Publication Date:
2011-04-28
Description:
Author(s): A. Parikh, K. Wimmer, T. Faestermann, R. Hertenberger, J. José, R. Longland, H.-F. Wirth, V. Bildstein, S. Bishop, A. A. Chen, J. A. Clark, C. M. Deibel, C. Herlitzius, R. Krücken, D. Seiler, K. Straub, and C. Wrede Calculation of the thermonuclear ^{30} P(p,γ) ^{31} S rate in oxygen-neon nova explosions depends critically upon nuclear structure information for states within ∼600 keV of the ^{30} P+p threshold in ^{31} S. We have studied the ^{31} P(^{3} He,t) ^{31} S reaction at 25 MeV using a high-resoluti... [Phys. Rev. C 83, 045806] Published Wed Apr 27, 2011
Keywords:
Nuclear Astrophysics
Print ISSN:
0556-2813
Electronic ISSN:
1089-490X
Topics:
Physics