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Neutron stars - cooling and transport

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 نشر من قبل Alexander Potekhin
 تاريخ النشر 2015
  مجال البحث فيزياء
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Observations of thermal radiation from neutron stars can potentially provide information about the states of supranuclear matter in the interiors of these stars with the aid of the theory of neutron-star thermal evolution. We review the basics of this theory for isolated neutron stars with strong magnetic fields, including most relevant thermodynamic and kinetic properties in the stellar core, crust, and blanketing envelopes.



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