Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
8190541 | Physics Letters B | 2012 | 4 Pages |
Abstract
Under astrophysical conditions of high temperature and density, such as for example found in X-ray bursts, breakout can occur from the hot CNO cycles into the rapid proton capture process. A key breakout route is via the sequence O15(α,γ)Ne19(p,γ)Na20. The Ne19(p,γ)Na20 reaction rate is expected to be dominated by a single resonance at 457(3) keV. The identity of the resonance has been under discussion for a long time, with JÏ=1+ and 3+ assignments suggested. In this study of the β-delayed proton decay of 20Mg we report a new, significantly more stringent, upper limit on the β-decay branch to this state of 0.02% with a confidence level of 90%. This makes a 1+ assignment highly unlikely and favours a 3+ assignment for which no branch is expected to be observed. The 3+ state is predicted to have a significantly higher resonance strength, and to produce a proportionately higher Ne19(p,γ)Na20 reaction rate in X-ray burst conditions.
Keywords
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Nuclear and High Energy Physics
Authors
J.P. Wallace, P.J. Woods, G. Lotay, A. Alharbi, A. Banu, H.M. David, T. Davinson, M. McCleskey, B.T. Roeder, E. Simmons, A. Spiridon, L. Trache, R.E. Tribble,