Cooling of Neutron Stars. Hadronic Model

Abstract

We study the cooling of isolated neutron stars. The main cooling regulators are introduced: EoS, thermal transport, heat capacity, neutrino and photon emissivity, superfluid nucleon gaps. Neutrino emissivity includes main processes. A strong impact of medium effects on the cooling rates is demonstrated. With taking into account of medium effects in reaction rates and in nucleon superfluid gaps modern experimental data can be well explained.

15 pages, 23 figures, aa.cls style included

References in corpus (2)

• Thermal states of coldest and hottest neutron stars in soft X-ray transients
• Neutron star cooling: Theoretical aspects and observational constraints

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