By the same authors

From the same journal

From the same journal

The Si-28(p,t)Si-26*(p) reaction and implications for the astrophysical Al-25(p,gamma)Si-26 reaction rate

Research output: Contribution to journalArticlepeer-review

Published copy (DOI)


  • K. A. Chipps
  • D. W. Bardayan
  • K. Y. Chae
  • J. A. Cizewski
  • R. L. Kozub
  • J. F. Liang
  • C. Matei
  • B. H. Moazen
  • C. D. Nesaraja
  • P. D. O'Malley
  • S. D. Pain
  • W. A. Peters
  • S. T. Pittman
  • K. T. Schmitt
  • M. S. Smith


Publication details

JournalPhysical Review C
DatePublished - 25 Oct 2010
Issue number4
Number of pages5
Pages (from-to)-
Original languageEnglish


Several resonances in Al-25(p,gamma)Si-26 have been studied via the Si-28(p,t)Si-26 reaction. Triton energies and angular distributions were measured using a segmented annular detector array. An additional silicon detector array was used to simultaneously detect the coincident protons emitted from the decay of states in Si-26 above the proton threshold in order to determine branching ratios. A resonance at 5927 +/- 4 keV has been experimentally confirmed as the first l = 0 state above the proton threshold, with a proton branching ratio consistent with one.

    Research areas

  • AL-26

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