Exploring the [Formula Presented] gateway to the formation of heavy elements in hot stars

  • K. E. Rehm
  • , C. L. Jiang
  • , M. Paul
  • , D. Blumenthal
  • , L. A. Daniel
  • , C. N. Davids
  • , P. Decrock
  • , S. M. Fischer
  • , D. Henderson
  • , C. Lister
  • , J. Nickles
  • , J. Nolen
  • , R. C. Pardo
  • , J. P. Schiffer
  • , D. Seweryniak
  • , R. E. Segel

Research output: Contribution to journalArticlepeer-review

27 Scopus citations

Abstract

An upper limit to the production of [Formula Presented] through the [Formula Presented] reaction at the recently discovered [Formula Presented]-wave resonance has been determined. The limit implies that in a hot stellar environment [Formula Presented] this reaction is not a significant gateway from the hot CNO cycle towards the production of heavier elements in stars.

Original languageEnglish
Pages (from-to)R566-R569
JournalPhysical Review C - Nuclear Physics
Volume55
Issue number2
DOIs
StatePublished - 1997

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