Weak interaction rates at high temperatures and densities

Details Weak interaction rates at high temperatures and densities Weak interaction rates at high temperatures and densities

Jul 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aipc..478..230n&link_type=abstract

Second international workshop on particle physics and the early universe (COSMO-98). AIP Conference Proceedings, Volume 478, pp

Other

Elementary Particle Processes, Weak-Interaction And Lepton Aspects, Hydrostatic Stellar Nucleosynthesis, Nucleosynthesis In Novae, Supernovae, And Other Explosive Environments

Scientific paper

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. Particle emission processes from excited states are taken into account and is found to considerably affect the recommended β decay rates. The calculated rates take into consideration the latest experimental energy levels and ft value compilations. The calculation is done for 709 nuclei with mass number ranging from 18 to 100. The astrophysical applications of the calculated rates are highlighted.

Affiliated with

Also associated with

No associations

Rating

Weak interaction rates at high temperatures and densities does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Weak interaction rates at high temperatures and densities, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Weak interaction rates at high temperatures and densities will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1618285