The electron capture of nuclides 55Co and 56Ni in the process of stellar core collapse

2012 ◽  
Vol 343 (1) ◽  
pp. 117-122 ◽  
Author(s):  
Jing-Jing Liu
2010 ◽  
Vol 848 (3-4) ◽  
pp. 454-478 ◽  
Author(s):  
A. Juodagalvis ◽  
K. Langanke ◽  
W.R. Hix ◽  
G. Martínez-Pinedo ◽  
J.M. Sampaio

2003 ◽  
Vol 90 (24) ◽  
Author(s):  
K. Langanke ◽  
G. Martínez-Pinedo ◽  
J. M. Sampaio ◽  
D. J. Dean ◽  
W. R. Hix ◽  
...  

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

2005 ◽  
Vol 758 ◽  
pp. 31-34 ◽  
Author(s):  
W.R. Hix ◽  
O.E.B. Messer ◽  
A. Mezzacappa ◽  
J. Sampaio ◽  
K. Langanke ◽  
...  

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 ◽  
...  

1981 ◽  
Vol 249 ◽  
pp. 270 ◽  
Author(s):  
K. A. van Riper ◽  
J. M. Lattimer
Keyword(s):  

2020 ◽  
Vol 7 (7) ◽  
pp. 200467
Author(s):  
Morgan Fraser

It is 30 years since the characteristic signatures of interaction with circumstellar material (CSM) were first observed in a core-collapse supernova. Since then, CSM interaction has been observed and inferred across a range of transients, from the low-energy explosions of low-mass stars as likely electron-capture supernovae, through to the brightest superluminous supernovae. In this review, I present a brief overview of some of the interacting supernovae and transients that have been observed to date, and attempt to classify and group them together in a phenomenological framework.


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