Measurements of Gamow-Teller transitions from 59Co via the 59Co (𝑡, 3He +𝛾) charge-exchange reaction and its application to the stellar electron-capture rates
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- Chinese Academy of Sciences, Lanzhou (China); University of Chinese Academy of Sciences, Beijing (China)
- Michigan State University, East Lansing, MI (United States)
- Shanghai Jiao Tong University (China)
- Southwest University, Chongqing (China)
- Lanzhou University (China); China Institute of Atomic Energy, Beijing (China); Chinese Academy of Sciences, Lanzhou (China)
- Chinese Academy of Sciences, Lanzhou (China)
Electron-capture reactions on iron-group nuclei play a crucial role in the late stages of massive star evolution. Since stellar evolution simulations depend on accurate electron-capture rates—which are highly sensitive to the detailed Gamow-Teller (GT) strength distributions—reliable theoretical models are essential. However, experimental data on GT strength distributions are scarce. High-resolution measurements are therefore vital for benchmarking and improving these theoretical calculations. To provide high-resolution data on Gamow-Teller strength distributions of iron-group nuclei and to compare these results with theoretical calculations within this mass region. Differential cross sections for the 59Co (𝑡, 3He) 59Fe charge-exchange reaction at 115 MeV/u were measured using the S800 spectrometer. Furthermore, to resolve individual levels that are not distinguishable in the S800 particle singles data, coincident 𝛾 rays from the 59Fe residual nucleus were detected by using the Gamma-Ray Energy Tracking In-beam Nuclear Array 𝛾-ray tracking array. Here, the Gamow-Teller transition strength distribution from the ground state of 59Co to 59Fe was extracted up to an excitation energy of 10 MeV. Additionally, transition strengths for several low-lying states were determined from coincident 𝛾-ray measurements. Electron-capture rates calculated using the present data indicate that these low-lying states contribute significantly to the overall rates in relevant stellar environments. The experimental results show reasonable agreement with theoretical predictions based on both shell-model and projected shell-model calculations. High-resolution data on Gamow-Teller strength distributions—particularly for individual low-lying states—are essential for accurately determining electron-capture rates in iron-group nuclei. Coincident 𝛾-ray measurements provide a powerful tool for obtaining such detailed information. While the present work demonstrates that shell-model calculations successfully reproduce the experimental results, such comparisons are scarce and more experimental data are desirable.
- Research Organization:
- Michigan State University, East Lansing, MI (United States)
- Sponsoring Organization:
- National Natural Science Foundation of China; National Science Foundation (NSF); USDOE National Nuclear Security Administration (NNSA); USDOE Office of Science (SC), Nuclear Physics (NP)
- Grant/Contract Number:
- AC02-05CH11231; NA0003180; SC0019034; SC0020451; SC0023633
- OSTI ID:
- 3001912
- Alternate ID(s):
- OSTI ID: 2584538
- Journal Information:
- Physical Review. C, Journal Name: Physical Review. C Journal Issue: 2 Vol. 112; ISSN 2469-9985; ISSN 2469-9993
- Publisher:
- American Physical Society (APS)Copyright Statement
- Country of Publication:
- United States
- Language:
- English
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