Medium Effects in Cooling of Neutron Stars and 3P₂ Neutron Gap
classification
🌌 astro-ph
hep-phnucl-th
keywords
neutroncoolingmediumstarsdemonstrateddependenceeffectsfavor
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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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