Ryosuke Komatani
Nagoya University
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Featured researches published by Ryosuke Komatani.
Progress of Theoretical and Experimental Physics | 2017
Masahiro Yoshimoto; T. Nakano; Ryosuke Komatani; Hiroaki Kawahara
Automatic nuclear emulsion readout systems have seen remarkable progress since the original idea was developed almost 40 years ago. After the success of its full application to a large-scale neutrino experiment, OPERA, a much faster readout system, the hyper-track selector (HTS), has been developed. HTS, which has an extremely wide-field objective lens, reached a scanning speed of 4700 cm
Progress of Theoretical and Experimental Physics | 2017
T. Fukuda; S. Aoki; S. V. Cao; N. Chikuma; Y. Fukuzawa; M. Gonin; T. Hayashino; Y. Hayato; A. Hiramoto; F. Hosomi; K. Ishiguro; S. Iori; T. Inoh; Hiroaki Kawahara; Hyun-Jeong Kim; N. Kitagawa; T. Koga; Ryosuke Komatani; M. Komatsu; A. Matsushita; S. Mikado; A. Minamino; H. Mizusawa; K. Morishima; T. Matsuo; T. Matsumoto; Y. Morimoto; Misaki Morishita; Kouji Nakamura; M. Nakamura
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Progress of Theoretical and Experimental Physics | 2018
H. Rokujo; Shigeki Aoki; Kaname Hamada; T. Hara; Tatsuki Inoue; K. Ishiguro; Atsushi Iyono; Hiroaki Kawahara; K. Kodama; Ryosuke Komatani; M. Komatsu; Tetsuya Kosaka; M. Miyanishi; F. Mizutani; K. Morishima; Misaki Morishita; N. Naganawa; Mitsuhiro Nakamura; T. Nakano; Akira Nishio; K. Niwa; Naoto Otsuka; K. Ozaki; O. Sato; E. Shibayama; A. T. Suzuki; Satoru Takahashi; Ryo Tanaka; Yurie Tateishi; Shuichi Tawa
/h, which is nearly 100 times faster than the previous system and therefore strongly promotes many new experimental projects. We will describe the concept, specifications, system structure, and achieved performance in this paper.
Progress of Theoretical and Experimental Physics | 2017
Kyohei Yamada; H. Kim; T. Nakaya; T. Matsumoto; Y. Seiya; S. Takahashi; K. Ishiguro; S. Mikado; N. Naganawa; Masahiro Yoshimoto; H. Shibuya; T. Matsuo; S. Ogawa; A. Matsushita; K. Morishima; S. Tada; B. Quilain; Y. Hayato; S. Cao; Ryosuke Komatani; O. Sato; M. Nakamura; K. Nakamura; S. Aoki; Y. Morimoto; Misaki Morishita; A. Minamino; Hiroaki Kawahara; N. Kitagawa; M. Komatsu
Precise neutrino–nucleus interaction measurements in the sub-multi-GeV region are important to reduce the systematic uncertainty in future neutrino oscillation experiments. Furthermore, an excess of νe interactions, as a possible interpretation of the existence of a sterile neutrino, has been observed in such an energy region. The nuclear emulsion technique can measure all the final state particles with low energy threshold for a variety of targets (Fe, C, H2O, and so on). Its sub- μm position resolution allows measurements of the νe cross-section with good electron/gamma separation capability. We started a new experiment at J-PARC to study sub-multi-GeV neutrino interactions by introducing the nuclear emulsion technique. The J-PARC T60 experiment has been implemented as a first step in such a project. Systematic neutrino event analysis with full scanning data in the nuclear emulsion detector was performed for the first time. The first neutrino event detection and its analysis are described in this paper.
Proceedings of The 3rd International Symposium on “Quest for the Origin of Particles and the Universe" — PoS(KMI2017) | 2017
Masahiro Yoshimoto; T. Nakano; Ryosuke Komatani
We promote the precise gamma-ray observation project Gamma-Ray Astro-Imager with Nuclear Emulsion (GRAINE), which uses balloon-borne emulsion gamma-ray telescopes. The emulsion telescope realizes observations with high angular resolution, polarization sensitivity, and large aperture area in the 0.01--100 GeV energy region. Herein, we report the data analysis of emulsion tracks and the first demonstration of gamma-ray imaging via an emulsion telescope by using the flight data from the balloon experiment performed in 2015 (GRAINE 2015). The emulsion films were scanned by the latest read-out system for a total area of 41 m
Proceedings of 35th International Cosmic Ray Conference — PoS(ICRC2017) | 2017
Atsushi Iyono; Shegeki Aoki; T. Hara; Kenji Kuretsubo; Haruka Matsumoto; F. Mizutani; K. Ozaki; E. Shibayama; A. T. Suzuki; Satoru Takahashi; Yurie Tateishi; Misato Yabu; Kyohei Yamada; K. Kodama; K. Hamada; Hiroki Kawahara; Ryosuke Komatani; M. Komatsu; Motoaki Miyashita; Misaki Morishita; K. Morishima; Mitsuhiro Nakamura; N. Naganawa; T. Nakano; Akira Nishio; K. Niwa; Naoto Otsuka; H. Rokujo; Osamu Sato; Masahiro Yoshimoto
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Progress of Theoretical and Experimental Physics | 2016
Satoru Takahashi; Shigeki Aoki; Kaname Hamada; T. Hara; Tatsuki Inoue; K. Ishiguro; Atsushi Iyono; Hiroaki Kawahara; K. Kodama; Ryosuke Komatani; M. Komatsu; Tetsuya Kosaka; M. Miyanishi; F. Mizutani; K. Morishima; Misaki Morishita; N. Naganawa; Mitsuhiro Nakamura; T. Nakano; Akira Nishio; K. Niwa; Naoto Otsuka; K. Ozaki; H. Rokujo; O. Sato; E. Shibayama; A. T. Suzuki; Ryo Tanaka; Yurie Tateishi; Shuichi Tawa
in three months, and then the gamma-ray event selection was automatically processed. Millions of electron-pair events are accumulated in the balloon-borne emulsion telescope. The emulsion telescope detected signals from a calibration source (gamma rays from the interaction of cosmic rays with an aluminum plate) with a high significance during the balloon observation and created a gamma-ray image consistent with the source size and the expected angular resolution in the energy range of 100--300 MeV. The flight performance obtained in the GRAINE 2015 experiment proves that balloon-borne emulsion telescope experiments with larger area are feasible while maintaining expected imaging performance.
Radiation Measurements | 2013
K. Morishima; K. Hamada; Ryosuke Komatani; T. Nakano; K. Kodama
We describe the first ever implementation of an emulsion multi-stage shifter in an accelerator neutrino experiment. The system was installed in the neutrino monitor building in J-PARC as a part of a test experiment T60 and stable operation was maintained for a total of 126.6 days. By applying time information to emulsion films, various results were obtained. Time resolutions of 5.3 to 14.7 s were evaluated in an operation spanning 46.9 days (time resolved numbers of 3.8--1.4
Transactions of The Japan Society for Aeronautical and Space Sciences, Space Technology Japan | 2018
F. Mizutani; Shigeki Aoki; K. Hamada; T. Hara; Atsushi Iyono; Hiroaki Kawahara; K. Kodama; Ryosuke Komatani; M. Komatsu; Kenji Kuretsubo; Toshitsugu Marushima; Haruka Matsumoto; M. Miyanishi; K. Morishima; Misaki Morishita; N. Naganawa; Mitsuhiro Nakamura; T. Nakano; Akira Nishio; K. Niwa; Naoto Otsuka; K. Ozaki; H. Rokujo; O. Sato; E. Shibayama; A. T. Suzuki; Satoru Takahashi; Yurie Tateishi; Misato Yabu; Kyohei Yamada
\times10^{5}
The Japan Society of Applied Physics | 2017
Kanji Watanabe; Hideki Tomita; Masahiro Yoshimoto; K. Morishima; Ryosuke Komatani; T. Naka; T. Nakano; Mitsuhiro Nakamura; Tetsuo Iguchi
). By using timing and spatial information, a reconstruction of coincident events that consisted of high multiplicity events and vertex events, including neutrino events was performed. Emulsion events were matched to events observed by INGRID, one of near detectors of the T2K experiment, with high reliability (98.5\%) and hybrid analysis was established via use of the multi-stage shifter. The results demonstrate that the multi-stage shifter is feasible for use in neutrino experiments.