期刊
PHYSICAL REVIEW LETTERS
卷 129, 期 18, 页码 -出版社
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevLett.129.172701
关键词
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资金
- JSPS KAKENHI [14F04808, 17H06090, 19H00693, 20H05648, 21H01087, 22H04946, 25247045, 19340074]
- RIKEN program for Evolution of Matter in the Universe (r-EMU)
- National Science Foundation [PHY-1430152, PHY-1565546, PHY-1714153]
- Spanish Ministerio de Economa y Competitividad [IJCI-2014-19172, FPA2014-52823-C2-1-P, FPA2014-52823-C2-2-P, FPA2017-83946-C2-1-P, FPA2017-83946-C2-2-P]
- Ministerio de Ciencia e Innovacion [PID2019-104714GB-C21, PID2019-104714GB-C22]
- European Regional Development Fund
- Generalitat Valenciana [PROMETEO/2019/007]
- Office of Nuclear Physics, U.S. Department of Energy [DE-FG02-96ER40983, DE-AC05-00OR22725]
- National Nuclear Security Administration
- DOE [DE-NA0002132]
- United Kingdom Science and Technology Facilities Council [ST/N00244X/1, ST/P004598/1, ST/V001027/1]
- National Nuclear Security Administration of the U.S. Department of Energy at Los Alamos National Laboratory [89233218CNA000001]
- Polish National Science Center [2020/36/T/ST2/00547, 2019/33/N/ST2/03023]
- NKFIH [NN128072]
- JSPS Invitational Fellowships for Research in Japan [L1955]
- RIKEN intensive Research Program
- Long-term International Program Associate
- Canadian Natural Sciences and Engineering Research Council (NSERC)
- Foundation for Polish Science (FNP)
- Institute for Basic Science of the Republic of Korea [IBS-R031-Y1, IBS-R031-D1]
The beta-delayed one- and two-neutron emission probabilities of neutron-rich nuclei with N >= 82 were measured at the RIKEN Nishina Center. The results provide important benchmarks for macroscopic-microscopic and self-consistent global models, and have significant implications for r-process nucleosynthesis.
The beta-delayed one- and two-neutron emission probabilities (P-1n and P-2n) of 20 neutron-rich nuclei with N >= 82 have been measured at the RIBF facility of the RIKEN Nishina Center. P-1n of Ag-130;131, Cd-133;134, In-135;136, and (138;13)9Sn were determined for the first time, and stringent upper limits were placed on P-2n for nearly all cases. beta-delayed two-neutron emission (beta 2n) was unambiguously identified in Cd-133 and In-135;136, and their P-2n were measured. Weak beta 2n was also detected from Sn-137;138. Our results highlight the effect of the N = 82 and Z = 50 shell closures on beta-delayed neutron emission probability and provide stringent benchmarks for newly developed macroscopic-microscopic and self-consistent global models with the inclusion of a statistical treatment of neutron and. emission. The impact of our measurements on r-process nucleosynthesis was studied in a neutron star merger scenario. Our P-1n and P-2n have a direct impact on the
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