Physics potentials with the second Hyper-Kamiokande detector in Korea
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Published version
Author(s)
Type
Journal Article
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∘ 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.
.
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.
Date Issued
2018-06-01
Date Acceptance
2018-03-16
Citation
Progress of Theoretical and Experimental Physics, 2018, 2018 (6)
ISSN
2050-3911
Publisher
Oxford University Press (OUP)
Journal / Book Title
Progress of Theoretical and Experimental Physics
Volume
2018
Issue
6
Copyright Statement
© The Author(s) 2018. Published by Oxford University Press on behalf of the Physical Society of Japan.
This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited.Funded by SCOAP3
This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited.Funded by SCOAP3
Sponsor
Science and Technology Facilities Council (STFC)
Identifier
http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000438300800001&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=1ba7043ffcc86c417c072aa74d649202
Grant Number
ST/M002691/1
Subjects
Science & Technology
Physical Sciences
Physics, Multidisciplinary
Physics, Particles & Fields
Physics
NEUTRINO OSCILLATION EXPERIMENTS
LINE-EXPERIMENT-SIMULATOR
CP VIOLATION
MATTER
SPECTROSCOPY
MUSIC
EARTH
CODE
Publication Status
Published
Article Number
ARTN 063C01
Date Publish Online
2018-06-20