Cooling of Neutron Stars and 3P_2 neutron gap
H. Grigorian, D.N. Voskresensky
TL;DR
This paper investigates how the cooling behavior of isolated neutron stars is affected by the size of the 3P_2 neutron gap, supporting a suppressed gap value within the nuclear medium cooling framework.
Contribution
It introduces a nuclear medium cooling scenario that favors a suppressed 3P_2 neutron gap for neutron star cooling.
Findings
Suppressed 3P_2 neutron gap aligns with observed cooling data.
Nuclear medium effects are significant in neutron star cooling models.
The scenario improves agreement between theory and observations.
Abstract
We study the dependence of the cooling of isolated neutron stars on the magnitude of the neutron gap. It is demonstrated that our ``Nuclear medium cooling scenario'' is in favor of a suppressed value of the neutron gap.
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Geophysics and Gravity Measurements · Atomic and Subatomic Physics Research