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Phys. Rev. C 85, 014607 (2012) [7 pages]

Correlation between the 12C+12C, 12C+13C, and 13C+13C fusion cross sections

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M. Notani1,*, H. Esbensen2, X. Fang1, B. Bucher1, P. Davies3, C. L. Jiang2, L. Lamm1,†, C. J. Lin4, C. Ma1, E. Martin3, K. E. Rehm2, W. P. Tan1, S. Thomas3, X. D. Tang1,‡, and E. Brown5
1Department of Physics, Institute for Structure and Nuclear Astrophysics, and the Joint Institute for Nuclear Astrophysics, University of Notre Dame, Notre Dame, Indiana 46556, USA
2Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
3Department of Physics, University of Surrey, Guildford, Surrey GU2 7XH, United Kingdom
4China Institute of Atomic Energy, P.O. Box 275(10), Beijing 102413, People's Republic of China
5Department of Physics & Astronomy, National Superconducting Cyclotron Laboratory, and the Joint Institute for Nuclear Astrophysics, Michigan State University, East Lansing, Michigan 48824, USA

Received 9 July 2011; revised 22 December 2011; published 17 January 2012

The fusion cross section for 12C+13C has been measured down to Ec.m.=2.6 MeV, at which the cross section is of the order of 20 nb. By comparing the cross sections for the three carbon isotope systems, 12C+12C, 12C+13C, and 13C+13C, it is found that the cross sections for 12C+13C and 13C+13C provide an upper limit for the fusion cross section of 12C+12C over a wide energy range. After calibrating the effective nuclear potential for 12C+12C using the 12C+13C and 13C+13C fusion cross sections, it is found that a coupled-channels calculation with the ingoing wave boundary condition (IWBC) is capable of predicting the major peak cross sections in 12C+12C. A qualitative explanation for this upper limit is provided by the Nogami-Imanishi model and by level density differences among the compound nuclei. It is found that the strong resonance found at 2.14 MeV in 12C+12C exceeds this upper limit by a factor of more than 20. The preliminary result from the most recent measurement shows a much smaller cross section at this energy, which agrees with our predicted upper limit.

©2012 American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevC.85.014607
DOI:
10.1103/PhysRevC.85.014607
PACS:
25.70.Jj, 24.30.-v, 25.70.Ef, 25.70.Gh

*Current address: APC Muon Accelerator R&D, Fermilab, Batavia, IL.

Deceased.

x.tang@nd.edu