Superfluid phases of triplet pairing and rapid cooling of the neutron star in cassiopeia A

DOI10.1016/J.PHYSLETB.2014.12.017zbMath1373.85002arXiv1411.6833OpenAlexW2161840757MaRDI QIDQ1674734

Lev B. Leinson

Publication date: 26 October 2017

Published in: Physics Letters. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1411.6833

zbMATH Keywords

superfluidityneutron starneutrino radiation

Mathematics Subject Classification ID

Statistical mechanics of superfluids (82D50) Galactic and stellar structure (85A15)

Related Items (4)

QCD axion and neutrino physics induced by hidden flavor structure ⋮ The landscape of QCD axion models ⋮ Neutrino emission from Cooper pairs at finite temperatures ⋮ Fermion masses and flavor mixings and strong CP problem

Cites Work

• \(^3P_2-^3F_2\) pairing in dense neutron matter: the spectrum of solutions

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