Computer Science – Numerical Analysis
Scientific paper
Sep 1974
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974phdt........37b&link_type=abstract
Ph.D. Thesis Arizona Univ., Tucson.
Computer Science
Numerical Analysis
Calcium Isotopes, Nuclear Fusion, Reaction Kinetics, Stellar Mass, Cross Sections, Numerical Analysis, Stellar Interiors, Temperature Effects
Scientific paper
The cross section for the reactions Ca-40 (alpha, gamma) Ti-44, Ca-40 (alpha, p) Sc-43, and Ca-48 (alpha, n) Ti-51 were measured between the center of mass energies of 3.5 MeV and 9.0 MeV. These cross sections were used to calculate reaction rates as a function of temperature for stellar interior and compared to theoretical predictions of the equivalent square well model.
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