Microscopic calculations of stellar weak rates for sd- and fp-shell nuclei for astrophysical applications.

Details Microscopic calculations of stellar weak rates for sd- and fp-shell nuclei for astrophysical applications. Microscopic calculations of stellar weak rates for sd- and fp-shell nuclei for astrophysical applications.

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999acppb..30..825n&link_type=abstract

Acta Phys. Pol., B, Vol. 30, No. 3, p. 825 - 833

Astronomy and Astrophysics

Astrophysics

2

Nuclear Reactions: Astrophysics

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. 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.

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