Ab initio calculations of anomalous seniority breaking in the πg9/2 shell for the N = 50 isotones

Q. Yuan, B. S. Hu

Research output: Contribution to journalArticlepeer-review

Abstract

We performed ab initio valence-space in-medium similarity renormalization group (VS-IMSRG) calculations based on chiral two-nucleon and three-nucleon interactions to investigate the anomalous seniority breaking in the neutron number N=50 isotones: 92Mo, 94Ru, 96Pd, and 98Cd. Our calculations well reproduced the measured low-lying spectra and electromagnetic E2 transitions in these nuclei, supporting partial seniority conservation in the first πg9/2 shell. Recent experiments have revealed that, compared to the symmetric patterns predicted under the conserved seniority symmetry, the 41+→21+ E2 transition strength in 94Ru is significantly enhanced and that in 96Pd is suppressed. In contrast, the 61+→41+ and 81+→61+ transitions exhibit the opposite trend. We found that this anomalous asymmetry is sensitive to subtle seniority breaking effects, providing a stringent test for state-of-the-art nucleon-nucleon interactions and nuclear models. We analyzed the anomalous asymmetry using VS-IMSRG calculations across various valence spaces. Our ab initio results suggest that core excitations of both proton and neutron across the Z=50 shell are ascribed to the observed anomalous seniority breaking in the N=50 isotones.

Original languageEnglish
Article number139018
JournalPhysics Letters B
Volume858
DOIs
StatePublished - Nov 2024

Funding

This manuscript has been authored by UT-Battelle, LLC, under contract DE-AC05-00OR22725 with the US Department of Energy (DOE). The US government retains and the publisher, by accepting the article for publication, acknowledges that the US government retains a nonexclusive, paid-up, irrevocable, worldwide license to publish or reproduce the published form of this manuscript, or allow others to do so, for US government purposes. DOE will provide public access to these results of federally sponsored research in accordance with the DOE Public Access Plan (http://energy.gov/downloads/doe-public-access-plan).We thank Takayuki Miyagi for the NuHamil code [65] used to generate matrix elements of the chiral three-body interaction, and Ragnar Stroberg for the imsrg++ code [66] used to perform VS-IMSRG decoupling. This work has been supported by the National Key R&D Program of China under Grant No. 2023YFA1606403; the National Natural Science Foundation of China under Grant Nos. 12205340, 12347106, and 12121005; the Gansu Natural Science Foundation under Grant No. 22JR5RA123 and 23JRRA614; the Key Research Program of the Chinese Academy of Sciences under Grant No. XDPB15; the State Key Laboratory of Nuclear Physics and Technology, Peking University under Grant No. NPT2020KFY13; and the U.S. Department of Energy (DOE), Office of Science, under SciDAC-5 (NUCLEI collaboration) and Contract No. DE-AC05-00OR22725. The numerical calculations in this paper have been done on Hefei advanced computing center. This manuscript has been authored by UT-Battelle, LLC, under contract DE-AC05-00OR22725 with the US Department of Energy (DOE). The US government retains and the publisher, by accepting the article for publication, acknowledges that the US government retains a nonexclusive, paid-up, irrevocable, worldwide license to publish or reproduce the published form of this manuscript, or allow others to do so, for US government purposes. DOE will provide public access to these results of federally sponsored research in accordance with the DOE Public Access Plan ( http://energy.gov/downloads/doe-public-access-plan ). We thank Takayuki Miyagi for the NuHamil code [65] used to generate matrix elements of the chiral three-body interaction, and Ragnar Stroberg for the imsrg++ code [66] used to perform VS-IMSRG decoupling. This work has been supported by the National Key R&D Program of China under Grant No. 2023YFA1606403; the National Natural Science Foundation of China under Grant Nos. 12205340, 12347106, and 12121005; the Gansu Natural Science Foundation under Grant No. 22JR5RA123 and 23JRRA614; the Key Research Program of the Chinese Academy of Sciences under Grant No. XDPB15; the State Key Laboratory of Nuclear Physics and Technology, Peking University under Grant No. NPT2020KFY13; and the U.S. Department of Energy (DOE), Office of Science, under SciDAC-5 (NUCLEI collaboration). The numerical calculations in this paper have been done on Hefei advanced computing center.

FundersFunder number
DOE Public Access Plan
U.S. Department of Energy
State Key Laboratory of Nuclear Physics and Technology, Peking UniversityNPT2020KFY13
Office of ScienceSciDAC-5
Chinese Academy of SciencesXDPB15
National Natural Science Foundation of China12121005, 12205340, 12347106
National Key Research and Development Program of China2023YFA1606403
Natural Science Foundation of Gansu Province23JRRA614, 22JR5RA123

    Keywords

    • Ab initio
    • Chiral nuclear force
    • Cross-shell excitations
    • N=50 isotones
    • Seniority breaking

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