Pygmy Gamow-Teller resonance in the N = 50 region: New evidence from staggering of β -delayed neutron-emission probabilities

We report on the β-delayed neutron emission probability (P1n) measurements of the Ga82,83,84 (N=51,52,53) precursors performed in one single experiment using the He3 neutron-counter TETRA at the ALTO facility in Orsay. Altogether our results for the three A=82,83, and 84 Ga precursors point towards...

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Veröffentlicht in:Phys.Rev.C 2017-05, Vol.95 (5), Article 054320
Hauptverfasser: Verney, D., Testov, D., Ibrahim, F., Penionzhkevich, Yu, Roussière, B., Smirnov, V., Didierjean, F., Flanagan, K., Franchoo, S., Kuznetsova, E., Li, R., Marsh, B., Matea, I., Pai, H., Sokol, E., Stefan, I., Suzuki, D.
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Sprache:eng
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Zusammenfassung:We report on the β-delayed neutron emission probability (P1n) measurements of the Ga82,83,84 (N=51,52,53) precursors performed in one single experiment using the He3 neutron-counter TETRA at the ALTO facility in Orsay. Altogether our results for the three A=82,83, and 84 Ga precursors point towards a sizable P1n staggering in the N=50 region, similar to the one already observed just after the N=28 shell closure in the K isotopes chain, hinting at a similar mechanism. We will discuss the possible microscopic origin of this behavior, i.e., the existence in the light N=51 isotones of low-lying components of the so called pygmy Gamow-Teller resonance, already well established at Z=36, and persisting toward Ni79.
ISSN:2469-9985
2469-9993
DOI:10.1103/PhysRevC.95.054320