Kaons in Nuclear Matter

Simple item page
dc.creatorHeiselberg, Henning
dc.date1998-02-05
dc.date.accessioned2026-07-07T02:25:59Z
dc.date.available2026-07-07T02:25:59Z
dc.descriptionThe kaon energy in a nuclear medium and its dependence on kaon-nucleon and nucleon-nucleon correlations is discussed. The transition from the Lenz potential at low densities to the Hartree potential at high densities can be calculated analytically by making a Wigner-Seitz cell approximation and employing a square well potential. As the Hartree potential is less attractive than the Lenz one, kaon condensation inside cores of neutron stars appears to be less likely than previously estimated.
dc.description5 pages, Proc. of "Nuclear Astrophysics", Hirschegg jan. 11-17, 1998
dc.identifierhttps://arxiv.org/abs/astro-ph/9802062
dc.identifierhttp://arxiv.org/abs/astro-ph/9802062
dc.identifierNordita-98/8 N/A
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12097
dc.subjectAstrophysics
dc.subjectNuclear Theory
dc.titleKaons in Nuclear Matter
dc.typetext

Files

Collections

arXiv