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Search for a resonant enhancement of the 7Be + d reaction and primordial 7Li abundances

  • P. D. O'Malley
  • , D. W. Bardayan
  • , A. S. Adekola
  • , S. Ahn
  • , K. Y. Chae
  • , J. A. Cizewski
  • , S. Graves
  • , M. E. Howard
  • , K. L. Jones
  • , R. L. Kozub
  • , L. Lindhardt
  • , M. Matos
  • , B. M. Moazen
  • , C. D. Nesaraja
  • , S. D. Pain
  • , W. A. Peters
  • , S. T. Pittman
  • , K. T. Schmitt
  • , J. F. Shriner
  • , M. S. Smith
  • I. Spassova, S. Y. Strauss, J. L. Wheeler
  • Rutgers - The State University of New Jersey, New Brunswick
  • Oak Ridge National Laboratory
  • University of Tennessee
  • Tennessee Technological University
  • Louisiana State University
  • Oak Ridge Associated Universities

Research output: Contribution to journalArticlepeer-review

Abstract

Big Bang nucleosynthesis calculations, constrained by the Wilkinson Microwave Anisotropy Probe results, produce 7Li abundances almost a factor of four larger than those extrapolated from observations. Since primordial 7Li is believed to be mostly produced by the beta decay of 7Be, one proposed solution to this discrepancy is a resonant enhancement of the 7Be(d,p)2α reaction rate through the 5/2+ 16.7-MeV state in 9B. The 2H(7Be,d)7Be reaction was used to search for such a resonance; none was observed. An upper limit on the width of the proposed resonance was deduced.

Original languageEnglish
Article number042801
JournalPhysical Review C - Nuclear Physics
Volume84
Issue number4
DOIs
StatePublished - 17 Oct 2011

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