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Cooling Of Neutron Stars. Hadronic Model

ASTRONOMY & ASTROPHYSICS, no. 3 (2004): 979-992

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academic.microsoft.com arxiv.org

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dense matter equation of state neutrinos stars : evolution stars : neutron更多(1+)

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We study the cooling of isolated neutron stars. The main cooling regulators are introduced: equation of state (EoS), thermal transport, heat capacity, neutrino and photon emissivity, superfluid nucleon gaps. The neutrino emissivity includes the main processes. A strong impact of medium effects on the cooling rates is demonstrated. Taking ...更多

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