Neutron superfluidity and the cooling of neutron stars

被引：0
作者：
Vigezzi, E
Barranco, F
Broglia, RA
Pizzochero, PM
机构：
[1] Ist Nazl Fis Nucl, Sez Milano, I-20133 Milan, Italy
[2] Excuela Super Ingn, Dept Fis Aplicada 3, Seville, Spain
[3] Univ Milan, Dipartimento Fis, I-20133 Milan, Italy
[4] Univ Copenhagen, Niels Bohr Inst, DK-2100 Copenhagen, Denmark
来源：
ACTA PHYSICA POLONICA B | 2003年 / 34卷 / 04期
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D O I：
暂无
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
We present a mean field quantum calculation of the superfluidity in the inner crust of neutron stars, taking into account the inhomogeneous character of the system, in which a lattice of neutron-rich nuclei coexists with a gas of unbound neutrons. We compare the resulting thermal properties of the star with those obtained neglecting the nuclear impurities.
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页码：2185 / 2193
页数：9
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