2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/82878The equation of state and the properties of neutron stars are studied for a phase transition to a charged kaon condensate. We study the mixed phase by using Gibbs condition with comparison to the hitherto applied Maxwell construction. Implications for kaon condensation and for the mass-radius relation of condensed neutron stars are examined.6 pages, 3 figures, Proceedings of the International Workshop XXVI on Gross Properties of Nuclei and Nuclear Excitations: Nuclear Astrophysics, Hirschegg, Austria, January 11-17, 1998Nuclear TheoryAstrophysicstext