Beta decay rates for nuclei with 115 < A < 140 for r-process nucleosynthesis
arXiv:astro-ph/0603517 · doi:10.1007/s12043-006-0081-2
Abstract
For r-process nucleosynthesis the beta decay rates for a number of neutron-rich intermediate heavy nuclei are calculated. The model for the beta strength function is able to reproduce the observed half~lives quite well.
arXiv commentTo be published in Pramana - Journal of Physics (Indian Academy of Sciences). 8 pages LaTeX
References in corpus (5)
- Nuclear weak-interaction processes in stars
- Beta decay of r-process waiting-point nuclei in a self-consistent approach
- Presupernova Evolution with Improved Rates for Weak Interactions
- Estimates of Stellar Weak Interaction Rates for Nuclei in the Mass Range A=65-80
- Shell Effects in Nuclei Near Neutron Drip