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Broken seniority symmetry in the semimagic proton mid-shell nucleus Rh 95
Lifetime measurements of low-lying excited states in the semimagic ( N = 50 ) nucleus Rh 95 have been performed by means of the fast-timing technique. The experiment was carried out using γ -ray detector arrays consisting of LaBr 3 (Ce) scintillators and germanium detectors integrated into the DESPE...
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Published in: | Physical review research 2024-05, Vol.6 (2), Article L022038 |
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Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
Format: | Article |
Language: | English |
Citations: | Items that this one cites |
Online Access: | Get full text |
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Summary: | Lifetime measurements of low-lying excited states in the semimagic ( N = 50 ) nucleus Rh 95 have been performed by means of the fast-timing technique. The experiment was carried out using γ -ray detector arrays consisting of LaBr 3 (Ce) scintillators and germanium detectors integrated into the DESPEC experimental setup commissioned for the Facility for Antiproton and Ion Research () Phase-0, Darmstadt, Germany. The excited states in Rh 95 were populated primarily via the β decays of Pd 95 nuclei, produced in the projectile fragmentation of a 850 MeV/nucleon Xe 124 beam impinging on a 4 g / cm 2 Be 9 target. The deduced electromagnetic E2 transition strengths for the γ -ray cascade within the multiplet structure depopulating from the isomeric I π = 21 / 2 + state are found to exhibit strong deviations from predictions of standard shell model calculations which feature approximately conserved seniority symmetry. In particular, the observation of a strongly suppressed E2 strength for the 13 / 2 + → 9 / 2 + ground state transition cannot be explained by calculations employing standard interactions. This remarkable result may require revision of the nucleon-nucleon interactions employed in state-of-the-art theoretical model calculations, and might also point to the need for including three-body forces in the Hamiltonian. |
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ISSN: | 2643-1564 2643-1564 |
DOI: | 10.1103/PhysRevResearch.6.L022038 |