Export citation

Export citation

Choose format for download:

Download Citation

    Precision Mass Measurements around Mo84 Rule Out ZrNb Cycle Formation in the Rapid Proton-Capture Process at Type I X-Ray Bursts

    S. Kimura1,*, M. Wada1,†, C. Y. Fu2,3, N. Fukuda2, Y. Hirayama1, D. S. Hou1,3, S. Iimura2,4, H. Ishiyama2, Y. Ito5,‡ et al.

    S. Kubono2,6, K. Kusaka2, S. Michimasa2, H. Miyatake1, S. Nishimura2, T. Niwase7, V. Phong2, M. Rosenbusch2, H. Schatz8, P. Schury1, Y. Shimizu2, H. Suzuki2, A. Takamine2,7, H. Takeda2, Y. Togano2, Y. X. Watanabe1, W. D. Xian1,3, Y. Yanagisawa2, T. T. Yeung2,9, M. Yoshimoto2, and S. Zha2,3

    • *Contact author: sota.kimura@kek.jp
    • †Present address: Institute of Modern Physics, Huizhou branch, Chinese Academy of Science, Huizhou 516000, China.
    • ‡Present address: Wako Nuclear Science Center, Institute of Particle and Nuclear Studies, High Energy Accelerator Research Organization, Wako 351-0198, Japan.

    Phys. Rev. Lett. 135, 152701 – Published 8 October, 2025

    DOI: https://doi.org/10.1103/2dyn-q7wp

    Abstract

    The rapid proton-capture process is one of the primary, explosive thermonuclear burning processes that drive type I x-ray bursts. A possible termination of the rapid proton-capture process at around Mo84 was previously suggested by the formation of a ZrNb cycle. We report here precision mass measurements at around Mo84 that conclude the issue regarding the possibility of the cycle. The experiment was conducted using the multireflection time-of-flight spectrograph at RIKEN Radioactive Isotope Beam Factory, and the masses of Y79, Nb83, Mo84, Ru88, and an isomer in Y78 were measured. For Mo84, Ru88, and the isomeric state of Y78, their masses were experimentally determined for the first time with uncertainties of δm≈20  keV/c2. The mass precisions of Y79 and Nb83 were improved to 13 and 9.6  keV/c2, respectively. The new α-separation energy of Mo84, 1.434(83) MeV, unambiguously rules out the possibility of forming the ZrNb cycle. The x-ray burst simulation with the new masses shows that our measurements effectively remove the large final abundance uncertainties in the A=80–90 mass region. The new mass values improve the prediction power for the composition of the nuclear ashes in x-ray bursts.

    Physics Subject Headings (PhySH)

    Authorization Required

    We need you to provide your credentials before accessing this content.

    References (Subscription Required)

    Outline

    Information

    Sign In to Your Journals Account

    Filter

    Filter

    Article Lookup

    Enter a citation