Laird, A.M., Cherubini, S., Ostrowski, A.N., Aliotta, M., Davinson, T., Di Pietro, A., Figuera, P., Galster, W., Graulich, J.S., Groombridge, D., Hinnefeld, J., Lattuada, M., Leleux, P., Michel, L., Musumarra, A., Ninane, A., Pellegriti, M.G., Shotter, A.C., Tumino, A., Vervier, J. and Woods, P. (2002) Indirect study of the astrophysically important 15O(alpha,gamma)19Ne reaction through 2H(18Ne,19Ne)1H. Physical Review C, 66 (4). Art. No. 048801. ISSN 1089-490XFull text not available from this repository.
The 15O(α,γ)19Ne reaction is generally considered as a potential breakout reaction from the hot CNO cycle. Under nova conditions, the reaction rate is dominated by a single sub-Coulomb resonance at Ec.m.=504 keV which corresponds to a 19Ne excitation energy of ER=4.033 MeV. Results from a d(18Ne,19Ne)p experiment show that states of astrophysical interest are populated in this reaction. An upper limit for the α-branching ratio of the 4.033 MeV state was identified and branching ratios for other states in 19Ne were found to be in good agreement with stable beam based results.
|Institution:||The University of York|
|Academic Units:||The University of York > Physics (York)|
|Depositing User:||York RAE Import|
|Date Deposited:||25 Feb 2009 15:47|
|Last Modified:||25 Feb 2009 18:13|
|Publisher:||The American Physical Society.|