Physics Letters B (May 2019)

Proton decay of 108I and its significance for the termination of the astrophysical rp-process

  • K. Auranen,
  • D. Seweryniak,
  • M. Albers,
  • A.D. Ayangeakaa,
  • S. Bottoni,
  • M.P. Carpenter,
  • C.J. Chiara,
  • P. Copp,
  • H.M. David,
  • D.T. Doherty,
  • J. Harker,
  • C.R. Hoffman,
  • R.V.F. Janssens,
  • T.L. Khoo,
  • S.A. Kuvin,
  • T. Lauritsen,
  • G. Lotay,
  • A.M. Rogers,
  • C. Scholey,
  • J. Sethi,
  • R. Talwar,
  • W.B. Walters,
  • P.J. Woods,
  • S. Zhu

Journal volume & issue
Vol. 792
pp. 187 – 192

Abstract

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Employing the Argonne Fragment Mass Analyzer and the implantation-decay-decay correlation technique, a weak 0.50(21)% proton decay branch was identified in 108I for the first time. The 108I proton-decay width is consistent with a hindered l=2 emission, suggesting a d52 origin. Using the extracted 108I proton-decay Q value of 597(13) keV, and the Qα values of the 108I and 107Te isotopes, a proton-decay Q value of 510(20) keV for 104Sb was deduced. Similarly to the 112,113Cs proton-emitter pair, the Qp(I108) value is lower than that for the less-exotic neighbor 109I, possibly due to enhanced proton-neutron interactions in N≈Z nuclei. In contrast, the present Qp(Sb104) is higher than that of 105Sb, suggesting a weaker interaction energy. For the present Qp(Sb104) value, network calculations with the one-zone X-ray burst model Mazzocchi et al. (2007) [18] predict no significant branching into the Sn-Sb-Te cycle at 103Sn. Keywords: α decay, Proton decay, Astrophysical rp process, 104Sb, 107Te, 108I