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@article{Abe:2018:ptep/pty044,
author = {Abe, K and Abe, K and Ahn, SH and Aihara, H and Aimi, A and Akutsu, R and Andreopoulos, C and Anghel, I and Anthony, LHV and Antonova, M and Ashida, Y and Aushev, V and Barbi, M and Barker, GJ and Barr, G and Beltrame, P and Berardi, V and Bergevin, M and Berkman, S and Berns, L and Berry, T and Bhadra, S and Blaszczyk, FDM and Blondel, A and Bolognesi, S and Boyd, SB and Bravar, A and Bronner, C and Avanzini, MB and Cafagna, FS and Calland, R and Cao, S and Cartwright, SL and Catanesi, MG and Checchia, C and Chen-Wishart, Z and Cheon, BG and Cheoun, MK and Cho, K and Choi, JH and Choi, K and Choi, KY and Chun, EJ and Cole, A and Coleman, J and Collazuol, G and Cowan, G and Cremonesi, L and Dealtry, T and De, Rosa G and Densham, C and Dewhurst, D and Drakopoulou, E and Di, Lodovico F and Drapier, O and Dumarchez, J and Dunne, P and Dziewiecki, M and Emery, S and Esmaili, A and Evangelisti, A and Fernandez-Martinez, E and Feusels, T and Finch, A and Fiorentini, GA and Fiorillo, G and Fi},
doi = {ptep/pty044},
journal = {Progress of Theoretical and Experimental Physics},
title = {Physics potentials with the second Hyper-Kamiokande detector in Korea},
url = {http://dx.doi.org/10.1093/ptep/pty044},
volume = {2018},
year = {2018}
}

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TY  - JOUR
AB  - 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 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 1–3.We conducted sensitivity studies on neutrino oscillation physics for a second detector, either in Japan (JD ×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 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.
AU  - Abe,K
AU  - Abe,K
AU  - Ahn,SH
AU  - Aihara,H
AU  - Aimi,A
AU  - Akutsu,R
AU  - Andreopoulos,C
AU  - Anghel,I
AU  - Anthony,LHV
AU  - Antonova,M
AU  - Ashida,Y
AU  - Aushev,V
AU  - Barbi,M
AU  - Barker,GJ
AU  - Barr,G
AU  - Beltrame,P
AU  - Berardi,V
AU  - Bergevin,M
AU  - Berkman,S
AU  - Berns,L
AU  - Berry,T
AU  - Bhadra,S
AU  - Blaszczyk,FDM
AU  - Blondel,A
AU  - Bolognesi,S
AU  - Boyd,SB
AU  - Bravar,A
AU  - Bronner,C
AU  - Avanzini,MB
AU  - Cafagna,FS
AU  - Calland,R
AU  - Cao,S
AU  - Cartwright,SL
AU  - Catanesi,MG
AU  - Checchia,C
AU  - Chen-Wishart,Z
AU  - Cheon,BG
AU  - Cheoun,MK
AU  - Cho,K
AU  - Choi,JH
AU  - Choi,K
AU  - Choi,KY
AU  - Chun,EJ
AU  - Cole,A
AU  - Coleman,J
AU  - Collazuol,G
AU  - Cowan,G
AU  - Cremonesi,L
AU  - Dealtry,T
AU  - De,Rosa G
AU  - Densham,C
AU  - Dewhurst,D
AU  - Drakopoulou,E
AU  - Di,Lodovico F
AU  - Drapier,O
AU  - Dumarchez,J
AU  - Dunne,P
AU  - Dziewiecki,M
AU  - Emery,S
AU  - Esmaili,A
AU  - Evangelisti,A
AU  - Fernandez-Martinez,E
AU  - Feusels,T
AU  - Finch,A
AU  - Fiorentini,GA
AU  - Fiorillo,G
AU  - Fitton,M
AU  - Frankiewicz,K
AU  - Friend,M
AU  - Fujii,Y
AU  - Fukuda,Y
AU  - Fukuda,D
AU  - Ganezer,K
AU  - Ghosh,M
AU  - Giganti,C
AU  - Gonin,M
AU  - Grant,N
AU  - Gumplinger,P
AU  - Hadley,DR
AU  - Hartfiel,B
AU  - Hartz,M
AU  - Hayato,Y
AU  - Hayrapetyan,K
AU  - Hill,J
AU  - Hirota,S
AU  - Horiuchi,S
AU  - Ichikawa,AK
AU  - Iijima,T
AU  - Ikeda,M
AU  - Imber,J
AU  - Inoue,K
AU  - Insler,J
AU  - Intonti,RA
AU  - Ioannisian,A
AU  - Ishida,T
AU  - Ishino,H
AU  - Ishitsuka,M
AU  - Itow,Y
AU  - Iwamoto,K
AU  - Izmaylov,A
AU  - Jamieson,B
AU  - Jang,HI
AU  - Jang,JS
AU  - Jeon,SH
AU  - Jeong,KS
AU  - Jiang,M
AU  - Jonsson,P
AU  - Joo,KK
AU  - Kaboth,A
AU  - Kachulis,C
AU  - Kajita,T
AU  - Kang,SK
AU  - Kameda,J
AU  - Kataoka,Y
AU  - Katori,T
AU  - Kayrapetyan,K
AU  - Kearns,E
AU  - Khabibullin,M
AU  - Khotjantsev,A
AU  - Kim,CS
AU  - Kim,HB
AU  - Kim,HJ
AU  - Kim,JH
AU  - Kim,J-S
AU  - Kim,JY
AU  - Kim,SB
AU  - Kim,SC
AU  - Kim,S-W
AU  - Kim,SY
AU  - Kim,TJ
AU  - Kim,W
AU  - King,S
AU  - Kishimoto,Y
AU  - Ko,P
AU  - Kobayashi,T
AU  - Koga,M
AU  - Konaka,A
AU  - Kormos,LL
AU  - Koshio,Y
AU  - Korzenev,A
AU  - Kowalik,KL
AU  - Kropp,WR
AU  - Kudenko,Y
AU  - Kurjata,R
AU  - Kutter,T
AU  - Kuze,M
AU  - Kwak,K
AU  - Kwon,EH
AU  - Labarga,L
AU  - Lagoda,J
AU  - Lasorak,PJJ
AU  - Laveder,M
AU  - Lawe,M
AU  - Learned,JG
AU  - Lee,CH
AU  - Lee,SJ
AU  - Lee,WJ
AU  - Lim,IT
AU  - Lindner,T
AU  - Litchfield,RP
AU  - Longhin,A
AU  - Loverre,P
AU  - Lou,T
AU  - Ludovici,L
AU  - Ma,W
AU  - Magaletti,L
AU  - Mahn,K
AU  - Malek,M
AU  - Maret,L
AU  - Mariani,C
AU  - Martens,K
AU  - Marti,L
AU  - Martin,JF
AU  - Marzec,J
AU  - Matsuno,S
AU  - Mazzucato,E
AU  - McCarthy,M
AU  - McCauley,N
AU  - McFarland,KS
AU  - McGrew,C
AU  - Mefodiev,A
AU  - Mermod,P
AU  - Metelko,C
AU  - Mezzetto,M
AU  - Migenda,J
AU  - Mijakowski,P
AU  - Minakata,H
AU  - Minamino,A
AU  - Mine
DO  - ptep/pty044
PY  - 2018///
SN  - 2050-3911
TI  - Physics potentials with the second Hyper-Kamiokande detector in Korea
T2  - Progress of Theoretical and Experimental Physics
UR  - http://dx.doi.org/10.1093/ptep/pty044
UR  - http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000438300800001&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=1ba7043ffcc86c417c072aa74d649202
UR  - http://hdl.handle.net/10044/1/74893
VL  - 2018
ER  -

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