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Mastromarco, M.*; Amaducci, S.*; Colonna, N.*; Kimura, Atsushi; 118 of others*
European Physical Journal A, 58(8), p.147_1 - 147_13, 2022/08
Times Cited Count:2 Percentile:49.92(Physics, Nuclear)Kovalenko, E.*; Tanida, Kiyoshi; Belle Collaboration*; 181 of others*
Physical Review D, 104(11), p.112006_1 - 112006_12, 2021/12
Times Cited Count:0 Percentile:0.01(Astronomy & Astrophysics)Uno, Kenta*; Tanida, Kiyoshi; Belle Collaboration*; 181 of others*
Journal of High Energy Physics (Internet), 2021(10), p.19_1 - 19_12, 2021/10
Times Cited Count:11 Percentile:63.98(Physics, Particles & Fields)Fittipaldi, R.*; Hartmann, R.*; Mercaldo, M. T.*; Komori, Sachio*; Bjrlig, A.*; Higemoto, Wataru; Maeno, Yoshiteru*; Di Bernardo, A.*; 18 of others*
Nature Communications (Internet), 12, p.5792_1 - 5792_9, 2021/10
Times Cited Count:11 Percentile:68.91(Multidisciplinary Sciences)The layered oxide perovskite SrRuO, which has been intensively investigated due to its unusual properties. Whilst the debate on the symmetry of the superconducting state in SrRuO is still ongoing, a deeper understanding of the SrRuO normal state appears crucial as this is the background in which electron pairing occurs. Here, by using low-energy muon spin spectroscopy we discover the existence of surface magnetism in SrRuO at an onset temperature higher than 50 K. Our observations set a reference for the discovery of the same magnetic phase in other materials.
Li, L. K.*; Tanida, Kiyoshi; Belle Collaboration*; 187 of others*
Journal of High Energy Physics (Internet), 2021(9), p.75_1 - 75_21, 2021/09
Times Cited Count:1 Percentile:10.04(Physics, Particles & Fields)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:27 Percentile:92.21(Physics, Multidisciplinary)Jia, S.*; Tanida, Kiyoshi; Belle Collaboration*; 186 of others*
Journal of High Energy Physics (Internet), 2021(6), p.160_1 - 160_13, 2021/06
Times Cited Count:5 Percentile:36.61(Physics, Particles & Fields)Mizuk, R.*; Tanida, Kiyoshi; Belle Collaboration*; 188 of others*
Journal of High Energy Physics (Internet), 2021(6), p.137_1 - 137_35, 2021/06
Times Cited Count:7 Percentile:50.25(Physics, Particles & Fields)Mohanty, S.*; Tanida, Kiyoshi; Belle Collaboration*; 184 of others*
Physical Review D, 103(5), p.052013_1 - 052013_9, 2021/03
Times Cited Count:0 Percentile:0.01(Astronomy & Astrophysics)Nayak, M.*; Tanida, Kiyoshi; Belle Collaboration*; 180 of others*
Physical Review D, 102(7), p.071102_1 - 071102_8, 2020/10
Times Cited Count:6 Percentile:41.47(Astronomy & Astrophysics)Chen, Y. Q.*; Tanida, Kiyoshi; Belle Collaboration*; 181 of others*
Physical Review D, 102(1), p.012002_1 - 012002_12, 2020/07
Times Cited Count:11 Percentile:61.3(Astronomy & Astrophysics)Mizuk, R.*; Tanida, Kiyoshi; Belle Collaboration*; 181 of others*
Journal of High Energy Physics (Internet), 2019(10), p.220_1 - 220_26, 2019/10
Times Cited Count:31 Percentile:84.26(Physics, Particles & Fields)Waheed, E.*; Tanida, Kiyoshi; Belle Collaboration*; 187 of others*
Physical Review D, 100(5), p.052007_1 - 052007_32, 2019/09
Times Cited Count:44 Percentile:91.52(Astronomy & Astrophysics)Amaducci, S.*; Harada, Hideo; Kimura, Atsushi; 118 of others*
European Physical Journal A, 55(7), p.120_1 - 120_19, 2019/07
Times Cited Count:23 Percentile:90.61(Physics, Nuclear)The U(n, f) cross section was measured at n_TOF relative to Li(n, t) and B(n, ), in a wide energy range (25 meV170 keV) with 1.5% systematic uncertainty, making use of a stack of six samples and six silicon detectors placed in the neutron beam. The present results indicate that the cross section in the 918 keV neutron energy range is indeed overestimated by almost 5% in the recently released evaluated data files ENDF/B-VIII.0 and JEFF3.3. Furthermore, these new high-resolution data confirm the existence of resonance-like structures in the keV neutron energy region. From the present data, a value of 249.71.4(stat)0.94(syst) b eV has been extracted for the cross section integral between 7.8 and 11 eV, confirming the value of 247.53 b eV recently established as a standard.
Lai, Y.-T.*; Tanida, Kiyoshi; Belle Collaboration*; 186 of others*
Physical Review D, 100(1), p.011101_1 - 011101_9, 2019/07
Times Cited Count:1 Percentile:7.66(Astronomy & Astrophysics)Seidl, R.*; Tanida, Kiyoshi; Belle Collaboration*; 186 of others*
Physical Review D, 99(11), p.112006_1 - 112006_15, 2019/06
Times Cited Count:15 Percentile:64.92(Astronomy & Astrophysics)Sumihama, Mizuki*; Tanida, Kiyoshi; Belle Collaboration*; 184 of others*
Physical Review Letters, 122(7), p.072501_1 - 072501_7, 2019/02
Times Cited Count:22 Percentile:81.07(Physics, Multidisciplinary)Kim, J. B.*; Tanida, Kiyoshi; Belle Collaboration*; 182 of others*
Physical Review D, 99(1), p.011104_1 - 011104_7, 2019/01
Times Cited Count:4 Percentile:25.62(Astronomy & Astrophysics)Gelb, M.*; Tanida, Kiyoshi; Belle Collaboration*; 185 of others*
Physical Review D, 98(11), p.112016_1 - 112016_13, 2018/12
Times Cited Count:16 Percentile:60.98(Astronomy & Astrophysics)Yin, J. H.*; Tanida, Kiyoshi; Belle Collaboration*; 189 of others*
Physical Review D, 98(9), p.091102_1 - 091102_9, 2018/11
Times Cited Count:4 Percentile:23.59(Astronomy & Astrophysics)