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Phys. Rev. C 75, 024607 (2007) [6 pages]

Lowest excited states of 13O

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B. B. Skorodumov1,*, G. V. Rogachev2, P. Boutachkov1, A. Aprahamian1, V. Z. Goldberg3, A. Mukhamedzhanov3, S. Almaraz1, H. Amro4, F. D. Becchetti4, S. Brown2,5, Y. Chen4, H. Jiang4, J. J. Kolata1, L. O. Lamm1, M. Quinn1, and A. Woehr1
1Institute for Structure and Nuclear Astrophysics, University of Notre Dame, Notre Dame, Indiana 46556, USA
2Physics Department, Florida State University, Tallahassee, Florida 32306, USA
3Texas A&M University, College Station, Texas 77843, USA
4Physics Department, University of Michigan, Ann Arbor, Michigan 48109, USA
5Department of Physics, University of Surrey, GU2 7XH, United Kingdom

Received 1 May 2006; published 14 February 2007

An excitation function for resonance elastic scattering of p+12N was measured in the center of mass energy range of 0.8–2.7 MeV. Measurements were performed using inverse kinematics and the thick-target techniques. The data were analyzed in the framework of the R-matrix formalism. A definitive spin and parity assignment was possible for the first excited state of 13O at an excitation energy of 2.69 MeV as Jπ=1/2+. An indication of the presence of a new level in 13O at an excitation energy of 3.29 MeV with tentative spin-parity assignment Jπ=1/2- or 3/2- was obtained. We evaluate the impact of this measurement on the reaction rate of 12N(p,γ)13O for nucleosynthesis in low-metallicity stars.

© 2007 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevC.75.024607
DOI:
10.1103/PhysRevC.75.024607
PACS:
21.10.-k, 24.30.-v, 27.20.+n

*Electronic address: bskorodo@nd.edu