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.

arXiv comment9p., 14 figures

References in corpus (7)

• Cooling of Neutron Stars with Color Superconducting Quark Cores
• Phase Transitions in Nucleonic Matter and Neutron-Star Cooling
• Rearrangement of the Fermi Surface of Dense Neutron Matter and Direct Urca Cooling of Neutron Stars
• Direct Urca neutrino radiation from superfluid baryonic matter
• Neutrino Cooling of Neutron Stars. Medium effects
• Testing Pulsar Thermal Evolution Theories with Observation
• Superfluidity in Neutron Star Matter

Cited by in corpus (2)

• Brightness constraint for cooling models of young neutron stars
• Hot Neutron and Quark Star Evolution