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Study of the F18(p)15O reaction at astrophysical energies using a F18 beam

  • K. E. Rehm*
  • , M. Paul
  • , A. D. Roberts
  • , D. J. Blumenthal
  • , J. Gehring
  • , D. Henderson
  • , C. L. Jiang
  • , J. Nickles
  • , J. Nolen
  • , R. C. Pardo
  • , J. P. Schiffer
  • , R. E. Segel
  • *Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

54 Scopus citations

Abstract

For the first time the F18(p)15O reaction has been studied with a F18 beam at energies which are of interest to explosive nucleosynthesis. Utilizing the gas-filled magnet technique a clean identification of the reaction products was achieved. A resonance with spin 3/2+ at an equivalent c.m. energy of 660 keV dominates the yield.

Original languageEnglish
Pages (from-to)R460-R463
JournalPhysical Review C - Nuclear Physics
Volume52
Issue number2
DOIs
StatePublished - 1995

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