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The 25Al(p,gamma)26Si Reaction Rate in Novae...

Publication Type
Conference Paper
Journal Name
PoS - Proceedings of Science
Publication Date
Page Number
217
Volume
NIC-IX
Conference Name
International Symposium on Nuclear Astrophysics - Nuclei in the Cosmos IX
Conference Location
Geneva, Switzerland
Conference Date
-

The production of 26Al in novae is uncertain, in part, because of the uncertain rate of the
25Al(p,g)26Si reaction at novae temperatures. This reaction is thought to be dominated by a longsought
3+ level in 26Si, and the calculated reaction rate varies by orders of magnitude depending
on the energy of this resonance. We present evidence concerning the spin of a level at 5.914
MeV in 26Si from the 28Si(p,t)26Si reaction studied at the Holifield Radioactive Beam Facility at
ORNL. We find that the angular distribution for this level implies either a 2+ or 3+ assignment,
with only a 3+ being consistent with the mirror nucleus, 26Mg. Additionally, we have used the
updated 25Al(p,g)26Si reaction rate in a nova nucleosynthesis calculation and have addressed the
effects of the remaining uncertainties in the rate on 26Al production.