Cooling of Neutron Stars and 3P₂ neutron gap
classification
🌌 astro-ph
nucl-th
keywords
neutroncoolingstarsdemonstrateddependencefavorisolatedmagnitude
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We 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.
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