Transport equations for nuclear fission and heavy-ion collisions: Exploiting locally harmonic approximations

1985 ◽  
Vol 87 (2) ◽  
pp. 189-200 ◽  
Author(s):  
H. Hofmann
1984 ◽  
Vol 45 (C6) ◽  
pp. C6-477-C6-488 ◽  
Author(s):  
R. K. Gupta ◽  
D. R. Saroha ◽  
N. Malhotra

2010 ◽  
Vol 19 (08n10) ◽  
pp. 1483-1490 ◽  
Author(s):  
T. STROTHER ◽  
W. BAUER

Motivated by the success of kinetic theory in the description of observables in intermediate and high energy heavy-ion collisions, we use kinetic theory to model the dynamics of core collapse supernovae. The specific way that we employ kinetic theory to solve the relevant transport equations allows us to explicitly model the propagation of neutrinos and a full ensemble of nuclei and treat neutrino–matter interactions in a very general way. With these abilities, our simulations have observed dynamics that may prove to be an entirely new neutrino capture induced supernova explosion mechanism.


2021 ◽  
Author(s):  
Xiaojun Yao ◽  
Weiyao Ke ◽  
Yingru Xu ◽  
Steffen A. Bass ◽  
Berndt Mueller

2019 ◽  
Author(s):  
Xiaojun Yao ◽  
Weiyao Ke ◽  
Yingru Xu ◽  
Steffen A. Bass ◽  
Berndt Muller

2019 ◽  
Vol 982 ◽  
pp. 755-758 ◽  
Author(s):  
Xiaojun Yao ◽  
Weiyao Ke ◽  
Yingru Xu ◽  
Steffen Bass ◽  
Berndt Müller

1984 ◽  
Vol 45 (C6) ◽  
pp. C6-269-C6-279
Author(s):  
A. Bonaccorso ◽  
M. Di Toro ◽  
U. Lombardo ◽  
G. Russo

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