Comment on ``Properties of 26Mg and 26Si in the sd shell model and the determination of the 25Al(p,γ)26Si reaction rate''

Details Comment on ``Properties of 26Mg and 26Si in the sd shell model and the determination of the 25Al(p,γ)26Si reaction rate'' Comment on ``Properties of 26Mg and 26Si in the sd shell model and the determination of the 25Al(p,γ)26Si reaction rate''

Nov 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011phrvc..84e9801c&link_type=abstract

Physical Review C, vol. 84, Issue 5, id. 059801

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1

Nucleosynthesis In Novae, Supernovae, And Other Explosive Environments, Coulomb Energies, Shell Model, Radiative Capture

Scientific paper

A recent discussion of theoretical work on the 25Al(p,γ)26Si astrophysical reaction rate [W.A. Richter, B. Alex Brown, A. Signoracci and M. Wiescher, Phys. Rev. CPRVCAN0556-281310.1103/PhysRevC.83.065803 83, 065803 (2011)] omits some current and relevant experimental information in forming its scientific conclusions. Accounting for this new information has the potential to significantly alter the reaction rate derived in the paper.

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