Neutrino-pair bremsstrahlung in dense stars. I - Liquid metal case

1983 ◽  
Vol 275 ◽  
pp. 858 ◽  
Author(s):  
N. Itoh ◽  
Y. Kohyama
1993 ◽  
Vol 404 ◽  
pp. 418 ◽  
Author(s):  
Naoki Itoh ◽  
Yasuharu Kohyama ◽  
Noriyoshi Matsumoto ◽  
Midori Seki

1984 ◽  
Vol 105 ◽  
pp. 355-356
Author(s):  
Naoki Itoh ◽  
Yasuharu Kohyama

Neutrino-pair bremsstrahlung rate is calculated in the framework of the Weinberg-Salam theory for the dense matter relevant to the interior of white dwarfs and neutron stars. Ionic correlations both in the liquid state and in the bcc lattice state have been taken into account accurately. It is found that the ionic correlation in the liquid state reduces the neutrino-pair bremsstrahlung rate typically by a factor 2–20 depending on the element and temperature. It is also found that accurate inclusion of the Debye-Waller factor reduces the neutrino-pair bremsstrahlung rate in the lattice state typically by a factor 2.


1984 ◽  
Vol 285 ◽  
pp. 304 ◽  
Author(s):  
N. Itoh ◽  
Y. Kohyama ◽  
N. Matsumoto ◽  
M. Seki

1987 ◽  
Vol 316 ◽  
pp. 708 ◽  
Author(s):  
Hiroharu Munakata ◽  
Yasuharu Kohyama ◽  
Naoki Itoh
Keyword(s):  

1984 ◽  
Vol 279 ◽  
pp. 413 ◽  
Author(s):  
N. Itoh ◽  
N. Matsumoto ◽  
M. Seki ◽  
Y. Kohyama

1987 ◽  
Vol 322 ◽  
pp. 584 ◽  
Author(s):  
Naoki Itoh ◽  
Yasuharu Kohyama ◽  
Noriyoshi Matsumoto ◽  
Midori Seki

1993 ◽  
Vol 3 (8) ◽  
pp. 1201-1225 ◽  
Author(s):  
G. N�ron de Surgy ◽  
J.-P. Chabrerie ◽  
O. Denoux ◽  
J.-E. Wesfreid

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