Published 1998
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Kaons in nuclear matter
Description
The 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. (orig.)
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Additional details
Publishing Information
- Imprint Title
- Nuclear astrophysics.Proceedings of the International workshop XXVI on gross properties of nuclei and nuclear excitations
- Imprint Pagination
- 442 p.
- Journal Page Range
- p. 96-100.
- Report number
- INIS-DE--0012
Conference
- Title
- Nuclear astrophysics (Hirschegg '98).
- Acronym
- 26. international workshop on gross properties of nuclei and nuclear excitations
- Dates
- 11-17 Jan 1998.
- Place
- Hirschegg (Austria).
INIS
- Country of Publication
- Germany
- Country of Input or Organization
- Germany
- INIS RN
- 29034967
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- HARTREE-FOCK METHOD; KAON-NUCLEON INTERACTIONS; KAONS; KLEIN-GORDON EQUATION; NEUTRON STARS; NUCLEAR MATTER; NUCLEON-NUCLEON INTERACTIONS; SQUARE-WELL POTENTIAL
- Descriptors DEC
- BARYON-BARYON INTERACTIONS; BOSONS; CALCULATION METHODS; DIFFERENTIAL EQUATIONS; ELEMENTARY PARTICLES; EQUATIONS; FIELD EQUATIONS; HADRON-HADRON INTERACTIONS; HADRONS; INTERACTIONS; MATTER; MESON-BARYON INTERACTIONS; MESON-NUCLEON INTERACTIONS; MESONS; NUCLEAR POTENTIAL; PARTIAL DIFFERENTIAL EQUATIONS; PARTICLE INTERACTIONS; POTENTIALS; PSEUDOSCALAR MESONS; STARS; STRANGE MESONS; STRANGE PARTICLES; WAVE EQUATIONS