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    Exploration for astromers near Sn132 with the Canadian Penning Trap

    A. A. Valverde1,*,†, S. Cupp2,3, A. Gross2,3, B. Liu1,4, M. R. Mumpower5,4,6,3, G. W. Misch7, W. S. Porter4, D. Ray1,8,‡, M. Brodeur4 et al.

    D. P. Burdette1, N. Callahan1, A. Cannon4,§, J. A. Clark1, A. T. Gallant9, D. E. M. Hoff9, A. M. Houff1,4, K. Kolos9, F. G. Kondev1, O. S. Kubiniec1, A. LaLiberte1,10, G. E. Morgan1,11,∥, R. Orford12, C. Quick4,¶, F. Rivero4, D. Santiago-Gonzalez1, G. Savard1,10, N. D. Scielzo9, K. S. Sharma8, and L. Varriano1,10,**

    • *Contact author: avalverde@ikp.tu-darmstadt.de
    • †Present Address: Institut für Kernphysik, TU Darmstadt, 64289 Darmstadt, Germany.
    • ‡Present address: TRIUMF, Vancouver, British Columbia, Canada V6T 2A3.
    • §Present address: TRIUMF, Vancouver, British Columbia, Canada V6T 2A3; Department of Physics and Astronomy, University of Victoria, Victoria, British Columbia, Canada V8W 3P6.
    • ∥Present address: Cyclotron Institute, Texas A&M University, College Station, TX 77843, USA.
    • Present address: Department of Physics and Astronomy, University of Tennessee, Knoxville, TN 37996, USA.
    • **Present address: Center for Experimental Nuclear Physics and Astrophysics, University of Washington, Seattle, WA 98195, USA.

    Phys. Rev. C 113, 065803 – Published 11 June, 2026

    DOI: https://doi.org/10.1103/p2lt-gchf

    Abstract

    Nuclear isomers can have significant impacts on astrophysical nucleosynthesis processes, with recent efforts demonstrating that the population of isomeric states with different half-lives may require separate treatment in reaction networks to accurately capture the differences in heating or in identifiable electromagnetic signals. Several potential so-called “astromers” in tin and antimony isotopes near doubly magic Sn132 were identified and direct mass measurements of their ground and isomeric states were performed with the Canadian Penning Trap at Argonne National Laboratory's CARIBU facility, and their impact on astrophysical reaction rates and in reaction networks was calculated. It was found that Sn129g,m, with measured mass excesses of −80593.2(25) and −80557.4(25) keV, respectively, and an excitation energy of 35.8(35) keV, behaves as an astromer during neutron capture in the i-process and in the r-process.

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