The superfluid phase transition in neutron star matter
- 1 June 1979
- journal article
- Published by IOP Publishing in Journal of Physics A: General Physics
- Vol. 12 (6) , L147-L149
- https://doi.org/10.1088/0305-4470/12/6/004
Abstract
The Ginzburg-Landau free energy describing p wave paired neutron star matter is used to derive renormalisation group equations. The absence of infrared stable fixed points indicates a first order phase transition.Keywords
This publication has 8 references indexed in Scilit:
- pairing near the transition temperature in neutron-star matterPhysical Review D, 1978
- Beta decay of pion condensates as a cooling mechanism for neutron starsThe Astrophysical Journal, 1977
- Phase transitions not controlled by stable fixed pointsJournal of Physics C: Solid State Physics, 1977
- Phase transitions in superfluid3HeJournal of Physics C: Solid State Physics, 1976
- Discussion of critical phenomena for general-vector modelsPhysical Review B, 1974
- Dimensional regularization and the renormalization groupNuclear Physics B, 1973
- Energy Gap in Neutron-Star MatterProgress of Theoretical Physics, 1972
- Anisotropic Superfluidity in Neutron Star MatterPhysical Review Letters, 1970