K-on Condensation and Cooling of Neutron Stars
Open Access
- 1 July 1988
- journal article
- Published by Oxford University Press (OUP) in Progress of Theoretical Physics
- Vol. 80 (1) , 22-27
- https://doi.org/10.1143/ptp.80.22
Abstract
K-on condensed phase is described on the basis of SU(3)L × SU(3)R chiral symmetry and then neutrino emmisivity inherent in this phase is discussed. It is shown that rapid cooling of neutron stars is still possible even if there is no pion condensate inside neutron stars.Keywords
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