Rate Tables for the Weak Processes of pf-SHELL Nuclei in Stellar Environments

Details Rate Tables for the Weak Processes of pf-SHELL Nuclei in Stellar Environments Rate Tables for the Weak Processes of pf-SHELL Nuclei in Stellar Environments

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001adndt..79....1l&link_type=abstract

Atomic Data and Nuclear Data Tables, Volume 79, Issue 1, p. 1-46.

Computer Science

53

Scientific paper

The weak interaction rates in stellar environments are computed for pf-shell nuclei in the mass range A=45-65 using large-scale shell-model calculations. The calculated capture and decay rates take into consideration the latest experimental energy levels and log ft-values. The rates are tabulated at the same grid points of density and temperature as those used by Fuller, Fowler, and Newman for densities ρYe=10-1011 g/cm3 and temperatures T=107-1011 K, and hence are relevant for both types of supernovae (Type Ia and Type II). Effective values for capture rates and average neutrino (antineutrino) energies are also given to facilitate the use of interpolated rates in stellar evolution codes.

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