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Lifetimes of states in Ne19 above the O15+α breakup threshold

  • S. Mythili*
  • , B. Davids
  • , T. K. Alexander
  • , G. C. Ball
  • , M. Chicoine
  • , R. S. Chakrawarthy
  • , R. Churchman
  • , J. S. Forster
  • , S. Gujrathi
  • , G. Hackman
  • , D. Howell
  • , R. Kanungo
  • , J. R. Leslie
  • , E. Padilla
  • , C. J. Pearson
  • , C. Ruiz
  • , G. Ruprecht
  • , M. A. Schumaker
  • , I. Tanihata
  • , C. Vockenhuber
  • P. Walden, S. Yen
*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

Abstract

The O15(α,γ)Ne19 reaction plays a role in the ignition of type I x-ray bursts on accreting neutron stars. The lifetimes of states in Ne19 above the O15+α threshold of 3.53 MeV are important inputs to calculations of the astrophysical reaction rate. These levels in Ne19 were populated in the He3(Ne20,α)Ne19 reaction at a Ne20 beam energy of 34 MeV. The lifetimes of six states above the threshold were measured with the Doppler-shift attenuation method. The present measurements agree with previous determinations of the lifetimes of these states and in some cases are considerably more precise.

Original languageEnglish
Article number035803
JournalPhysical Review C - Nuclear Physics
Volume77
Issue number3
DOIs
StatePublished - 11 Mar 2008
Externally publishedYes

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