Cosmic-ray muons that enter the Super-Kamiokande detector cause hadronic showers due to spallation in water, producing neutrons and radioactive isotopes. These are a major background source for studies of MeV-scale neutrinos and searches for rare events. In 2020, gadolinium was introduced into the ultra-pure water in the Super-Kamiokande detector to improve the detection efficiency of neutrons. In this study, the cosmogenic neutron yield was measured using data acquired during the period after the gadolinium loading. The yield was found to be (2.76 0.02(stat) 0.19(syst)) x 10(-4) mu(-1) g(-1) cm(2) at an average muon energy 259 GeV at the Super-Kamiokande detector.

Measurement of the cosmogenic neutron yield in Super-Kamiokande with gadolinium loaded water / Shinoki, M; Abe, K; Hayato, Y; Hiraide, K; Hosokawa, K; Ieki, K; Ikeda, M; Kameda, J; Kanemura, Y; Kaneshima, R; Kashiwagi, Y; Kataoka, Y; Miki, S; Mine, S; Miura, M; Moriyama, S; Nakano, Y; Nakahata, M; Nakayama, S; Noguchi, Y; Okamoto, K; Sato, K; Sekiya, H; Shiba, H; Shimizu, K; Shiozawa, M; Sonoda, Y; Suzuki, Y; Takeda, A; Takemoto, Y; Takenaka, A; Tanaka, H; Watanabe, S; Yano, T; Han, S; Kajita, T; Okumura, K; Tashiro, T; Tomiya, T; Wang, X; Yoshida, S; Megias, Gd; Fernandez, P; Labarga, L; Ospina, N; Zaldivar, B; Pointon, Bw; Kearns, E; Raaf, Jl; Wan, L; Wester, T; Bian, J; Griskevich, Nj; Kropp, Wr; Locke, S; Smy, Mb; Sobel, Hw; Takhistov, V; Yankelevich, A; Hill, J; Lee, Sh; Moon, Dh; Park, Rg; Bodur, B; Scholberg, K; Walter, Cw; Beauchêne, A; Bernard, L; Coffani, A; Drapier, O; El Hedri, S; Giampaolo, A; Mueller, Ta; Santos, Ad; Paganini, P; Quilain, B; Ishizuka, T; Nakamura, T; Jang, Js; Learned, Jg; Choi, K; Cao, S; Anthony, Lhv; Martin, D; Scott, M; Sztuc, Aa; Uchida, Y; Berardi, V; Catanesi, Mg; Radicioni, E; Calabria, Nf; Langella, A; Machado, Ln; De Rosa, G; Collazuol, G; Iacob, F; Lamoureux, M; Mattiazzi, M; Ludovici, L; Gonin, M; Pronost, G; Fujisawa, C; Maekawa, Y; Nishimura, Y; Akutsu, R; Friend, M; Hasegawa, T; Ishida, T; Kobayashi, T; Jakkapu, M; Matsubara, T; Nakadaira, T; Nakamura, K; Oyama, Y; Sakashita, K; Sekiguchi, T; Tsukamoto, T; Bhuiyan, N; Boschi, T; Burton, Gt; Di Lodovico, F; Gao, J; Goldsack, A; Katori, T; Migenda, J; Taani, M; Xie, Z; Zsoldos, S; Kotsar, Y; Ozaki, H; Suzuki, At; Takeuchi, Y; Bronner, C; Feng, J; Kikawa, T; Mori, M; Nakaya, T; Wendell, Ra; Yasutome, K; Jenkins, Sj; Mccauley, N; Mehta, P; Tarrant, A; Tsui, Km; Fukuda, Y; Itow, Y; Menjo, H; Ninomiya, K; Lagoda, J; Lakshmi, Sm; Mandal, M; Mijakowski, P; Prabhu, Ys; Zalipska, J; Jia, M; Jiang, J; Jung, Ck; Wilking, Mj; Yanagisawa, C; Harada, M; Ishino, H; Ito, S; Kitagawa, H; Koshio, Y; Nakanish, F; Sakai, S; Barr, G; Barrow, D; Cook, L; Samani, S; Wark, D; Holin, A; Nova, F; Yang, Jy; Yang, Bs; Yoo, J; Fannon, Jep; Kneale, L; Malek, M; Mcelwee, Jm; Stone, O; Thiesse, Md; Thompson, Lf; Okazawa, H; Kim, Sb; Kwon, E; Seo, Jw; Yu, I; Ichikawa, Ak; Nakamura, Kd; Tairafune, S; Nishijima, K; Koshiba, M; Iwamoto, K; Nakagiri, K; Nakajima, Y; Shima, S; Taniuchi, N; Yokoyama, M; Martens, K; de Perio, P; Vagins, Mr; Xia, J; Kuze, M; Izumiyama, S; Inomoto, M; Ishitsuka, M; Ito, H; Kinoshita, T; Matsumoto, R; Ommura, Y; Shigeta, N; Suganuma, T; Yamauchi, K; Martin, Jf; Tanaka, Ha; Towstego, T; Gaur, R; Gousy-Leblanc, V; Hartz, M; Konaka, A; Li, X; Prouse, Nw; Chen, S; Xu, Bd; Zhang, B; Posiadala-Zezula, M; Boyd, Sb; Hadley, D; Nicholson, M; O'Flaherty, M; Richards, B; Ali, A; Jamieson, B; Marti, L; Minamino, A; Pintaudi, G; Sano, S; Suzuki, S; Wada, K. - In: PHYSICAL REVIEW D. - ISSN 2470-0010. - 107:9(2023). [10.1103/PhysRevD.107.092009]

Measurement of the cosmogenic neutron yield in Super-Kamiokande with gadolinium loaded water

Berardi, V
Membro del Collaboration Group
;
Calabria, NF
Membro del Collaboration Group
;
2023-01-01

Abstract

Cosmic-ray muons that enter the Super-Kamiokande detector cause hadronic showers due to spallation in water, producing neutrons and radioactive isotopes. These are a major background source for studies of MeV-scale neutrinos and searches for rare events. In 2020, gadolinium was introduced into the ultra-pure water in the Super-Kamiokande detector to improve the detection efficiency of neutrons. In this study, the cosmogenic neutron yield was measured using data acquired during the period after the gadolinium loading. The yield was found to be (2.76 0.02(stat) 0.19(syst)) x 10(-4) mu(-1) g(-1) cm(2) at an average muon energy 259 GeV at the Super-Kamiokande detector.
2023
Measurement of the cosmogenic neutron yield in Super-Kamiokande with gadolinium loaded water / Shinoki, M; Abe, K; Hayato, Y; Hiraide, K; Hosokawa, K; Ieki, K; Ikeda, M; Kameda, J; Kanemura, Y; Kaneshima, R; Kashiwagi, Y; Kataoka, Y; Miki, S; Mine, S; Miura, M; Moriyama, S; Nakano, Y; Nakahata, M; Nakayama, S; Noguchi, Y; Okamoto, K; Sato, K; Sekiya, H; Shiba, H; Shimizu, K; Shiozawa, M; Sonoda, Y; Suzuki, Y; Takeda, A; Takemoto, Y; Takenaka, A; Tanaka, H; Watanabe, S; Yano, T; Han, S; Kajita, T; Okumura, K; Tashiro, T; Tomiya, T; Wang, X; Yoshida, S; Megias, Gd; Fernandez, P; Labarga, L; Ospina, N; Zaldivar, B; Pointon, Bw; Kearns, E; Raaf, Jl; Wan, L; Wester, T; Bian, J; Griskevich, Nj; Kropp, Wr; Locke, S; Smy, Mb; Sobel, Hw; Takhistov, V; Yankelevich, A; Hill, J; Lee, Sh; Moon, Dh; Park, Rg; Bodur, B; Scholberg, K; Walter, Cw; Beauchêne, A; Bernard, L; Coffani, A; Drapier, O; El Hedri, S; Giampaolo, A; Mueller, Ta; Santos, Ad; Paganini, P; Quilain, B; Ishizuka, T; Nakamura, T; Jang, Js; Learned, Jg; Choi, K; Cao, S; Anthony, Lhv; Martin, D; Scott, M; Sztuc, Aa; Uchida, Y; Berardi, V; Catanesi, Mg; Radicioni, E; Calabria, Nf; Langella, A; Machado, Ln; De Rosa, G; Collazuol, G; Iacob, F; Lamoureux, M; Mattiazzi, M; Ludovici, L; Gonin, M; Pronost, G; Fujisawa, C; Maekawa, Y; Nishimura, Y; Akutsu, R; Friend, M; Hasegawa, T; Ishida, T; Kobayashi, T; Jakkapu, M; Matsubara, T; Nakadaira, T; Nakamura, K; Oyama, Y; Sakashita, K; Sekiguchi, T; Tsukamoto, T; Bhuiyan, N; Boschi, T; Burton, Gt; Di Lodovico, F; Gao, J; Goldsack, A; Katori, T; Migenda, J; Taani, M; Xie, Z; Zsoldos, S; Kotsar, Y; Ozaki, H; Suzuki, At; Takeuchi, Y; Bronner, C; Feng, J; Kikawa, T; Mori, M; Nakaya, T; Wendell, Ra; Yasutome, K; Jenkins, Sj; Mccauley, N; Mehta, P; Tarrant, A; Tsui, Km; Fukuda, Y; Itow, Y; Menjo, H; Ninomiya, K; Lagoda, J; Lakshmi, Sm; Mandal, M; Mijakowski, P; Prabhu, Ys; Zalipska, J; Jia, M; Jiang, J; Jung, Ck; Wilking, Mj; Yanagisawa, C; Harada, M; Ishino, H; Ito, S; Kitagawa, H; Koshio, Y; Nakanish, F; Sakai, S; Barr, G; Barrow, D; Cook, L; Samani, S; Wark, D; Holin, A; Nova, F; Yang, Jy; Yang, Bs; Yoo, J; Fannon, Jep; Kneale, L; Malek, M; Mcelwee, Jm; Stone, O; Thiesse, Md; Thompson, Lf; Okazawa, H; Kim, Sb; Kwon, E; Seo, Jw; Yu, I; Ichikawa, Ak; Nakamura, Kd; Tairafune, S; Nishijima, K; Koshiba, M; Iwamoto, K; Nakagiri, K; Nakajima, Y; Shima, S; Taniuchi, N; Yokoyama, M; Martens, K; de Perio, P; Vagins, Mr; Xia, J; Kuze, M; Izumiyama, S; Inomoto, M; Ishitsuka, M; Ito, H; Kinoshita, T; Matsumoto, R; Ommura, Y; Shigeta, N; Suganuma, T; Yamauchi, K; Martin, Jf; Tanaka, Ha; Towstego, T; Gaur, R; Gousy-Leblanc, V; Hartz, M; Konaka, A; Li, X; Prouse, Nw; Chen, S; Xu, Bd; Zhang, B; Posiadala-Zezula, M; Boyd, Sb; Hadley, D; Nicholson, M; O'Flaherty, M; Richards, B; Ali, A; Jamieson, B; Marti, L; Minamino, A; Pintaudi, G; Sano, S; Suzuki, S; Wada, K. - In: PHYSICAL REVIEW D. - ISSN 2470-0010. - 107:9(2023). [10.1103/PhysRevD.107.092009]
File in questo prodotto:
File Dimensione Formato  
PhysRevD.107.092009.pdf

accesso aperto

Tipologia: Versione editoriale
Licenza: Creative commons
Dimensione 597.07 kB
Formato Adobe PDF
597.07 kB Adobe PDF Visualizza/Apri

I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.

Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11589/262883
Citazioni
  • Scopus 0
  • ???jsp.display-item.citation.isi??? 0
social impact