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

K. A. Chipps, D. W. Bardayan, K. Y. Chae, J. A. Cizewski, R. L. Kozub, J. F. Liang, C. Matei, P. D. O'Malley, S. D. Pain, W. A. Peters, S. T. Pittman, M. S. Smith

Research output: Contribution to journalArticlepeer-review

3 Scopus citations

Abstract

A recent discussion of theoretical work on the 25Al(p,γ)26Si astrophysical reaction rate 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.

Original languageEnglish
Article number059801
JournalPhysical Review C - Nuclear Physics
Volume84
Issue number5
DOIs
StatePublished - Nov 7 2011

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