Neutrino emissivity under neutral kaon condensation
arXiv:astro-ph/0503659 · doi:10.1103/PhysRevC.73.015805
Abstract
Neutrino emissivity from neutron star matter with neutral kaon condensate is considered. It is shown that a new cooling channel is opened, and what is more, all previously known channels acquire the greater emissivity reaching the level of the direct URCA cycle in normal matter.
arXiv comment7 pages, 1 figure, to be published in Phys.Rev.C, revised version: the sectioning changed and more discussion added
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