Superfluid phases of triplet pairing and neutrino emission from neutron stars
L. B. Leinson

TL;DR
This paper investigates how superfluid triplet neutron pairing in neutron stars leads to enhanced neutrino emission via spin waves, significantly impacting neutron star cooling, especially at low temperatures.
Contribution
It introduces the analysis of collective spin density waves in multicomponent superfluid phases and their role in neutrino emission, highlighting a phase transition effect on cooling.
Findings
Spin waves cause substantial neutrino emission at low temperatures.
Neutrino losses sharply increase then decrease during phase transitions.
Spin wave decay significantly influences neutron star cooling.
Abstract
Neutrino energy losses through neutral weak currents in the triplet-spin superfluid neutron liquid are studied for the case of condensate involving several magnetic quantum numbers. Low-energy excitations of the multicomponent condensate in the timelike domain of the energy and momentum are analyzed. Along with the well-known excitations in the form of broken Cooper pairs, the theoretical analysis predicts the existence of collective waves of spin density at very low energy. Because of a rather small excitation energy of spin waves, their decay leads to a substantial neutrino emission at the lowest temperatures, when all other mechanisms of neutrino energy loss are killed by a superfluidity. Neutrino energy losses caused by the pair recombination and spin-wave decays are examined in all of the multicomponent phases that might represent the ground state of the condensate, according to…
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