Formation of an anisotropic energy gap in the valence-fluctuating system of CeNiSn

1990 ◽  
Vol 41 (13) ◽  
pp. 9607-9610 ◽  
Author(s):  
T. Takabatake ◽  
F. Teshima ◽  
H. Fujii ◽  
S. Nishigori ◽  
T. Suzuki ◽  
...  
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1987 ◽  
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pp. 1253
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Yoshio Kitaoka ◽  
Yutaka Kishimoto ◽  
Tatsuo Kobayashi ◽  
Kiichi Amaya ◽  
Kunisuke Asayama

1992 ◽  
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M. Nagasawa ◽  
H. Fujii ◽  
M. Nohara ◽  
T. Suzuki ◽  
...  

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M. A. SHAHZAMANIAN ◽  
H. YAVARY

The components of the diffusive thermal conductivity tensor of superfluid neutron stars are calculated by using anisotropic energy gap for 3p2 pairing and approximation collision integrals at temperatures where [Formula: see text]. The contribution from neutron–neutron collisions is taken into account. Nonrelativistic effects for pairing will be studied. A comparison with the corresponding relativistic case is also made.


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