Published 1998
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The EOS and neutrino interactions in dense matter
Creators
- 1. Dept. of Physics and Astronomy, SUNY at Stony Brook, Stony Brook, NY (United States)
Description
The deleptonization and cooling times of a newly born neutron star depend on the equation of state (EOS) and neutrino opacities in dense matter. Through model calculations we show that effects of Pauli blocking and many-body correlations due to strong interactions reduce both the neutral and charged current neutrino cross sections by large factors compared to the case in which these effects are ignored. (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. 187-200.
- 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
- 29034965
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- CHARGED-CURRENT INTERACTIONS; CORRELATIONS; EQUATIONS OF STATE; MANY-BODY PROBLEM; NEUTRAL-CURRENT INTERACTIONS; NEUTRINO-NUCLEON INTERACTIONS; NEUTRON STARS; NUCLEAR MATTER; PAULI PRINCIPLE; RELATIVISTIC RANGE
- Descriptors DEC
- ENERGY RANGE; EQUATIONS; INTERACTIONS; LEPTON-BARYON INTERACTIONS; LEPTON-HADRON INTERACTIONS; LEPTON-NUCLEON INTERACTIONS; MATTER; PARTICLE INTERACTIONS; STARS