Thermonuclear reaction rate of 56Ni(p,γ)57Cu and 57Cu(p,γ)58Zn

Details Thermonuclear reaction rate of 56Ni(p,γ)57Cu and 57Cu(p,γ)58Zn Thermonuclear reaction rate of 56Ni(p,γ)57Cu and 57Cu(p,γ)58Zn

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001phrvc..64d5801f&link_type=abstract

Physical Review C (Nuclear Physics), Volume 64, Issue 4, October 2001, id.045801

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Nucleosynthesis In Novae, Supernovae, And Other Explosive Environments, Spectroscopic Factors And Asymptotic Normalization Coefficients, Radiative Capture, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages

Scientific paper

Updated stellar rates for the reactions 56Ni(p,γ)57Cu and 57Cu(p,γ)58Zn are calculated by using all available experimental information as well as input data from the nuclear shell model. We calculated Coulomb and Thomas-Ehrmann shifts to obtain the unknown excitation energies and the spin/parity assignments of 58Zn. The astrophysical consequences are discussed.

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