Cooling of Neutron Stars. Hadronic Model

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dc.creatorBlaschke, D.
dc.creatorGrigorian, H.
dc.creatorVoskresensky, D. N.
dc.date2004-03-07
dc.date.accessioned2026-07-07T02:12:32Z
dc.date.available2026-07-07T02:12:32Z
dc.descriptionWe 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.
dc.description15 pages, 23 figures, aa.cls style included
dc.identifierhttps://arxiv.org/abs/astro-ph/0403170
dc.identifierhttp://arxiv.org/abs/astro-ph/0403170
dc.identifierAstron.Astrophys. 424 (2004) 979-992
dc.identifierdoi:10.1051/0004-6361:20040404
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7487
dc.subjectAstrophysics
dc.subjectNuclear Theory
dc.titleCooling of Neutron Stars. Hadronic Model
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