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    Microscopic theory of the γ decay of giant resonances in superfluid nuclei

    W.-L. Lv (吕万里)

    Y.-F. Niu (牛一斐)*

    G. Colò

    • School of Physics and Astronomy, Shanghai Jiao Tong University, Key Laboratory for Particle Astrophysics and Cosmology (MoE), Shanghai 200240, China; Shanghai Key Laboratory for Particle Physics and Cosmology, Shanghai 200240, China; Frontiers Science Center for Rare isotopes, Lanzhou University, Lanzhou 730000, China; and School of Nuclear Science and Technology, Lanzhou University, Lanzhou 730000, China

    • *Contact author: niuyf@sjtu.edu.cn

    Phys. Rev. C 114, 034333 – Published 28 September, 2026

    DOI: https://doi.org/10.1103/qlby-yll5

    Abstract

    Recent advances in experiments have enabled the measurement of γ decay from giant and pygmy resonances to low-lying states, establishing this technique as a unique probe for nuclear structure. However, a microscopic description of γ decay to low-lying states in superfluid nuclei is still lacking. We develop the Skyrme quasiparticle vibration (QPVC) model to calculate γ-decay widths between vibrational states. This model treats initial and final states as quasiparticle random-phase-approximation (QRPA) phonons and includes all the second-order diagrams for the interaction between the quasiparticles and the phonons, while consistently accounting for the polarization processes. The same Skyrme functional is employed for the ground state and the interaction vertices. As a timely application, the γ-decay width from the giant dipole resonance (GDR) to the 21+ state in Ce140 is calculated, which has recently been measured at the High Intensity γ-ray Source (HIγS). For the 4 Skyrme functionals we used, the total width of the collective dipole states in GDR region is 250–420 eV and the corresponding branching ratio is 0.87–1.18%. The polarization effect, extracted microscopically, agrees in trend with the macroscopic Bohr-Mottelson formula.

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