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Yoshida, Shuhei*; Gong, W.; 9 of others*
Acta Materialia, 283, p.120498_1 - 120498_15, 2025/01
Times Cited Count:0 Percentile:0.00(Materials Science, Multidisciplinary)Hwang, J.*; Chillery, T.*; Dozono, Masanori*; Imai, Nobuaki*; Michimasa, Shinichiro*; Sumikama, Toshiyuki*; Chiga, Nobuyuki*; Ota, Shinsuke*; Nakayama, Shinsuke; 49 of others*
Progress of Theoretical and Experimental Physics (Internet), 2024(9), p.093D03_1 - 093D03_12, 2024/09
Times Cited Count:0 Percentile:0.00(Physics, Multidisciplinary)Nuclear transmutation emerges as a promising approach for reprocessing high-level waste, specifically treating long-lived nuclides like Zr from spent fuel. It is essential to accumulate reaction data for these nuclei to advance this prominent treatment and to build a comprehensive understanding of reaction mechanisms. In this study, the residual production cross-sections resulting from proton-induced reactions on
Zr were measured at 27 MeV/nucleon in inverse kinematics. At the RIKEN-RIBF facility the OEDO beamline was used to deduce production cross-sections for isotopes,
Nb,
Zr, and
Y. Comparing the results from this study and prior research with calculated excitation functions, a moderate agreement is found with theoretical predictions derived from TALYS and CCONE. Despite the potential limitations of low-energy proton-induced reactions for
Zr transmutation, the measured cross-sections offer valuable insights for future considerations in nuclear-waste treatment facilities. This is particularly relevant for facilities exploring innovative methods, such as accelerator-driven systems.
Kawamoto, Yo*; Kikkawa, Takashi; Saito, Eiji; 9 of others*
Applied Physics Letters, 124(13), p.132406_1 - 132406_7, 2024/03
Times Cited Count:3 Percentile:88.42(Physics, Applied)Zhou, X.*; Fukutani, Katsuyuki; 9 of others*
Applied Physics Letters, 124(8), p.082103_1 - 082103_7, 2024/02
Times Cited Count:6 Percentile:92.44(Physics, Applied)Chillery, T.*; Hwang, J.*; Dozono, Masanori*; Imai, Nobuaki*; Michimasa, Shinichiro*; Sumikama, Toshiyuki*; Chiga, Nobuyuki*; Ota, Shinsuke*; Nakayama, Shinsuke; 49 of others*
Progress of Theoretical and Experimental Physics (Internet), 2023(12), p.121D01_1 - 121D01_11, 2023/12
Times Cited Count:2 Percentile:48.32(Physics, Multidisciplinary)The deuteron is a loosely bound system which can easily break up into its constituent proton and neutron whilst in the presence of Coulomb and nuclear fields. Previous experimental studies have shown that this breakup process has a significant impact on residual nucleus production from deuteron bombardment in the high energy range of 50 - 210 MeV/nucleon. However, there remains a lack of cross-section data at energies below 50 MeV/nucleon. The current study determined Zr + d reaction cross sections under inverse kinematics at approximately 28 MeV/nucleon using the BigRIPS separator, OEDO beamline, and SHARAQ spectrometer. Cross sections from this research were compared with previous measurements and theoretical calculations. The experimental results show a large enhancement of the production cross sections of residual nuclei, especially those produced from a small number of particle emissions, compared to the proton-induced reaction data at similar bombarding energy. The DEURACS calculation, which quantitatively takes deuteron-breakup effects into account, reproduces the data well. As a long-lived fission product,
Zr remains a challenge for nuclear waste disposal and treatment. This study's low-energy data may assist future consideration of nuclear-waste treatment facilities, where
Zr + d may feasibly transmute the waste into short-lived/stable nuclei.
Yang, S.*; Tanida, Kiyoshi; Belle Collaboration*; 196 of others*
Physical Review D, 108(3), p.L031104_1 - L031104_6, 2023/08
Times Cited Count:3 Percentile:51.06(Astronomy & Astrophysics)Pedersen, L. G.*; Sahin, E.*; Grgen, A.*; Bello Garrote, F. L.*; Tsunoda, Yusuke*; Otsuka, Takaharu*; Niikura, Megumi*; Orlandi, R.; 59 of others*
Physical Review C, 107(4), p.044301_1 - 044301_10, 2023/04
Times Cited Count:1 Percentile:34.19(Physics, Nuclear)Yin, J. H.*; Tanida, Kiyoshi; Belle Collaboration*; 193 of others*
Physical Review D, 107(5), p.052004_1 - 052004_8, 2023/03
Times Cited Count:3 Percentile:51.06(Astronomy & Astrophysics)Choudhury, S.*; Tanida, Kiyoshi; Belle Collaboration*; 198 of others*
Physical Review D, 107(3), p.L031102_1 - L031102_6, 2023/02
Times Cited Count:8 Percentile:81.35(Astronomy & Astrophysics)Li, L. K.*; Tanida, Kiyoshi; Belle Collaboration*; 197 of others*
Physical Review D, 107(3), p.033003_1 - 033003_9, 2023/02
Times Cited Count:0 Percentile:0.00(Astronomy & Astrophysics)Nakamura, Tomoki*; Osawa, Takahito; 219 of others*
Science, 379(6634), p.eabn8671_1 - eabn8671_14, 2023/02
Times Cited Count:175 Percentile:99.99(Multidisciplinary Sciences)Mineralogical, petrological, and physical properties of sixteen Ryugu particles measuring 1-8 mm indicate that they are most similar to CI chondrites. The presence of CO-bearing water in pyrrhotite indicates that the original parent asteroid formed beyond the H
O and CO
snow lines in the solar nebula, where, based on Ryugu mineralogy, very limited amounts of high-temperature objects including small chondrules and Ca, Al-rich inclusions were present. Fluid-rock reactions occurred at low-temperature, high pH, and reducing conditions at water/rock mass ratios smaller than 1 and changed an olivine-pyroxene rich lithology, remaining as the least-altered fragments in Ryugu samples, into phyllosilicate-carbonate rich lithologies, the predominant material of Ryugu samples. The solar nebula might have been still present when magnetite crystallized from the fluid in Ryugu's parent body.
Krohn, J.-F.*; Tanida, Kiyoshi; Belle Collaboration*; 198 of others*
Physical Review D, 107(1), p.012003_1 - 012003_12, 2023/01
Times Cited Count:1 Percentile:21.72(Astronomy & Astrophysics)Li, Y. B.*; Tanida, Kiyoshi; Belle Collaboration*; 194 of others*
Physical Review Letters, 130(3), p.031901_1 - 031901_7, 2023/01
Times Cited Count:13 Percentile:92.03(Physics, Multidisciplinary)Sakuma, Fuminori*; Tamura, Hirokazu; Tanida, Kiyoshi; Yamamoto, Takeshi; 39 of others*
EPJ Web of Conferences, 271, p.11001_1 - 11001_7, 2022/11
Nanamura, Takuya; Fujita, Manami; Hasegawa, Shoichi; Ichikawa, Masaya; Ichikawa, Yudai; Imai, Kenichi*; Naruki, Megumi; Sato, Susumu; Sako, Hiroyuki; Tamura, Hirokazu; et al.
Progress of Theoretical and Experimental Physics (Internet), 2022(9), p.093D01_1 - 093D01_35, 2022/09
Times Cited Count:15 Percentile:84.99(Physics, Multidisciplinary)Czank, T.*; Tanida, Kiyoshi; Belle Collaboration*; 209 of others*
Physical Review D, 106(1), p.012003_1 - 012003_10, 2022/07
Times Cited Count:8 Percentile:60.51(Astronomy & Astrophysics)Jeon, H. B.*; Tanida, Kiyoshi; Belle Collaboration*; 219 of others*
Physical Review D, 106(1), p.012006_1 - 012006_9, 2022/07
Times Cited Count:0 Percentile:0.00(Astronomy & Astrophysics)Li, S. X.*; Tanida, Kiyoshi; Belle Collaboration*; 197 of others*
Journal of High Energy Physics (Internet), 2022(3), p.90_1 - 90_11, 2022/03
Times Cited Count:8 Percentile:65.00(Physics, Particles & Fields)Venhart, M.*; Andreyev, A. N.; Cubiss, J. G.*; Wood, J. L.*; Barzakh, A. E.*; Van Beveren, C.*; Cocolios, T. E.*; de Groote, R. P.*; 19 of others*
Physical Review C, 105(3), p.034338_1 - 034338_9, 2022/03
Times Cited Count:2 Percentile:36.77(Physics, Nuclear)Abudinn, F.*; Tanida, Kiyoshi; Belle II Collaboration*; 319 of others*
Journal of High Energy Physics (Internet), 2022(2), p.63_1 - 63_33, 2022/02
Times Cited Count:4 Percentile:42.30(Physics, Particles & Fields)