Production of A=6,7 nuclides in the α+α reaction and cosmic ray nucleosynthesis

David J. Mercer, Sam M. Austin, J. A. Brown, S. A. Danczyk, S. E. Hirzebruch, J. H. Kelley, T. Suomijärvi, D. A. Roberts, and T. P. Walker
Phys. Rev. C 63, 065805 – Published 15 May 2001
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Abstract

Cross sections for production of 6He, 6Li, 7Li, and 7Be in the α+α reaction were measured at bombarding energies of 159.3, 279.6, and 619.8 MeV and are found to decrease rapidly with increasing energy. These cross sections are essential for the calculation of the rate of nucleosynthesis of the lithium isotopes in the cosmic rays and thereby play a key role in our understanding of the synthesis of Li, Be, and B. The results for 6Li differ significantly from the tabulated values commonly used in cosmic ray production calculations and lead to lower production of 6Li.

  • Received 1 October 2000

DOI:https://doi.org/10.1103/PhysRevC.63.065805

©2001 American Physical Society

Authors & Affiliations

David J. Mercer1,2,*, Sam M. Austin2,3,†, J. A. Brown2,‡, S. A. Danczyk2,3, S. E. Hirzebruch2, J. H. Kelley2,3,§, T. Suomijärvi2,4, D. A. Roberts5, and T. P. Walker6

  • 1Nuclear Physics Laboratory, University of Colorado, Boulder, Colorado 80309-0446
  • 2National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824
  • 3Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824
  • 4Institute de Physique Nucléaire, IN2P3-CNRS, F-91406 Orsay, France
  • 5Department of Physics, University of Michigan, Ann Arbor, Michigan, 48109
  • 6Department of Physics, The Ohio State University, Columbus, Ohio 43210

  • *Present address: NIS-5 Group, LANL, Los Alamos, NM 87545; electronic address: mercer@lanl.gov
  • Electronic address: austin@nscl.msu.edu
  • Present address: Physics Department, Millikin University, Decatur, IL 62522.
  • §Present address: Department of Physics, North Carolina State University, Raleigh, NC 27695.

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Vol. 63, Iss. 6 — June 2001

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