1. Unexpected high-energy γ emission from decaying exotic nuclei.
- Author
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Gottardo, A., Verney, D., Deloncle, I., Péru, S., Delafosse, C., Roccia, S., Matea, I., Sotty, C., Andreoiu, C., Costache, C., Delattre, M.-C., Etilé, A., Franchoo, S., Gaulard, C., Guillot, J., Ibrahim, F., Lebois, M., MacCormick, M., Marginean, N., and Marginean, R.
- Subjects
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EXOTIC nuclei , *PARTICLE physics , *NUCLEAR energy , *PHOTOFISSION , *NEUTRON emission - Abstract
The N = 52 Ga 83 β decay was studied at ALTO. The radioactive 83 Ga 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. [ABSTRACT FROM AUTHOR]
- Published
- 2017
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