Applications for fission product data to problems in stellar nucleosynthesis

Details Applications for fission product data to problems in stellar nucleosynthesis Applications for fission product data to problems in stellar nucleosynthesis

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983stin...8420458m&link_type=abstract

Presented at Spec. Meeting on Yields and Decay of Fission Product Nuclides, Upton, N.Y., 24 Oct. 1983

Astronomy and Astrophysics

Astrophysics

Astrophysics, Fission Products, Heavy Nuclei, Neutron Decay, Neutron Flux Density, Nuclear Capture, Nuclear Fusion, Stellar Models, Boltzmann Distribution, Isotopes, Nuclear Binding Energy, Red Giant Stars, Saha Equations, Shock Wave Interaction

Scientific paper

A general overview of the nucleosynthesis mechanisms for heavy (A greater than or equal to 70) nuclei is presented with particular emphasis on critical data needs. The current state of the art in nucleosynthesis model is described and areas in which fission product data may provide useful insight are proposed. The fission product data were divided into four categories (classical r-process, the n-process, p-process, and s-process) and applied to the study of heavy nuclei generation.

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