Cooling of Neutron Stars and 3P_2 neutron gap

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dc.creatorGrigorian, H.
dc.creatorVoskresensky, D. N.
dc.date2005-01-31
dc.date2005-03-09
dc.date.accessioned2026-07-07T02:16:53Z
dc.date.available2026-07-07T02:16:53Z
dc.descriptionWe study the dependence of the cooling of isolated neutron stars on the magnitude of the $3P_2$ neutron gap. It is demonstrated that our ``Nuclear medium cooling scenario'' is in favor of a suppressed value of the $3P_2$ neutron gap.
dc.description9p., 14 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0501678
dc.identifierhttp://arxiv.org/abs/astro-ph/0501678
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8967
dc.subjectAstrophysics
dc.subjectNuclear Theory
dc.titleCooling of Neutron Stars and 3P_2 neutron gap
dc.typetext

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