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Measurement of the F(p,α)O cross section at nova energies

Research output: Contribution to journalArticle

  • D.W. Bardayan
  • J.C. Batchelder
  • J.C. Blackmon
  • A.E. Champagne
  • T. Davinson
  • R. Fitzgerald
  • W.R. Hix
  • C. Iliadis
  • R.L. Kozub
  • Z. Ma
  • S. Parete-Koon
  • P.D. Parker
  • N. Shu
  • M.S. Smith
  • P.J. Woods

Related Edinburgh Organisations

Original languageEnglish
JournalNuclear Physics A
Volume723
Issue number1-2
DOIs
Publication statusPublished - 28 Jul 2003

Abstract

Production of the radioisotope F in novae is severely constrained by the rate of the F(p,α)O reaction. A resonance at E = 330 keV may strongly enhance the 18F(p,α)O reaction rate, but its strength has been very uncertain. We have determined the strength of this important resonance by measuring the F(p,α)O cross section on-and off-resonance using a radioactive F beam at ORNL's Holifield Radioactive Ion Beam Facility. We find that its resonance strength is 1.48 ± 0.46 eV, and that it dominates the F(p,α)O reaction rate over a significant range of temperatures characteristic of nova outbursts occuring on ONeMg white dwarfs.

ID: 14693574