Estimates of Stellar Weak Interaction Rates for Nuclei in the Mass Range <i>A</i> = 65โ80
Estimates of Stellar Weak Interaction Rates for Nuclei in the Mass Range <i>A</i> = 65โ80
We estimate lepton capture and emission rates, as well as neutrino energy loss rates, for nuclei in the mass range A=65-80. These rates are calculated on a temperature/density grid appropriate for a wide range of astrophysical applications including simulations of late time stellar evolution and x-ray bursts. The basic inputs โฆ