Shell-model calculations of beta-decay rates for s- and r-process nucleosyntheses

Details Shell-model calculations of beta-decay rates for s- and r-process nucleosyntheses Shell-model calculations of beta-decay rates for s- and r-process nucleosyntheses

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985acs..meets....t&link_type=abstract

Presented at the 190th American Chemical Society National Meeting, Chicago, Ill., 8 Sep. 1985

Statistics

Computation

Nuclear Fusion, Nuclear Models, Radioactive Decay, Shell Theory, Stellar Evolution, Astrophysics, Atomic Excitations, Beta Particles, Computation

Scientific paper

Examples of large-basis shell-model calculations of Gamow-Teller (BETA)-decay properties of specific interest in the astrophysical s- and r- processes are presented. Numerical results are given for: (1) the GT-matrix elements for the excited state decays of the unstable s-process nucleus Tc-99; and (2) the GT-strength function for the neutron-rich nucleus Cd-130, which lies on the r-process path. The results are discussed in conjunction with the astrophysics problems.

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