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author Andreopoulos, C
Barbato, FCT
Barker, G
Barr, G
Beltrame, P
Berardi, V
Berry, T
Blondel, A
Boyd, S
Bravar, A
Cafagna, FS
Cartwright, S
Catanesi, MG
Checchia, C
Cole, A
Collazuol, G
Cowan, GA
Davenne, T
Dealtry, T
Densham, C
Rosa, GD
Lodovico, FD
Drakopoulou, E
Dunne, P
Finch, A
Fitton, M
Hadley, D
Hayrapetyan, K
Intonti, RA
Jonsson, P
Kaboth, A
Katori, T
Kormos, L
Kudenko, Y
Lagoda, J
Lasorak, P
Laveder, M
Lawe, M
Litchfield, P
Longhin, A
Ludovici, L
Ma, W
Magaletti, L
Malek, M
McCauley, N
Mezzetto, M
Monroe, J
Nicholls, T
Needham, M
Noah, E
Nova, F
O'Keeffe, HM
Owen, A
Palladino, V
Payne, D
Perkin, J
Playfer, S
Pritchard, A
Prouse, N
Radicioni, E
Rayner, M
Riccio, C
Richards, B
Rose, J
Ruggeri, AC
Shah, R
Shitov, Y
Simpson, C
Sidiropoulos, G
Stewart, T
Terri, R
Thompson, L
Thorpe, M
Uchida, Y
Wark, D
Wascko, MO
Weber, A
Wilson, JR
author_facet Andreopoulos, C
Barbato, FCT
Barker, G
Barr, G
Beltrame, P
Berardi, V
Berry, T
Blondel, A
Boyd, S
Bravar, A
Cafagna, FS
Cartwright, S
Catanesi, MG
Checchia, C
Cole, A
Collazuol, G
Cowan, GA
Davenne, T
Dealtry, T
Densham, C
Rosa, GD
Lodovico, FD
Drakopoulou, E
Dunne, P
Finch, A
Fitton, M
Hadley, D
Hayrapetyan, K
Intonti, RA
Jonsson, P
Kaboth, A
Katori, T
Kormos, L
Kudenko, Y
Lagoda, J
Lasorak, P
Laveder, M
Lawe, M
Litchfield, P
Longhin, A
Ludovici, L
Ma, W
Magaletti, L
Malek, M
McCauley, N
Mezzetto, M
Monroe, J
Nicholls, T
Needham, M
Noah, E
Nova, F
O'Keeffe, HM
Owen, A
Palladino, V
Payne, D
Perkin, J
Playfer, S
Pritchard, A
Prouse, N
Radicioni, E
Rayner, M
Riccio, C
Richards, B
Rose, J
Ruggeri, AC
Shah, R
Shitov, Y
Simpson, C
Sidiropoulos, G
Stewart, T
Terri, R
Thompson, L
Thorpe, M
Uchida, Y
Wark, D
Wascko, MO
Weber, A
Wilson, JR
author_sort Andreopoulos, C
collection OXFORD
description The TITUS, Tokai Intermediate Tank for Unoscillated Spectrum, detector, is a proposed Gd-doped Water Cherenkov tank with a magnetised muon range detector downstream. It is located at J-PARC at about 2 km from the neutrino target and it is proposed as a potential near detector for the Hyper-Kamiokande experiment. Assuming a beam power of 1.3 MW and 27.05 x 10^{21} protons-on-target the sensitivity to CP and mixing parameters achieved by Hyper-Kamiokande with TITUS as a near detector is presented. Also, the potential of the detector for cross sections and Standard Model parameter determination, supernova neutrino and dark matter are shown.
first_indexed 2024-03-07T02:39:39Z
format Journal article
id oxford-uuid:a9fefdf7-5683-4524-aed6-aec59967af5a
institution University of Oxford
last_indexed 2024-03-07T02:39:39Z
publishDate 2018
record_format dspace
spelling oxford-uuid:a9fefdf7-5683-4524-aed6-aec59967af5a2022-03-27T03:12:26ZTITUS: the Tokai Intermediate Tank for the Unoscillated SpectrumJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:a9fefdf7-5683-4524-aed6-aec59967af5aSymplectic Elements at Oxford2018Andreopoulos, CBarbato, FCTBarker, GBarr, GBeltrame, PBerardi, VBerry, TBlondel, ABoyd, SBravar, ACafagna, FSCartwright, SCatanesi, MGChecchia, CCole, ACollazuol, GCowan, GADavenne, TDealtry, TDensham, CRosa, GDLodovico, FDDrakopoulou, EDunne, PFinch, AFitton, MHadley, DHayrapetyan, KIntonti, RAJonsson, PKaboth, AKatori, TKormos, LKudenko, YLagoda, JLasorak, PLaveder, MLawe, MLitchfield, PLonghin, ALudovici, LMa, WMagaletti, LMalek, MMcCauley, NMezzetto, MMonroe, JNicholls, TNeedham, MNoah, ENova, FO'Keeffe, HMOwen, APalladino, VPayne, DPerkin, JPlayfer, SPritchard, AProuse, NRadicioni, ERayner, MRiccio, CRichards, BRose, JRuggeri, ACShah, RShitov, YSimpson, CSidiropoulos, GStewart, TTerri, RThompson, LThorpe, MUchida, YWark, DWascko, MOWeber, AWilson, JRThe TITUS, Tokai Intermediate Tank for Unoscillated Spectrum, detector, is a proposed Gd-doped Water Cherenkov tank with a magnetised muon range detector downstream. It is located at J-PARC at about 2 km from the neutrino target and it is proposed as a potential near detector for the Hyper-Kamiokande experiment. Assuming a beam power of 1.3 MW and 27.05 x 10^{21} protons-on-target the sensitivity to CP and mixing parameters achieved by Hyper-Kamiokande with TITUS as a near detector is presented. Also, the potential of the detector for cross sections and Standard Model parameter determination, supernova neutrino and dark matter are shown.
spellingShingle Andreopoulos, C
Barbato, FCT
Barker, G
Barr, G
Beltrame, P
Berardi, V
Berry, T
Blondel, A
Boyd, S
Bravar, A
Cafagna, FS
Cartwright, S
Catanesi, MG
Checchia, C
Cole, A
Collazuol, G
Cowan, GA
Davenne, T
Dealtry, T
Densham, C
Rosa, GD
Lodovico, FD
Drakopoulou, E
Dunne, P
Finch, A
Fitton, M
Hadley, D
Hayrapetyan, K
Intonti, RA
Jonsson, P
Kaboth, A
Katori, T
Kormos, L
Kudenko, Y
Lagoda, J
Lasorak, P
Laveder, M
Lawe, M
Litchfield, P
Longhin, A
Ludovici, L
Ma, W
Magaletti, L
Malek, M
McCauley, N
Mezzetto, M
Monroe, J
Nicholls, T
Needham, M
Noah, E
Nova, F
O'Keeffe, HM
Owen, A
Palladino, V
Payne, D
Perkin, J
Playfer, S
Pritchard, A
Prouse, N
Radicioni, E
Rayner, M
Riccio, C
Richards, B
Rose, J
Ruggeri, AC
Shah, R
Shitov, Y
Simpson, C
Sidiropoulos, G
Stewart, T
Terri, R
Thompson, L
Thorpe, M
Uchida, Y
Wark, D
Wascko, MO
Weber, A
Wilson, JR
TITUS: the Tokai Intermediate Tank for the Unoscillated Spectrum
title TITUS: the Tokai Intermediate Tank for the Unoscillated Spectrum
title_full TITUS: the Tokai Intermediate Tank for the Unoscillated Spectrum
title_fullStr TITUS: the Tokai Intermediate Tank for the Unoscillated Spectrum
title_full_unstemmed TITUS: the Tokai Intermediate Tank for the Unoscillated Spectrum
title_short TITUS: the Tokai Intermediate Tank for the Unoscillated Spectrum
title_sort titus the tokai intermediate tank for the unoscillated spectrum
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