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The Ne(p,γ)Na astrophysical reaction rate determined from measurements with a radioactive beam

Research output: Contribution to journalArticle

  • G. Vancraeynest
  • C.R. Bain
  • F. Binon
  • R. Coszach
  • P. Decrock
  • Th. Delbar
  • P. Duhamel
  • M. Gaelens
  • W. Galster
  • J.-S. Graulich
  • M. Huyse
  • P. Leleux
  • I. Licot
  • E. Liénard
  • P. Lipnik
  • C. Michotte
  • A. Ninane
  • R.D. Page
  • P.J. Sellin
  • Cs. Sükösd
  • P. Van Duppen
  • J. Vanhorenbeeck
  • J. Vervier
  • M. Wiescher

Related Edinburgh Organisations

Original languageEnglish
JournalNuclear Physics A
Volume616
Issue number1-2
Publication statusPublished - 14 Apr 1997

Abstract

The Ne(p,γ)Na as well as the Ne(d,n)Na reaction have been studied in inverse kinematics using Ne radioactive beams. Upper and lower limits for the Ne(p,γ)Na astrophysical reaction rate have been deduced, for the first time on the basis of direct experimental data. It is concluded that the transition from the hot-CNO cycle to the rp-process in explosive hydrogen burning is most likely governed by the preceeding O(a,γ)Ne reaction.

ID: 14703758