Published January 2006
| Version v1
Journal article
Neutrino emissivity under neutral kaon condensation
Creators
- 1. Henryk Niewodniczanski Institute of Nuclear Physics, Polish Academy of Sciences, ul.Radzikowskiego 152, PL-31-342 Cracow (Poland)
Description
Neutrino emissivity from neutron star matter with neutral kaon condensate is considered. It is shown that a new cooling channel is opened and that all previously known channels acquire greater emissivity reaching the level of the direct URCA cycle in normal matter
Additional details
Identifiers
- DOI
- 10.1103/PhysRevC.73.015805;
- arXiv
- arXiv:astro-ph/0503659v2;
Publishing Information
- Journal Title
- Physical Review. C, Nuclear Physics
- Journal Volume
- 73
- Journal Issue
- 1
- Journal Page Range
- p. 015805-015805.6
- ISSN
- 0556-2813
- CODEN
- PRVCAN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 37076663
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS; S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- BOSE-EINSTEIN CONDENSATION; EMISSIVITY; KAONS NEUTRAL; NEUTRINOS; NEUTRON STARS; NUCLEAR MATTER
- Descriptors DEC
- BOSONS; ELEMENTARY PARTICLES; FERMIONS; HADRONS; KAONS; LEPTONS; MASSLESS PARTICLES; MATTER; MESONS; OPTICAL PROPERTIES; PHYSICAL PROPERTIES; PSEUDOSCALAR MESONS; STARS; STRANGE MESONS; STRANGE PARTICLES; SURFACE PROPERTIES
Optional Information
- Notes
- (c) 2006 The American Physical Society