Published March 1999
| Version v1
Journal article
Microscopic calculations of stellar weak rates for sd- and fp-shell nuclei for astrophysical applications
- 1. Max-Planck-Institut fuer Kernphysik, Heidelberg (Germany)
Description
Proton-neutron quasiparticle RPA is used for the first time to calculate weak interaction rates for sd- and fp-shell nuclei at high temperatures and densities. The calculated rates take into consideration the latest experimental energy levels and ft value compilations. Particle emission processes from excited states are taken into account. The calculation is done for 700 nuclei with mass number ranging from 18 to 100. The astrophysical applications of the calculated rates are highlighted. (author)
Additional details
Publishing Information
- Journal Title
- Acta Physica Polonica. Series B
- Journal Volume
- 30
- Journal Issue
- 3
- Journal Page Range
- p. 825-833
- ISSN
- 0587-4254
Conference
- Title
- Trends in Nuclear Physics - 23. Zakopane School of Physics
- Dates
- 1-9 Sep 1998
- Place
- Zakopane (Poland)
INIS
- Country of Publication
- Poland
- Country of Input or Organization
- Poland
- INIS RN
- 30030413
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ASTROPHYSICS; BETA DECAY; MEETINGS; NEUTRON-RICH ISOTOPES; NUCLEAR MATTER; STAR EVOLUTION; SUPERNOVAE; WEAK INTERACTIONS
- Descriptors DEC
- BASIC INTERACTIONS; BETA DECAY RADIOISOTOPES; BETA-MINUS DECAY RADIOISOTOPES; BINARY STARS; DECAY; ERUPTIVE VARIABLE STARS; INTERACTIONS; ISOTOPES; MATTER; NUCLEAR DECAY; RADIOISOTOPES; STARS; VARIABLE STARS
Optional Information
- Notes
- 32 refs, 1 fig