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Liu, R.*; Yan, S.*; Nishio, Katsuhisa; Makii, Hiroyuki; Orlandi, R.; 17 of others*
Chinese Physics C, 50(9), p.094004_1 - 094004_6, 2026/09
Times Cited Count:0 Percentile:0.00(Physics, Nuclear)
Mn
O
Revealed by Micro-focused Angle-resolved Photoemission Spectroscopy and Tight-binding ModelsSawata, Yasutaka*; Shibata, Goro; Saito, Tomohiko*; 7 of others*
Journal of the Physical Society of Japan, 95(8), p.084703_1 - 084703_7, 2026/08
Times Cited Count:0 Percentile:0.00(Physics, Multidisciplinary)Cullings, H. M.*; Funamoto, Sachiyo*; Sato, Tatsuhiko; Endo, Akira; 7 of others*
Medical Research Archives, 14(7), 21 Pages, 2026/08
Lerendegui-Marco, J.*; Balibrea-Correa, J.*; Babiano-Suarez, V.*; Domingo-Pardo, C.*; Rovira Leveroni, G.; 147 of others*
Galaxies (Internet), 14(3), p.59_1 - 59_26, 2026/07
Neutron capture reactions provide essential nuclear physics input for modeling the synthesis of heavy elements in stars. The growing precision of stellar spectroscopy and isotopic measurements in presolar SiC grains now demands cross sections with improved accuracy over the full energy range, and access to unstable nuclei relevant to slow (s-) process branchings and the intermediate (i-) process. This article reviews recent progress in direct neutron capture measurements, focusing on time-of-flight (TOF) experiments at CERN n
TOF and complementary activation techniques. Substantial advances have been achieved for stable s-only and bottleneck isotopes, significantly improving constraints on s-process models.
Ar and the shell closures at
and 
Begala, M.*; Elekes, Z.*; Utsuno, Yutaka; 77 of others*
Journal of Physics G; Nuclear and Particle Physics, 53(7), p.075104_1 - 075104_9, 2026/07
Times Cited Count:0 Percentile:0.00(Physics, Nuclear)no abstracts in English
S and
SBegala, M.*; Elekes, Z.*; Utsuno, Yutaka; 75 of others*
Physical Review C, 113(6), p.064312_1 - 064312_9, 2026/06
Times Cited Count:0 Percentile:0.00(Physics, Nuclear)no abstracts in English
Noda, Yohei*; Kumada, Takayuki; 7 of others*
Journal of Applied Crystallography, 59(2), p.492 - 512, 2026/04
Times Cited Count:0 Percentile:0.00(Chemistry, Multidisciplinary)Choung, S.*; Matsumura, Daiju; 17 of others*
Nature Communications (Internet), 17(1), p.5868_1 - 5868_17, 2026/04
Times Cited Count:0 Percentile:0.00(Multidisciplinary Sciences)
-ray halo beyond 100 TeVAmenomori, Michihiro*; Takita, Masato*; Tsuchiya, Harufumi; Tibet AS
Collaboration*; 78 of others*
Science Advances (Internet), 12(10), p.eadv8173_1 - eadv8173_6, 2026/03
Times Cited Count:0 Percentile:0.00(Multidisciplinary Sciences)Garnaud, L.*; Ogawa, Tatsuhiko; 7 of others*
EPJ Nuclear Sciences & Technologies (Internet), 12, p.5_1 - 5_115, 2026/01
Photoneutrons, produced by photonuclear reactions, appear in diverse applications using high-energy gamma sources, electron accelerators, or nuclear reactors. Monte Carlo particle-transport codes typically simulate their emission, characterize their fields, and evaluate their impact on nuclear systems. This work aims to compile a compendium on photoneutron simulation using MCNP6, PHITS, and TRIPOLI-4. Each code runs with both ENDF/B-VIII.0 and JENDL-5 nuclear data libraries. We investigate photoneutron fields from 50 naturally isotopic elements, ranging from reaction energy threshold up to 30 MeV (the Giant Dipole Resonance regime). These fields are characterized by photoneutron current, energy spectrum, and angular distribution. This paper details results for the initial five elements: deuterium, beryllium, carbon, nitrogen, and oxygen, ordered by increasing atomic number. This compendium will serve as a valuable resource for users to understand code capabilities and limitations, for developers to improve neutron-emitting photonuclear reaction sampling, and for all photoneutron researchers, including nuclear data evaluators and experimental physicists.
Sakai, Hideaki*; Kimata, Motoi; 7 of others*
Nature Communications (Internet), 16, p.11112_1 - 11112_8, 2026/01
Times Cited Count:0 Percentile:0.00(Multidisciplinary Sciences)K
nstle, K.*; Yamamoto, Kei; 7 of others*
Nature Communications (Internet), 16, p.10116_1 - 10116_8, 2025/11
Times Cited Count:13 Percentile:88.83(Multidisciplinary Sciences)
/
for the 19.40-MeV state in
Be for studying the
Be(
,
)
Li
reaction relevant to the cosmological lithium problemIwasa, Naohito*; Nishio, Katsuhisa; Hirose, Kentaro; Makii, Hiroyuki; Orlandi, R.; Suzaki, Fumi; Smallcombe, J.; 7 of others*
Physical Review C, 112(3), p.035801_1 - 035801_6, 2025/09
Times Cited Count:2 Percentile:62.61(Physics, Nuclear)
Sb
Liu, S.*; Kimata, Motoi; Shibauchi, Takasada*; Hashimoto, Kenichiro*; 7 of others*
Physical Review Letters, 135(5), p.056502_1 - 056502_7, 2025/08
Times Cited Count:4 Percentile:64.60(Physics, Multidisciplinary)Horiuchi, Hiroto*; Araki, Yasufumi; Wakabayashi, Yuki*; Ieda, Junichi; Yamanouchi, Michihiko*; 7 of others*
Advanced Materials, 37(26), p.2416091_1 - 2416091_9, 2025/07
Times Cited Count:11 Percentile:86.24(Chemistry, Multidisciplinary)Wang, Y.*; Gong, W.; Harjo, S.; 7 of others*
Acta Materialia, 288, p.120840_1 - 120840_14, 2025/04
Times Cited Count:47 Percentile:99.32(Materials Science, Multidisciplinary)Sanfilippo, A.*; Abe, Noriaki; 27 of others*
Nature Communications (Internet), 16, p.2016_1 - 2016_11, 2025/02
Times Cited Count:15 Percentile:96.39(Multidisciplinary Sciences)Marzec, E.*; Dodo, Taku; Haga, Katsuhiro; Harada, Masahide; Hasegawa, Shoichi; Kasugai, Yoshimi; Kinoshita, Hidetaka; Masuda, Shiho; Meigo, Shinichiro; Sakai, Kenji; et al.
Physical Review Letters, 134(8), p.081801_1 - 081801_9, 2025/02
Times Cited Count:9 Percentile:90.65(Physics, Multidisciplinary)
GeTe
nanomeshesObata, Reiji*; Kikkawa, Takashi*; Saito, Eiji; 7 of others*
Nanotechnology, 35(47), p.475601_1 - 475601_9, 2024/11
Times Cited Count:4 Percentile:28.31(Nanoscience & Nanotechnology)Ozawa, Takahiro*; Fukutani, Katsuyuki; 7 of others*
Nature Communications (Internet), 15, p.9558_1 - 9558_8, 2024/11
Times Cited Count:7 Percentile:42.97(Multidisciplinary Sciences)