Zobrazeno 1 - 10
of 82
pro vyhledávání: '"Nakamura, Kiseki"'
Autor:
Honjo, Takashi, Ashida, Yosuke, Auersperg-Castell, Oderich F., Friend, Megan, Heitkamp, Ian, Ichikawa, Atsuko K., Ishitsuka, Masaki, Izumi, Nao, Kasama, Sohei, Kashiwagi, Shigeru, Kawamura, Yuma, Kikawa, Tatsuya, Kobata, Takuya, Matsubara, Tsunayuki, Miyabe, Manabu, Nakamura, Kiseki D., Nakamura, Hina, Sato, Yukine, Sakashita, Ken, Seiya, Yoshihiro, Takifuji, Kouchi, Tokiyasu, Atsushi, Yamamoto, Tatsuya, Yamamoto, Kazuhiro, Yasutome, Kenji
Upgrade work towards increasing the beam intensity of the neutrino beamline at J- PARC is underway. Monitoring tertiary muon beams is essential for stable operation of the beamline. Accordingly, we plan to replace the present muon monitor sensors wit
Externí odkaz:
http://arxiv.org/abs/2405.05877
Autor:
KamLAND, Collaborations, Super-Kamiokande, Abe, Seisho, Eizuka, Minori, Futagi, Sawako, Gando, Azusa, Gando, Yoshihito, Goto, Shun, Hachiya, Takahiko, Hata, Kazumi, Ichimura, Koichi, Ieki, Sei, Ikeda, Haruo, Inoue, Kunio, Ishidoshiro, Koji, Kamei, Yuto, Kawada, Nanami, Kishimoto, Yasuhiro, Koga, Masayuki, Kurasawa, Maho, Mitsui, Tadao, Miyake, Haruhiko, Morita, Daisuke, Nakahata, Takeshi, Nakajima, Rika, Nakamura, Kengo, Nakamura, Rikuo, Nakamura, Ryo, Nakane, Jun, Ozaki, Hideyoshi, Saito, Keita, Sakai, Taichi, Shimizu, Itaru, Shirai, Junpei, Shiraishi, Kensuke, Shoji, Ryunosuke, Suzuki, Atsuto, Takeuchi, Atsuto, Tamae, Kyoko, Watanabe, Hiroko, Watanabe, Kazuho, Yoshida, Sei, Umehara, Saori, Fushimi, Ken-Ichi, Kotera, Kenta, Urano, Yusuke, Berger, Bruce E., Fujikawa, Brian K., Larned, John G., Maricic, Jelena, Fu, Zhenghao, Smolsky, Joseph, Winslow, Lindley A., Efremenko, Yuri, Karwowski, Hugon J., Markoff, Diane M., Tornow, Werner, Dell'Oro, Stefano, O'Donnell, Thomas, Detwiler, Jason A., Enomoto, Sanshiro, Decowski, Michal P., Weerman, Kelly M., Grant, Christopher, Song, Hasung, Li, Aobo, Axani, Spencer N., Garcia, Miles, Abe, Ko, Bronner, Christophe, Hayato, Yoshinari, Hiraide, Katsuki, Hosokawa, Keishi, Ieki, Kei, Ikeda, Motoyasu, Kameda, June, Kanemura, Yuki, Kaneshima, Ryota, Kashiwagi, Yuri, Kataoka, Yousuke, Miki, Shintaro, Mine, Shunichi, Miura, Makoto, Moriyama, Shigetaka, Nakahata, Masayuki, Nakano, Yuuki, Nakayama, Shoei, Noguchi, Yohei, Sato, Kazufumi, Sekiya, Hiroyuki, Shiba, Hayato, Shimizu, Kotaro, Shiozawa, Masato, Sonoda, Yutaro, Suzuki, Yoichiro, Takeda, Atsushi, Takemoto, Yasuhiro, Tanaka, Hidekazu K., Yano, Takatomi, Han, Seungho, Kajita, Takaaki, Okumura, Kimihiro, Tashiro, Takuya, Tomiya, Takuya, Wang, Xubin, Yoshida, Shunsuke, Fernandez, Pablo, Labarga, Luis, Ospina, Nataly, Zaldivar, Bryan, Pointon, Barry W., Kearns, Edward, Raaf, Jennifer L., Wan, Linyan, Wester, Thomas, Bian, Jianming, Griskevich, Jeff, Smy, Michael B., Sobel, Henry W., Takhistov, Volodymyr, Yankelevich, Alejandro, Hill, James, Jang, MinCheol, Lee, Seonghak, Moon, DongHo, Park, RyeongGyoon, Bodur, Baran, Scholberg, Kate, Walter, Chris W., Beauchêne, Antoine, Drapier, Olivier, Giampaolo, Alberto, Mueller, Thomas A., Santos, Andrew D., Paganini, Pascal, Quilain, Benjamin, Rogly, Rudolph, Nakamura, Taku, Jang, Jee-Seung, Machado, Lucas N., Learned, John G., Choi, Koun, Iovine, Nadege, Cao, Son V., Anthony, Lauren H. V., Martin, Daniel G. R., Prouse, Nick W., Scott, Mark, Uchida, Yoshi, Berardi, Vincenzo, Calabria, Nicola F., Catanesi, M. G., Radicioni, Emilio, Langella, Aurora, de Rosa, Gianfranca, Collazuol, Gianmaria, Feltre, Matteo, Iacob, Fabio, Mattiazzi, Marco, Ludovici, Lucio, Gonin, Michel, Périssé, Lorenzo, Pronost, Guillaume, Fujisawa, Chiori, Horiuchi, Shogo, Kobayashi, Misaki, Liu, Yu-Ming, Maekawa, Yuto, Nishimura, Yasuhiro, Okazaki, Reo, Akutsu, Ryosuke, Friend, Megan, Hasegawa, Takuya, Ishida, Taku, Kobayashi, Takashi, Jakkapu, Mahesh, Matsubara, Tsunayuki, Nakadaira, Takeshi, Nakamura, Kenzo, Oyama, Yuichi, Sakashita, Ken, Sekiguchi, Tetsuro, Tsukamoto, Toshifumi, Yrey, Antoniosk Portocarrero, Bhuiyan, Nahid, Burton, George T., Di Lodovico, Francesca, Gao, Joanna, Goldsack, Alexander, Katori, Teppei, Migenda, Jost, Ramsden, Rory M., Xie, Zhenxiong, Zsoldos, Stephane, Suzuki, Atsumu T., Takagi, Yusuke, Takeuchi, Yasuo, Zhong, Haiwen, Feng, Jiahui, Feng, Li-Cheng, Hu, Jianrun, Hu, Zhuojun, Kawaue, Masaki, Kikawa, Tatsuya, Mori, Masamitsu, Nakaya, Tsuyoshi, Wendell, Roger A., Yasutome, Kenji, Jenkins, Sam J., McCauley, Neil K., Mehta, Pruthvi, Tarrant, Adam, Wilking, Mike J., Fukuda, Yoshiyuki, Itow, Yoshitaka, Menjo, Hiroaki, Ninomiya, Kotaro, Yoshioka, Yushi, Lagoda, Justyna, Mandal, Maitrayee, Mijakowski, Piotr, Prabhu, Yashwanth S., Zalipska, Joanna, Jia, Mo, Jiang, Junjie, Shi, Wei, Yanagisawa, Chiaki, Harada, Masayuki, Hino, Yota, Ishino, Hirokazu, Koshio, Yusuke, Nakanishi, Fumi, Sakai, Seiya, Tada, Tomoaki, Tano, Tomohiro, Ishizuka, Takeharu, Barr, Giles, Barrow, Daniel, Cook, Laurence, Samani, Soniya, Wark, David, Holin, Anna, Nova, Federico, Jung, Seunghyun, Yang, Byeongsu, Yang, JeongYeol, Yoo, Jonghee, Fannon, Jack E. P., Kneale, Liz, Malek, Matthew, McElwee, Jordan M., Thiesse, Matthew D., Thompson, Lee F., Wilson, Stephen T., Okazawa, Hiroko, Mohan, Lakshmi S., Kim, SooBong, Kwon, Eunhyang, Seo, Ji-Woong, Yu, Intae, Ichikawa, Atsuko K., Nakamura, Kiseki D., Tairafune, Seidai, Nishijima, Kyoshi, Eguchi, Aoi, Nakagiri, Kota, Nakajima, Yasuhiro, Shima, Shizuka, Taniuchi, Natsumi, Watanabe, Eiichiro, Yokoyama, Masashi, de Perio, Patrick, Fujita, Saki, Jesus-Valls, Cesar, Martens, Kai, Tsui, Ka M., Vagins, Mark R., Xia, Junjie, Izumiyama, Shota, Kuze, Masahiro, Matsumoto, Ryo, Terada, Kotaro, Asaka, Ryusei, Ishitsuka, Masaki, Ito, Hiroshi, Ommura, Yuga, Shigeta, Natsuki, Shinoki, Masataka, Yamauchi, Koki, Yoshida, Tsukasa, Gaur, Rhea, Gousy-Leblan, Vincent, Hartz, Mark, Konaka, Akira, Li, Xiaoyue, Chen, Shaomin, Xu, Benda, Zhang, Aiqiang, Zhang, Bin, Posiadala-Zezula, Magdalena, Boyd, Steven B., Edwards, Rory, Hadley, David, Nicholson, Matthew, O'Flaherty, Marcus, Richards, Benjamin, Ali, Ajmi, Jamieson, Blair, Amanai, Shogo, Marti-Magro, Lluis, Minamino, Akihiro, Shibayama, Ryo, Suzuki, Serina
Preceding a core-collapse supernova, various processes produce an increasing amount of neutrinos of all flavors characterized by mounting energies from the interior of massive stars. Among them, the electron antineutrinos are potentially detectable b
Externí odkaz:
http://arxiv.org/abs/2404.09920
Autor:
Namai, Ryota, Higashino, Satoshi, Ishiura, Hirohisa, Ikeda, Tomonori, Ofuji, Mizuno, Nakayama, Ayaka, Nakamura, Kiseki, Ito, Hiroshi, Ichimura, Koichi, Abe, Ko, Kobayashi, Kazuyoshi, Takada, Atsushi, Kubota, Ryo, Miuchi, Kentaro
Direct detection of weakly interacting massive particles (WIMPs) can provide strong evidence of their existence and the directional method would have an advantage over other methods to detect the clear signal of WIMPs. Time projection chambers with m
Externí odkaz:
http://arxiv.org/abs/2403.11736
Autor:
Yoshida, Masashi, Nakamura, Kazuhiro, Akiyama, Shinichi, Ban, Sei, Hikida, Junya, Hirose, Masanori, Ichikawa, Atsuko K., Iwashita, Yoshihisa, Kashino, Yukimasa, Kikawa, Tatsuya, Minamino, Akihiro, Miuchi, Kentaro, Nakajima, Yasuhiro, Nakamura, Kiseki D., Nakaya, Tsuyoshi, Obara, Shuhei, Sakashita, Ken, Sekiya, Hiroyuki, Shinagawa, Hibiki, Sugashima, Bungo, Urano, Soki
Publikováno v:
Progress of Theoretical and Experimental Physics, Volume 2024 Issue 1, 013H01
We have been developing a high-pressure xenon gas time projection chamber (TPC) to search for neutrinoless double beta ($0\nu\beta\beta$) decay of $^{136}$Xe. The unique feature of this TPC is in the detection part of ionization electrons, called ELC
Externí odkaz:
http://arxiv.org/abs/2310.19714
Autor:
Shimada, Takuya, Higashino, Satoshi, Ikeda, Tomonori, Nakamura, Kiseki, Yakabe, Ryota, Hashimoto, Takashi, Ishiura, Hirohisa, Nakamura, Takuma, Nakazawa, Miki, Kubota, Ryo, Nakayama, Ayaka, Ito, Hiroshi, Ichimura, Koichi, Abe, Ko, Kobayashi, Kazuyoshi, Tanimori, Toru, Kubo, Hidetoshi, Takada, Atsushi, Sekiya, Hiroyuki, Takeda, Atsushi, Miuchi, Kentaro
NEWAGE is a direction-sensitive dark matter search experiment with a three-dimensional tracking detector based on a gaseous micro time projection chamber. A direction-sensitive dark matter search was carried out at Kamioka Observatory with a total li
Externí odkaz:
http://arxiv.org/abs/2301.04779
Autor:
Ikeda, Tomonori, Nakamura, Kiseki, Shimada, Takuya, Yakabe, Ryota, Hashimoto, Takashi, Ishiura, Hirohisa, Nakamura, Takuma, Ito, Hiroshi, Ichimura, Koichi, Abe, Ko, Kobayashi, Kazuyoshi, Tanimori, Toru, Kubo, Hidetoshi, Takada, Atsushi, Sekiya, Hiroyuki, Takeda, Atsushi, Miuchi, Kentaro
Publikováno v:
Prog. Theor. Exp. Phys. 2021, 063F01
NEWAGE is a direction-sensitive dark matter search using a low-pressure gaseous time projection chamber. A low alpha-ray emission rate micro pixel chamber had been developed in order to reduce background for dark matter search. We conducted the dark
Externí odkaz:
http://arxiv.org/abs/2101.09921
Autor:
Nakamura, Kiseki D., Miuchi, Kentaro, Kazama, Shingo, Shoji, Yutaro, Ibe, Masahiro, Nakano, Wakutaka
Migdal effect is attracting interests because of the potential to enhance the sensitivities of direct dark matter searches to the low mass region. In spite of its great importance, the Migdal effect has not been experimentally observed yet. A realist
Externí odkaz:
http://arxiv.org/abs/2009.05939
Autor:
Yakabe, Ryota, Nakamura, Kiseki, Ikeda, Tomonori, Ito, Hiroshi, Yamaguchi, Yushiro, Taishaku, Ryosuke, Nakazawa, Miki, Ishiura, Hirohisa, Nakamura, Takuma, Shimada, Takuya, Tanimori, Toru, Kubo, Hidetoshi, Takada, Atsushi, Sekiya, Hiroyuki, Takeda, Atsushi, Miuchi, Kentaro
The first directional dark matter search with three-dimensional tracking with head-tail sensitivity (3d-vector tracking analysis) was performed with a gaseous three-dimensional tarcking detector, or the NEWAGE-0.3b' detector. The search was carried o
Externí odkaz:
http://arxiv.org/abs/2005.05157
Autor:
Hashimoto, Takashi, Miuchi, Kentaro, Ikeda, Tomonori, Ishiura, Hirohisa, Nakamura, Kiseki D., Ito, Hiroshi, Ichimura, Koichi, Abe, Ko, Kobayashi, Kazuyoshi, Takada, Atsushi, Ochi, Atsuhiko, Nakamura, Takuma, Shimada, Takuya
Direction sensitivity could provide robust evidence for the direct detection of weakly interacting massive particles constituting dark matter. However, the sensitivity of this method remains low due to the radioactive backgrounds. The purpose of this
Externí odkaz:
http://arxiv.org/abs/2002.12633
The electronic energy deposited on nuclear emulsions due to C ions of 5 -- 200~keV and Kr ions of 5 -- 600~keV are evaluated and compared with those due to fast ions for design and construction of fine grain nuclear emulsion for directional dark matt
Externí odkaz:
http://arxiv.org/abs/1905.06664