Comment on “Properties of 26Mg and 26Si in the sd shell model and the determination of the 25Al(p, gamma)26Si reaction rate”
A recent discussion of theoretical work on the 25Al(p,gamma)26Si astrophysical reaction rate [W.A. Richter, B. Alex Brown, A. Signoracci and M. Wiescher, Phys. Rev. C 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.
CHIPPS K. A.;
BARDAYAN D. W.;
CHAE K.Y.;
CIZEWSKI J. A.;
KOZUB R. L.;
LIANG J. F.;
MATEI Catalin;
O’MALLEY P. D.;
PAIN S. D.;
PETERS W. A.;
PITTMAN S. T.;
SMITH M. S.;
2012-06-22
AMER PHYSICAL SOC
JRC66367
0556-2813,
https://publications.jrc.ec.europa.eu/repository/handle/JRC66367,
10.1103/PhysRevC.84.059801,
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