Medium Effects in Cooling of Neutron Stars and $3P_2$ Neutron Gap

Abstract

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.

18 p., 12 figs., extended version of astro-ph/0501678, accepted in A&A

References in corpus (6)

• Cooling of Neutron Stars. Hadronic Model
• Cooling of Neutron Stars with Color Superconducting Quark Cores
• Relativistic Mean-Field Models with Effective Hadron Masses and Coupling Constants, and rho^- Condensation
• Thermal states of coldest and hottest neutron stars in soft X-ray transients
• Neutron star cooling: Theoretical aspects and observational constraints
• Direct Urca neutrino radiation from superfluid baryonic matter

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