutrino-driven overturn (``convection'') between the shock…
Conditions for shock revival by neutrino heating in core-collapse supernovae
- Physics
- 2001
Energy deposition by neutrinos can rejuvenate the stalled bounce shock and can provide the energy for the supernova explosion of a massive star. This neutrino-heating mechanism, though investigated…
Asymmetric Supernova Explosions
- Physics
- 2004
Core collapse supernovae (SN) are the final stages of stellar evolution in massive stars during which the central region collapses, forms a neutron star (NS) or black hole, and the outer layers are…
The Physics of Supernova Explosions
- Physics
- 1986
The modern study of supernovae involves many aspects: presupernova stellar evolution, the physics of the explosions themselves, observations at all wavelengths of the outbursts and their remnants,…
Gravitational Waves from Stellar Collapse: Correlations to Explosion Asymmetries
- Physics
- 2004
The collapse of massive stars produces not only observable outbursts across the entire electromagnetic spectrum but, for Galactic (or near-Galactic) supernovae, detectable signals for ground-based…
Radiation Hydrodynamics with Neutrinos: Stellar Core Collapse and the Explosion Mechanism of Type II Supernovae
- Physics
- 2000
According to the current standard picture supernova explosions of evolved massive stars are mediated by the deposition of neutrino energy in the stellar medium. Detailed numerical simulations,…
Supernova neutrinos, neutrino oscillations, and the mass of the progenitor star
- Physics
- 2003
We investigate the initial progenitor mass dependence of the early-phase neutrino signal from supernovae taking neutrino oscillations into account. The early-phase analysis has advantages in that it…