From Kaon-Nuclear Interactions to Kaon Condensation
arXiv:hep-ph/9304204 · doi:10.1016/0375-9474(94)90335-2
Abstract
An effective chiral Lagrangian in heavy-fermion formalism whose parameters are constrained by kaon-nucleon and kaon-nuclear interactions next to the leading order in chiral expansion is used to describe kaon condensation in dense ``neutron star" matter. The critical density is found to be robust with respect to the parameters of the chiral Lagrangian and comes out to be . Once kaon condensation sets in, the system is no longer composed of neutron matter but of nuclear matter. Possible consequences on stellar collapse with the formation of compact ``nuclear stars" or light-mass black holes are pointed out.
20 pages, LaTeX, NORDITA-93/30 N, SUNY-NTG-93-7
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Cited by in corpus (154)
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