1. The 21Na(p,gamma)22Mg Reaction and Oxygen-Neon Novae
- Author
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Bishop, S., Azuma, R. E., Buchmann, L., Chen, A. A., Chatterjee, M. L., D'Auria, J. M., Engel, S., Gigliotti, D., Greife, U., Hernanz, M., Hunter, D., Hussein, A., Hutcheon, D., Jewett, C., Jose, J., King, J., Kubono, S., Laird, A. M., Lamey, M., Lewis, R., Liu, W., Michimasa, S., Olin, A., Ottewell, D., Parker, P. D., Rogers, J. G., Strieder, F., and Wrede, C.
- Subjects
Astrophysics ,Nuclear Experiment - Abstract
The 21Na(p,gamma)22Mg reaction is expected to play an important role in the nucleosynthesis of 22Na in Oxygen-Neon novae. The decay of 22Na leads to the emission of a characteristic 1.275 MeV gamma-ray line. This report provides the first direct measurement of the rate of this reaction using a radioactive 21Na beam, and discusses its astrophysical implications. The energy of the important state was measured to be E$_{c.m.}$= 205.7 $\pm$ 0.5 keV with a resonance strength $\omega\gamma = 1.03\pm0.16_{stat}\pm0.14_{sys}$ meV., Comment: Accepted for publication in Physical Review Letters
- Published
- 2003
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