Nuclear astrophysics away from stability

Details Nuclear astrophysics away from stability Nuclear astrophysics away from stability

Aug 1985

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

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

Astronomy and Astrophysics

Astrophysics

Astrophysics, Nuclear Astrophysics, Nuclear Fusion, Stars, Stellar Models, High Temperature, Hydrogen, Stability, Theoretical Physics

Scientific paper

Explosive astrophysical environments invariably lead to the production of nuclei away from stability. An understanding of the dynamics and nucleosynthesis in such environments is inextricably coupled to an understanding of the properties of the synthesized nuclei. In this talk a review is presented of the basic explosive nucleosynthesis mechanisms (s-process, r-process, n-process, p-process, and rp-process). Specific stellar model calculations are discussed and a summary of the pertinent nuclear data is presented. Possible experiments and nuclear-model calculations are suggested that could facilitate a better understanding of the astrophysical scenarios.

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