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Hyper-Kamiokande consists of two identical water-Cherenkov detectors of total 520 kt, with the first one in Japan at 295 km from the J-PARC neutrino beam with 2.5 degrees off-axis angles (OAAs), and the second one possibly in Korea at a later stage. Having the second detector in Korea would benefit almost all areas of neutrino oscillation physics, mainly due to longer baselines. There are several candidate sites in Korea with baselines of 1000-1300 km and OAAs of 1 degrees-3 degrees.We conducted sensitivity studies on neutrino oscillation physics for a second detector, either in Japan (JD x 2) or Korea (JD + KD), and compared the results with a single detector in Japan. Leptonic charge-parity (CP) symmetry violation sensitivity is improved, especially when the CP is non-maximally violated. The larger matter effect at Korean candidate sites significantly enhances sensitivities to non-standard interactions of neutrinos and mass ordering determination. Current studies indicate the best sensitivity is obtained at Mt. Bisul (1088 km baseline, 1.3 degrees OAA). Thanks to a larger (1000 m) overburden than the first detector site, clear improvements to sensitivities for solar and supernova relic neutrino searches are expected.
Physics potentials with the second Hyper-Kamiokande detector in Korea / Abe, K; Abe, Ke; Ahn, S H; Aihara, H; Aimi, A; Akutsu, R; Andreopoulos, C; Anghel, I; Anthony, L H V; Antonova, M; Ashida, Y; Aushev, V; Barbi, M; Barker, G J; Barr, G; Beltrame, P; Berardi, V; Bergevin, M; Berkman, S; Berns, L; Berry, T; Bhadra, S; Blaszczyk, F d M; Blondel, A; Bolognesi, S; Boyd, S B; Bravar, A; Bronner, C; Buizza Avanzini, M; Cafagna, F S; Calland, R; Cao, S; Cartwright, S L; Catanesi, M G; Checchia, C; Chen-Wishart, Z; Cheon, B G; Cheoun, M K; Cho, K; Choi, J H; Choi, K; Choi, K Y; Chun, E J; Cole, A; Coleman, J; Collazuol, G; Cowan, G; Cremonesi, L; Dealtry, T; De Rosa, G; Densham, C; Dewhurst, D; Drakopoulou, E; Di Lodovico, F; Drapier, O; Dumarchez, J; Dunne, P; Dziewiecki, M; Emery, S; Esmaili, A; Evangelisti, A; Fernández-Martinez, E; Feusels, T; Finch, A; Fiorentini, G A; Fiorillo, G; Fitton, M; Frankiewicz, K; Friend, M; Fujii, Y; Fukuda, Y; Fukuda, D; Ganezer, K; Ghosh, M; Giganti, C; Gonin, M; Grant, N; Gumplinger, P; Hadley, D R; Hartfiel, B; Hartz, M; Hayato, Y; Hayrapetyan, K; Hill, J; Hirota, S; Horiuchi, S; Ichikawa, A K; Iijima, T; Ikeda, M; Imber, J; Inoue, K; Insler, J; Intonti, R A; Ioannisian, A; Ishida, T; Ishino, H; Ishitsuka, M; Itow, Y; Iwamoto, K; Izmaylov, A; Jamieson, B; Jang, H I; Jang, J S; Jeon, S H; Jeong, K S; Jiang, M; Jonsson, P; Joo, K K; Kaboth, A; Kachulis, C; Kajita, T; Kang, S K; Kameda, J; Kataoka, Y; Katori, T; Kayrapetyan, K; Kearns, E; Khabibullin, M; Khotjantsev, A; Kim, C S; Kim, H B; Kim, H J; Kim, J H; Kim, J-S; Kim, J Y; Kim, S B; Kim, S C; Kim, S-W; Kim, S Y; Kim, T J; Kim, W; King, S; Kishimoto, Y; Ko, P; Kobayashi, T; Koga, M; Konaka, A; Kormos, L L; Koshio, Y; Korzenev, A; Kowalik, K L; Kropp, W R; Kudenko, Y; Kurjata, R; Kutter, T; Kuze, M; Kwak, K; Kwon, E H; Labarga, L; Lagoda, J; Lasorak, P J J; Laveder, M; Lawe, M; Learned, J G; Lee, C H; Lee, S J; Lee, W J; Lim, I T; Lindner, T; Litchfield, R P; Longhin, A; Loverre, P; Lou, T; Ludovici, L; Ma, W; Magaletti, L; Mahn, K; Malek, M; Maret, L; Mariani, C; Martens, K; Marti, Ll; Martin, J F; Marzec, J; Matsuno, S; Mazzucato, E; Mccarthy, M; Mccauley, N; Mcfarland, K S; Mcgrew, C; Mefodiev, A; Mermod, P; Metelko, C; Mezzetto, M; Migenda, J; Mijakowski, P; Minakata, H; Minamino, A; Mine, S; Mineev, O; Mitra, A; Miura, M; Mochizuki, T; Monroe, J; Moon, C S; Moon, D H; Moriyama, S; Mueller, T; Muheim, F; Murase, K; Muto, F; Nakahata, M; Nakajima, Y; Nakamura, K; Nakaya, T; Nakayama, S; Nantais, C; Needham, M; Nicholls, T; Nishimura, Y; Noah, E; Nova, F; Nowak, J; Nunokawa, H; Obayashi, Y; Oh, Y D; Oh, Y; O’Keeffe, H M; Okajima, Y; Okumura, K; Onishchuk, Yu; O’Sullivan, E; O’Sullivan, L; Ovsiannikova, T; Owen, R A; Oyama, Y; Pérez, J; Pac, M Y; Palladino, V; Palomino, J L; Paolone, V; Park, H S; Park, J C; Park, M G; Park, S C; Parker, W; Parsa, S; Payne, D; Perkin, J D; Pidcott, C; Pinzon Guerra, E; Playfer, S; Popov, B; Posiadala-Zezula, M; Poutissou, J-M; Pritchard, A; Prouse, N W; Pronost, G; Przewlocki, P; Quilain, B; Quinto, M; Radicioni, E; Ratoff, P N; Retiere, F; Riccio, C; Richards, B; Rondio, E; Rose, H J; Rott, C; Rountree, S D; Ruggeri, A C; Rychter, A; Ryu, D; Sacco, R; Sakuda, M; Sanchez, M C; Scantamburlo, E; Scott, M; Molina Sedgwick, S; Seiya, Y; Sekiguchi, T; Sekiya, H; Seo, H; Seo, S H; Sgalaberna, D; Shah, R; Shaikhiev, A; Shimizu, I; Shiozawa, M; Shitov, Y; Short, S; Simpson, C; Sinnis, G; Smy, M B; Snow, S; Sobczyk, J; Sobel, H W; Son, D C; Sonoda, Y; Spina, R; Stewart, T; Stone, J L; Suda, Y; Suwa, Y; Suzuki, Y; Suzuki, A T; Svoboda, R; Taani, M; Tacik, R; Takeda, A; Takenaka, A; Taketa, A; Takeuchi, Y; Takhistov, V; Tanaka, H A; Tanaka, H K M; Tanaka, H; Terri, R; Thiesse, M; Thompson, L F; Thorpe, M; Tobayama, S; Touramanis, C; Towstego, T; Tsukamoto, T; Tsui, K M; Tzanov, M; Uchida, Y; Vagins, M R; Vasseur, G; Vilela, C; Vogelaar, R B; Walding, J; Walker, J; Ward, M; Wark, D; Wascko, M O; Weber, A; Wendell, R; Wilkes, R J; Wilking, M J; Wilson, J R; Won, E; Xin, T; Yamamoto, K; Yanagisawa, C; Yano, T; Yasuda, O; Yen, S; Yershov, N; Yeum, D N; Yokoyama, M; Yoo, H D; Yoo, J; Yoon, S C; Yoon, T S; Yoshida, T; Yu, I; Yu, M; Zalipska, J; Zaremba, K; Ziembicki, M; Zito, M; Zsoldos, S. - In: PROGRESS OF THEORETICAL AND EXPERIMENTAL PHYSICS. - ISSN 2050-3911. - ELETTRONICO. - 2018:6(2018). [10.1093/ptep/pty044]
Physics potentials with the second Hyper-Kamiokande detector in Korea
Abe, K;Abe, Ke;Ahn, S H;Aihara, H;Aimi, A;Akutsu, R;Andreopoulos, C;Anghel, I;Anthony, L H V;Antonova, M;Ashida, Y;Aushev, V;Barbi, M;Barker, G J;Barr, G;Beltrame, P;Berardi, V;Bergevin, M;Berkman, S;Berns, L;Berry, T;Bhadra, S;Blaszczyk, F d M;Blondel, A;Bolognesi, S;Boyd, S B;Bravar, A;Bronner, C;Buizza Avanzini, M;Cafagna, F S;Calland, R;Cao, S;Cartwright, S L;Catanesi, M G;Checchia, C;Chen-Wishart, Z;Cheon, B G;Cheoun, M K;Cho, K;Choi, J H;Choi, K;Choi, K Y;Chun, E J;Cole, A;Coleman, J;Collazuol, G;Cowan, G;Cremonesi, L;Dealtry, T;De Rosa, G;Densham, C;Dewhurst, D;Drakopoulou, E;Di Lodovico, F;Drapier, O;Dumarchez, J;Dunne, P;Dziewiecki, M;Emery, S;Esmaili, A;Evangelisti, A;Fernández-Martinez, E;Feusels, T;Finch, A;Fiorentini, G A;Fiorillo, G;Fitton, M;Frankiewicz, K;Friend, M;Fujii, Y;Fukuda, Y;Fukuda, D;Ganezer, K;Ghosh, M;Giganti, C;Gonin, M;Grant, N;Gumplinger, P;Hadley, D R;Hartfiel, B;Hartz, M;Hayato, Y;Hayrapetyan, K;Hill, J;Hirota, S;Horiuchi, S;Ichikawa, A K;Iijima, T;Ikeda, M;Imber, J;Inoue, K;Insler, J;Intonti, R A;Ioannisian, A;Ishida, T;Ishino, H;Ishitsuka, M;Itow, Y;Iwamoto, K;Izmaylov, A;Jamieson, B;Jang, H I;Jang, J S;Jeon, S H;Jeong, K S;Jiang, M;Jonsson, P;Joo, K K;Kaboth, A;Kachulis, C;Kajita, T;Kang, S K;Kameda, J;Kataoka, Y;Katori, T;Kayrapetyan, K;Kearns, E;Khabibullin, M;Khotjantsev, A;Kim, C S;Kim, H B;Kim, H J;Kim, J H;Kim, J-S;Kim, J Y;Kim, S B;Kim, S C;Kim, S-W;Kim, S Y;Kim, T J;Kim, W;King, S;Kishimoto, Y;Ko, P;Kobayashi, T;Koga, M;Konaka, A;Kormos, L L;Koshio, Y;Korzenev, A;Kowalik, K L;Kropp, W R;Kudenko, Y;Kurjata, R;Kutter, T;Kuze, M;Kwak, K;Kwon, E H;Labarga, L;Lagoda, J;Lasorak, P J J;Laveder, M;Lawe, M;Learned, J G;Lee, C H;Lee, S J;Lee, W J;Lim, I T;Lindner, T;Litchfield, R P;Longhin, A;Loverre, P;Lou, T;Ludovici, L;Ma, W;Magaletti, L;Mahn, K;Malek, M;Maret, L;Mariani, C;Martens, K;Marti, Ll;Martin, J F;Marzec, J;Matsuno, S;Mazzucato, E;McCarthy, M;McCauley, N;McFarland, K S;McGrew, C;Mefodiev, A;Mermod, P;Metelko, C;Mezzetto, M;Migenda, J;Mijakowski, P;Minakata, H;Minamino, A;Mine, S;Mineev, O;Mitra, A;Miura, M;Mochizuki, T;Monroe, J;Moon, C S;Moon, D H;Moriyama, S;Mueller, T;Muheim, F;Murase, K;Muto, F;Nakahata, M;Nakajima, Y;Nakamura, K;Nakaya, T;Nakayama, S;Nantais, C;Needham, M;Nicholls, T;Nishimura, Y;Noah, E;Nova, F;Nowak, J;Nunokawa, H;Obayashi, Y;Oh, Y D;Oh, Y;O’Keeffe, H M;Okajima, Y;Okumura, K;Onishchuk, Yu;O’Sullivan, E;O’Sullivan, L;Ovsiannikova, T;Owen, R A;Oyama, Y;Pérez, J;Pac, M Y;Palladino, V;Palomino, J L;Paolone, V;Park, H S;Park, J C;Park, M G;Park, S C;Parker, W;Parsa, S;Payne, D;Perkin, J D;Pidcott, C;Pinzon Guerra, E;Playfer, S;Popov, B;Posiadala-Zezula, M;Poutissou, J-M;Pritchard, A;Prouse, N W;Pronost, G;Przewlocki, P;Quilain, B;Quinto, M;Radicioni, E;Ratoff, P N;Retiere, F;Riccio, C;Richards, B;Rondio, E;Rose, H J;Rott, C;Rountree, S D;Ruggeri, A C;Rychter, A;Ryu, D;Sacco, R;Sakuda, M;Sanchez, M C;Scantamburlo, E;Scott, M;Molina Sedgwick, S;Seiya, Y;Sekiguchi, T;Sekiya, H;Seo, H;Seo, S H;Sgalaberna, D;Shah, R;Shaikhiev, A;Shimizu, I;Shiozawa, M;Shitov, Y;Short, S;Simpson, C;Sinnis, G;Smy, M B;Snow, S;Sobczyk, J;Sobel, H W;Son, D C;Sonoda, Y;Spina, R;Stewart, T;Stone, J L;Suda, Y;Suwa, Y;Suzuki, Y;Suzuki, A T;Svoboda, R;Taani, M;Tacik, R;Takeda, A;Takenaka, A;Taketa, A;Takeuchi, Y;Takhistov, V;Tanaka, H A;Tanaka, H K M;Tanaka, H;Terri, R;Thiesse, M;Thompson, L F;Thorpe, M;Tobayama, S;Touramanis, C;Towstego, T;Tsukamoto, T;Tsui, K M;Tzanov, M;Uchida, Y;Vagins, M R;Vasseur, G;Vilela, C;Vogelaar, R B;Walding, J;Walker, J;Ward, M;Wark, D;Wascko, M O;Weber, A;Wendell, R;Wilkes, R J;Wilking, M J;Wilson, J R;Won, E;Xin, T;Yamamoto, K;Yanagisawa, C;Yano, T;Yasuda, O;Yen, S;Yershov, N;Yeum, D N;Yokoyama, M;Yoo, H D;Yoo, J;Yoon, S C;Yoon, T S;Yoshida, T;Yu, I;Yu, M;Zalipska, J;Zaremba, K;Ziembicki, M;Zito, M;Zsoldos, S
2018-01-01
Abstract
Hyper-Kamiokande consists of two identical water-Cherenkov detectors of total 520 kt, with the first one in Japan at 295 km from the J-PARC neutrino beam with 2.5 degrees off-axis angles (OAAs), and the second one possibly in Korea at a later stage. Having the second detector in Korea would benefit almost all areas of neutrino oscillation physics, mainly due to longer baselines. There are several candidate sites in Korea with baselines of 1000-1300 km and OAAs of 1 degrees-3 degrees.We conducted sensitivity studies on neutrino oscillation physics for a second detector, either in Japan (JD x 2) or Korea (JD + KD), and compared the results with a single detector in Japan. Leptonic charge-parity (CP) symmetry violation sensitivity is improved, especially when the CP is non-maximally violated. The larger matter effect at Korean candidate sites significantly enhances sensitivities to non-standard interactions of neutrinos and mass ordering determination. Current studies indicate the best sensitivity is obtained at Mt. Bisul (1088 km baseline, 1.3 degrees OAA). Thanks to a larger (1000 m) overburden than the first detector site, clear improvements to sensitivities for solar and supernova relic neutrino searches are expected.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11589/160090
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Il report seguente simula gli indicatori relativi alla propria produzione scientifica in relazione alle soglie ASN 2023-2025 del proprio SC/SSD. Si ricorda che il superamento dei valori soglia (almeno 2 su 3) è requisito necessario ma non sufficiente al conseguimento dell'abilitazione. La simulazione si basa sui dati IRIS e sugli indicatori bibliometrici alla data indicata e non tiene conto di eventuali periodi di congedo obbligatorio, che in sede di domanda ASN danno diritto a incrementi percentuali dei valori. La simulazione può differire dall'esito di un’eventuale domanda ASN sia per errori di catalogazione e/o dati mancanti in IRIS, sia per la variabilità dei dati bibliometrici nel tempo. Si consideri che Anvur calcola i valori degli indicatori all'ultima data utile per la presentazione delle domande.
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