K-on Condensation and Cooling of Neutron Stars
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概要
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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 discussed. It is shown that rapid cooling of neutron stars is still possible even if there is no pion condensate inside neutron stars.
- 理論物理学刊行会の論文
- 1988-07-25
著者
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