1. Time-Reversal Measurement of the p -Wave Cross Sections of the Be7(n,α)He4 Reaction for the Cosmological Li Problem
- Author
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M. Murata, Tatsuya Morimoto, Kazuya Watanabe, A. Sakaue, D Takechi, Shin-Ichiro Nishimura, Yoshiko Kanada-En'yo, T. Nanamura, K Mizutani, T Goto, Shigeru Kubono, A. Koshikawa, I Sakata, Takeo Kawabata, E Miyawaki, Masatoshi Itoh, T. Takeda, Yutaka Takahashi, M Mizuno, C Takimoto, Takeji Hashimoto, Ryo Sawada, Y Sakaguchi, M. Tsumura, Yuki Shikata, Shuhei Yoshida, Shintaro Okamoto, Naohito Iwasa, Yuki Fujikawa, M. Ichikawa, and Tatsuya Furuno
- Subjects
Physics ,010308 nuclear & particles physics ,P wave ,General Physics and Astronomy ,chemistry.chemical_element ,Nuclear data ,Detailed balance ,Neutron radiation ,01 natural sciences ,Nuclear physics ,Reaction rate ,chemistry ,Nucleosynthesis ,Quantum mechanics ,0103 physical sciences ,Neutron ,Lithium ,Nuclear Experiment ,010303 astronomy & astrophysics - Abstract
The cross sections of the $^{7}\mathrm{Be}(n,\ensuremath{\alpha})^{4}\mathrm{He}$ reaction for $p$-wave neutrons were experimentally determined at ${E}_{\mathrm{c}.\mathrm{m}.}=0.20--0.81\text{ }\text{ }\mathrm{MeV}$ slightly above the big bang nucleosynthesis (BBN) energy window for the first time on the basis of the detailed balance principle by measuring the time-reverse reaction. The obtained cross sections are much larger than the cross sections for $s$-wave neutrons inferred from the recent measurement at the n_TOF facility in CERN, but significantly smaller than the theoretical estimation widely used in the BBN calculations. The present results suggest the $^{7}\mathrm{Be}(n,\ensuremath{\alpha})^{4}\mathrm{He}$ reaction rate is not large enough to solve the cosmological lithium problem, and this conclusion agrees with the recent result from the direct measurement of the $s$-wave cross sections using a low-energy neutron beam and the evaluated nuclear data library ENDF/B-VII.1.
- Published
- 2017