Physics Letters B (Sep 2017)

Unexpected high-energy γ emission from decaying exotic nuclei

  • A. Gottardo,
  • D. Verney,
  • I. Deloncle,
  • S. Péru,
  • C. Delafosse,
  • S. Roccia,
  • I. Matea,
  • C. Sotty,
  • C. Andreoiu,
  • C. Costache,
  • M.-C. Delattre,
  • A. Etilé,
  • S. Franchoo,
  • C. Gaulard,
  • J. Guillot,
  • F. Ibrahim,
  • M. Lebois,
  • M. MacCormick,
  • N. Marginean,
  • R. Marginean,
  • M. Martini,
  • C. Mihai,
  • I. Mitu,
  • L. Olivier,
  • C. Portail,
  • L. Qi,
  • B. Roussière,
  • L. Stan,
  • D. Testov,
  • J. Wilson,
  • D.T. Yordanov

DOI
https://doi.org/10.1016/j.physletb.2017.06.050
Journal volume & issue
Vol. 772, no. C
pp. 359 – 362

Abstract

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The N=52 Ga83 β decay was studied at ALTO. The radioactive 83Ga beam was produced through the ISOL photofission technique and collected on a movable tape for the measurement of γ-ray emission following β decay. While β-delayed neutron emission has been measured to be 56–85% of the decay path, in this experiment an unexpected high-energy 5–9 MeV γ-ray yield of 16(4)% was observed, coming from states several MeVs above the neutron separation threshold. This result is compared with cutting-edge QRPA calculations, which show that when neutrons deeply bound in the core of the nucleus decay into protons via a Gamow–Teller transition, they give rise to a dipolar oscillation of nuclear matter in the nucleus. This leads to large electromagnetic transition probabilities which can compete with neutron emission, thus affecting the β-decay path. This process is enhanced by an excess of neutrons on the nuclear surface and may thus be a common feature for very neutron-rich isotopes, challenging the present understanding of decay properties of exotic nuclei.