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Investigation of J-1 anomaly and nuclear states in odd-A silver isotopes using the interacting boson–fermion model implies astrophysical significance.
The structure of the odd-A silver isotopes Ag103–115 is discussed within the frame of the interacting boson–fermion model (IBFM). An overview of their key properties is presented, with a particular attention paid to the “J-1 anomaly”, represented by an abnormal ordering of the lowest 7/2+ and 9/2+ states. By examining previously published data and newly performed calculations, it is demonstrated that the experimentally known level schemes and electromagnetic properties of Ag103–115 can be reproduced well within IBFM-1 by using a consistent set of model parameters. The contribution of different single-particle orbitals to the structure of the lowest-lying excited nuclear states in Ag103–115 is discussed. Given that the J-1 anomaly brings down the 7/2+ level from the j−3 multiplet to energies, which can be thermally populated in hot stellar environments, the importance of low-lying excited states in odd-A silver isotopes for astrophysical processes is outlined.
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Kisyov et al. (2025) studied this question.
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