Thermal evolution of isolated neutron stars

被引：0
|
作者：
Page, D [1 ]
机构：
[1] Univ Nacl Autonoma Mexico, Astron Inst, Mexico City, DF, Mexico
来源：
MANY FACES OF NEUTRON STARS | 1998年 / 515卷
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D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
I give a general overview of the theory of neutron star cooling, emphasizing the intuitive understanding of the effects of the various physical ingredients, including the recently proposed accreted envelopes and neutrino emission from Cooper pair breaking and formation. I describe how the present data may be compatible with both the 'standard model' and the fast-cooling scenarios, with or without invoking extensive presence of baryon pairing.
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页码：539 / 551
页数：13
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