Edinburgh Research Explorer

Indirect study of the astrophysically important O(α, γ)Ne reaction through H(Ne, Ne)H

Research output: Contribution to journalArticle

  • A.M. Laird
  • S. Cherubini
  • A. Di Pietro
  • P. Figuera
  • W. Galster
  • J.S. Graulich
  • D. Groombridge
  • J. Hinnefeld
  • M. Lattuada
  • P. Leleux
  • L. Michel
  • A. Musumarra
  • A. Ninane
  • M.G. Pellegriti
  • C. Spitaleri
  • A. Tumino
  • J. Vervier

Related Edinburgh Organisations

Original languageEnglish
Pages (from-to)488011-488014
Number of pages4
JournalPhysical Review C
Volume66
Issue number4
StatePublished - 1 Oct 2002

Abstract

The O(α, γ) Ne reaction is generally considered as a potential breakout reaction from the hot CNO cycle. Under nova conditions, the reaction rate is dominated by a single sub-Coulomb resonance at E = 504 kev which corresponds to a Ne excitation energy of E = 4.033 MeV. Results from a d(Ne, Ne)p experiment show that states of astrophysical interest are populated in this reaction. An upper limit for the α-branching ratio of the 4.033 MeV state was identified and branching ratios for other states in Ne were found to be in good agreement with stable beam based results.

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