scholarly journals Gravitational Waves from Axisymmetric, Rotating Stellar Core Collapse

2004 ◽  
Vol 600 (2) ◽  
pp. 834-864 ◽  
Author(s):  
Christian D. Ott ◽  
Adam Burrows ◽  
Eli Livne ◽  
Rolf Walder
2008 ◽  
Vol 120 (3) ◽  
pp. 032013
Author(s):  
R Honda ◽  
N Kanda ◽  
T Akutsu ◽  
M Ando ◽  
Y Tsunesada ◽  
...  

2011 ◽  
Vol 83 (6) ◽  
Author(s):  
C. Reisswig ◽  
C. D. Ott ◽  
U. Sperhake ◽  
E. Schnetter

2016 ◽  
pp. 906-914
Author(s):  
G.S. Bisnovatyi-Kogan ◽  
S.G. Moiseenko

2011 ◽  
Vol 7 (S279) ◽  
pp. 367-368
Author(s):  
Ken'ichiro Nakazato ◽  
Kohsuke Sumiyoshi

AbstractSome supernovae and gamma-ray bursts are thought to accompany a black hole formation. In the process of a black hole formation, a central core becomes hot and dense enough for hyperons and quarks to appear. In this study, we perform neutrino-radiation hydrodynamical simulations of a stellar core collapse and black hole formation taking into account such exotic components. In our computation, general relativity is fully considered under spherical symmetry. As a result, we find that the additional degrees of freedom soften the equation of state of matter and promote the black hole formation. Furthermore, their effects are detectable as a neutrino signal. We believe that the properties of hot and dense matter at extreme conditions are essential for the studies on the astrophysical black hole formation. This study will be hopefully a first step toward a physics of the central engine of gamma-ray bursts.


1994 ◽  
Vol 35 ◽  
pp. 270-272 ◽  
Author(s):  
E.N. Alexeyev ◽  
L.N. Alexeyeva ◽  
A.E. Chudakov ◽  
G.D. Korotkii ◽  
N.A. Metlinskii ◽  
...  

2015 ◽  
Vol 811 (2) ◽  
pp. 86 ◽  
Author(s):  
Takaaki Yokozawa ◽  
Mitsuhiro Asano ◽  
Tsubasa Kayano ◽  
Yudai Suwa ◽  
Nobuyuki Kanda ◽  
...  

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