Neutrino emissivity under neutral kaon condensation
Astrophysics
2009-11-10 v2
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.
Keywords
Cite
@article{arxiv.astro-ph/0503659,
title = {Neutrino emissivity under neutral kaon condensation},
author = {Sebastian Kubis},
journal= {arXiv preprint arXiv:astro-ph/0503659},
year = {2009}
}
Comments
7 pages, 1 figure, to be published in Phys.Rev.C, revised version: the sectioning changed and more discussion added