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Schnabel, G.*; Kunieda, Satoshi; Konno, Chikara; Nakayama, Shinsuke; 27 of others*
Nuclear Data Sheets, 193, p.1 - 78, 2024/02
Fusion Evaluated Nuclear Data Library (FENDL), which has been coordinated by International Atomic Energy Agency (IAEA), was updated for the neutronics analysis on the fusion reactors and related applications. The main sources of data files are the national nuclear data libraries such as ENDF, JEFF and JENDL, where the best data was selected for each isotope through comparisons of the evaluated cross-sections and a number of benchmark analyses. Large differences from the previous library (FENDL-2.1) are extension of the upper energy limit from 20 MeV to 200 MeV and inclusion of the charged-particle reaction data, which had been requested by accelerator-based studies on structural materials for the fusion reactors. This paper gives a comprehensive description on the latest version FENDL-3.2b. A number of validations on the neutronics analysis show that the performance of FENDL-3.2b is better than FENDL-2.1.
Sano, Tomokazu*; Matsuda, Tomoki*; Hirose, Akio*; Terai, Tomoyuki*; Kakeshita, Tomoyuki*; Inubushi, Yuichi*; Sato, Takahiro*; Yabashi, Makina*; Shobu, Takahisa; 22 of others*
Scientific Reports (Internet), 13, p.13796_1 - 13796_10, 2023/08
Times Cited Count:0 Percentile:0(Multidisciplinary Sciences)Muramatsu, Norihito*; Tsuchikawa, Yusuke; LEPS2 BGOegg Collaboration*; 61 of others*
Physical Review C, 107(4), p.L042201_1 - L042201_5, 2023/04
Times Cited Count:0 Percentile:0.02(Physics, Nuclear)Nakamura, Tomoki*; Osawa, Takahito; 219 of others*
Science, 379(6634), p.eabn8671_1 - eabn8671_14, 2023/02
Times Cited Count:98 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 HO 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.
Fujita, Manami; Hasegawa, Shoichi; Hosomi, Kenji; Ichikawa, Masaya; Ichikawa, Yudai; Kim, S.; Nanamura, Takuya; Sako, Hiroyuki; Tamura, Hirokazu; Yamamoto, Takeshi; et al.
Progress of Theoretical and Experimental Physics (Internet), 2022(12), p.123D01_1 - 123D01_17, 2022/12
Times Cited Count:0 Percentile:0.01(Physics, Multidisciplinary)Gerst, R.-B.*; Blazhev, A.*; Moschner, K.*; Doornenbal, P.*; Obertelli, A.*; Orlandi, R.; 62 of others*
Physical Review C, 105(2), p.024302_1 - 024302_11, 2022/02
Times Cited Count:6 Percentile:82.52(Physics, Nuclear)Nagatsuka, Naoki*; Fukutani, Katsuyuki; 2 of others*
Physical Review B, 105(4), p.045424_1 - 045424_6, 2022/01
Times Cited Count:3 Percentile:48.5(Materials Science, Multidisciplinary)van Tonder, R.*; Tanida, Kiyoshi; Belle Collaboration*; 202 of others*
Physical Review D, 104(11), p.112011_1 - 112011_32, 2021/12
Times Cited Count:10 Percentile:65.5(Astronomy & Astrophysics)Yakushev, A.*; Lens, L.*; Dllmann, C. E.*; Block, M.*; Nagame, Yuichiro*; Sato, Tetsuya; Toyoshima, Atsushi*; 42 of others*
Frontiers in Chemistry (Internet), 9, p.753738_1 - 753738_9, 2021/11
Times Cited Count:10 Percentile:63.67(Chemistry, Multidisciplinary)Nihonium (Nh, element 113) and flerovium (Fl, element 114) are the first superheavy elements in which the 7p shell is occupied. High volatility and inertness were predicted for Fl due to the strong relativistic stabilization of the closed 7p sub-shell, which originates from a large spin-orbit splitting between the 7p and 7p orbitals. One unpaired electron in the outermost 7p sub-shell in Nh is expected to give rise to a higher chemical reactivity. Theoretical predictions of Nh reactivity are discussed, along with results of the first experimental attempts to study Nh chemistry in the gas phase. The experimental observations verify a higher chemical reactivity of Nh atoms compared to its neighbor Fl and call for the development of advanced setups. First tests of a newly developed detection device miniCOMPACT with highly reactive Fr isotopes assure that effective chemical studies of Nh are within reach.
Andel, B.*; Van Duppen, P.*; Andreyev, A. N.; Blazhev, A.*; Grawe, H.*; Lica, R.*; Nadja, H.*; Stryjczyk, M.*; 52 of others*
Physical Review C, 104(5), p.054301_1 - 054301_13, 2021/11
Times Cited Count:1 Percentile:18.91(Physics, Nuclear)Atmacan, H.*; Tanida, Kiyoshi; Belle Collaboration*; 219 of others*
Physical Review D, 104(9), p.L091105_1 - L091105_9, 2021/11
Times Cited Count:3 Percentile:20.63(Astronomy & Astrophysics)Gilbert, M. R.*; Arakawa, Kazuto*; Suzudo, Tomoaki; Tsuru, Tomohito; 26 of others*
Journal of Nuclear Materials, 554, p.153113_1 - 153113_31, 2021/10
Times Cited Count:33 Percentile:90.46(Materials Science, Multidisciplinary)Modelling will continue to do so until the first generation of fusion power plants come on line and allow long-term behaviour to be observed. In the meantime, the modelling is supported by experiments that attempt to replicate some aspects of the eventual operational conditions. In 2019, a group of leading experts met under the umbrella of the IEA to discuss the current position and ongoing challenges in modelling of fusion materials and how advanced experimental characterisation is aiding model improvement. This review draws from the discussions held during that workshop. Topics covering modelling of irradiation-induced defect production and fundamental properties, gas behaviour, clustering and segregation, defect evolution and interactions are discussed, as well as new and novel multiscale simulation approaches, and the latest efforts to link modelling to experiments through advanced observation and characterisation techniques.
Tonev, D.*; De Angelis, G.*; Deloncle, I.*; Orlandi, R.; 27 of others*
Physics Letters B, 821, p.136603_1 - 136603_6, 2021/10
Times Cited Count:5 Percentile:65.12(Astronomy & Astrophysics)Yelton, J.*; Tanida, Kiyoshi; Belle Collaboration*; 205 of others*
Physical Review D, 104(5), p.052003_1 - 052003_8, 2021/09
Times Cited Count:4 Percentile:37.94(Astronomy & Astrophysics)Li, Y. B.*; Tanida, Kiyoshi; Belle Collaboration*; 182 of others*
Physical Review Letters, 127(12), p.121803_1 - 121803_8, 2021/09
Times Cited Count:26 Percentile:91.72(Physics, Multidisciplinary)Harding, R. D.*; Andreyev, A. N.; Barzakh, A. E.*; Cubiss, J. G.*; Van Duppen, P.*; Al Monthery, M.*; Althubiti, N. A.*; Andel, B.*; 26 of others*
Physical Review C, 104(2), p.024326_1 - 024326_16, 2021/08
Times Cited Count:5 Percentile:46.8(Physics, Nuclear)Cao, L.*; Tanida, Kiyoshi; Belle Collaboration*; 236 of others*
Physical Review D, 104(1), p.012008_1 - 012008_32, 2021/07
Times Cited Count:10 Percentile:65.5(Astronomy & Astrophysics)Jia, S.*; Tanida, Kiyoshi; Belle Collaboration*; 200 of others*
Physical Review D, 104(1), p.012012_1 - 012012_9, 2021/07
Times Cited Count:0 Percentile:0.01(Astronomy & Astrophysics)Guan, Y.*; Tanida, Kiyoshi; Belle Collaboration*; 202 of others*
Physical Review D, 103(11), p.112005_1 - 112005_11, 2021/06
Times Cited Count:5 Percentile:45.23(Astronomy & Astrophysics)Moon, T. J.*; Tanida, Kiyoshi; Belle Collaboration*; 203 of others*
Physical Review D, 103(11), p.L111101_1 - L111101_9, 2021/06
Times Cited Count:18 Percentile:85.82(Astronomy & Astrophysics)