Prospects for neutrino astrophysics with Hyper-Kamiokande

the Hyper-Kamiokande Collaboration

Prospects for neutrino astrophysics with Hyper-Kamiokande

the Hyper-Kamiokande Collaboration

University of Tokyo
National Centre for Nuclear Research (NCBJ)
TRIUMF
P.N. Lebedev Physical Institute of the Russian Academy of Sciences
Kyoto University
Imperial College London
University of Rome
National University of Kyiv
Instituto de Instrumentaciòn para Imagen Molecular (i3M)
Laboratorio Subterráneo de Canfranc
University of Regina
University of Oxford
Institute for Nuclear Physics
University of Padova
Politecnico di Bari
Ip Paris
Tokyo Institute of Technology
York University
Long Beach VA and University of California
Sorbonne Université
INFN Sezione di Napoli
Université Paris-Saclay
University of Oviedo
University of Victoria
University of Geneva
King's College London
S. N. Bose National Center for Basic Sciences
University of Warwick
University of Salerno
University of Silesia
Warsaw University of Technology
University of Naples Federico II
High Energy Accelerator Research Organization (KEK)
J-PARC Center
University of Liverpool
University of Zaragoza
Department of Biosciences and Bioengineering
Dongshin University
KTH Royal Institute of Technology
Laboratori Nazionali di Legnaro
Universidad Autonoma de Sinaloa
University Santiago de Compostela
Universidad de Guadalajara
Lancaster University
CCLRC Rutherford Appleton Laboratory
Institute for Nuclear Research of the Russian Academy of Sciences
Vishwakarma Institute of Information Technology
Tezpur University
University of Edinburgh
University of Glasgow
Pontifícia Universidade Católica do Rio de Janeiro
Universidad Autónoma de Madrid
CIBERfes
Oskar Klein Centre
Keio University
Miyagi University of Education
University of Campania L. Vanvitelli
Carleton University
Okayama University
Tohoku University
Institute for Theoretical Physics and Modeling
Tokyo University of Science
The University of Sheffield
Nagoya University
The Graduate University for Advanced Studies
University of Winnipeg
Gwangju Institute of Science and Technology
Kyungpook National University
Chonnam National University
Tokyo Metropolitan University
Sungkyunkwan University
Kobe University
Moscow State University
Louisiana State University
Ulsan National Institute of Science and Technology
Charles University
ETH Zurich
Virginia Polytechnic Institute and State University
University of Toronto
Yokohama National University
Indian Institute of Technology Jodhpur
Wroclaw University
Jagiellonian University
Uppsala University
British Columbia Institute of Technology
University of Warsaw
Agh University of Science and Technology Faculty of Computer Science
RWTH Aachen University
Osaka City University
Sezione di Roma
Kyoto Sangyo University
Tecnologico de Monterrey
Korea Institute of Science and Technology

Résultats de recherche: Contribution à un journal › Article de conférence › Revue par des pairs

Résumé

Hyper-Kamiokande is a multi-purpose next generation neutrino experiment. The detector is a two-layered cylindrical shape ultra-pure water tank, with its height of 64 m and diameter of 71 m. The inner detector will be surrounded by tens of thousands of twenty-inch photosensors and multi-PMT modules to detect water Cherenkov radiation due to the charged particles and provide our fiducial volume of 188 kt. This detection technique is established by Kamiokande and Super-Kamiokande. As the successor of these experiments, Hyper-K will be located deep underground, 600 m below Mt. Tochibora at Kamioka in Japan to reduce cosmic-ray backgrounds. Besides our physics program with accelerator neutrino, atmospheric neutrino and proton decay, neutrino astrophysics is an important research topic for Hyper-K. With its fruitful physics research programs, Hyper-K will play a critical role in the next neutrino physics frontier. It will also provide important information via astrophysical neutrino measurements, i.e., solar neutrino, supernova burst neutrinos and supernova relic neutrino. Here, we will discuss the physics potential of Hyper-K neutrino astrophysics.

langue originale	Anglais
Numéro d'article	1193
journal	Proceedings of Science
Volume	395
état	Publié - 18 mars 2022
Evénement	37th International Cosmic Ray Conference, ICRC 2021 - Virtual, Berlin, Allemagne Durée: 12 juil. 2021 → 23 juil. 2021

Contient cette citation

@article{f2066b43054740deb14ffb14d6f09a29,

title = "Prospects for neutrino astrophysics with Hyper-Kamiokande",

abstract = "Hyper-Kamiokande is a multi-purpose next generation neutrino experiment. The detector is a two-layered cylindrical shape ultra-pure water tank, with its height of 64 m and diameter of 71 m. The inner detector will be surrounded by tens of thousands of twenty-inch photosensors and multi-PMT modules to detect water Cherenkov radiation due to the charged particles and provide our fiducial volume of 188 kt. This detection technique is established by Kamiokande and Super-Kamiokande. As the successor of these experiments, Hyper-K will be located deep underground, 600 m below Mt. Tochibora at Kamioka in Japan to reduce cosmic-ray backgrounds. Besides our physics program with accelerator neutrino, atmospheric neutrino and proton decay, neutrino astrophysics is an important research topic for Hyper-K. With its fruitful physics research programs, Hyper-K will play a critical role in the next neutrino physics frontier. It will also provide important information via astrophysical neutrino measurements, i.e., solar neutrino, supernova burst neutrinos and supernova relic neutrino. Here, we will discuss the physics potential of Hyper-K neutrino astrophysics.",

author = "\{the Hyper-Kamiokande Collaboration\} and Takatomi Yano and K. Abe and P. Adrich and H. Aihara and R. Akutsu and I. Alekseev and A. Ali and \{Alj Hakim\}, \{Y. I.\} and F. Ameli and Anthony, \{L. H.V.\} and A. Araya and Y. Asaoka and V. Aushev and F. Ballester and I. Bandac and M. Barbi and G. Barr and M. Batkiewicz-Kwasniak and M. Bellato and V. Berardi and L. Bernard and E. Bernardini and L. Berns and S. Bhadra and J. Bian and A. Blanchet and A. Blondel and A. Boiano and S. Bolognesi and L. Bonavera and N. Booth and S. Bordoni and S. Borjabad and T. Boschi and D. Bose and Boyd, \{S. B.\} and C. Bozza and A. Bravar and C. Bronner and L. Brown and A. Bubak and A. Buchowicz and \{Buizza Avanzini\}, M. and Cafagna, \{F. S.\} and Calabria, \{N. F.\} and Calvo-Mozota, \{J. M.\} and O. Drapier and M. Gonin and P. Paganini and B. Quilain",

note = "Publisher Copyright: {\textcopyright} Copyright owned by the author(s).; 37th International Cosmic Ray Conference, ICRC 2021 ; Conference date: 12-07-2021 Through 23-07-2021",

year = "2022",

month = mar,

day = "18",

language = "English",

volume = "395",

journal = "Proceedings of Science",

issn = "1824-8039",

}

TY - JOUR

T1 - Prospects for neutrino astrophysics with Hyper-Kamiokande

AU - the Hyper-Kamiokande Collaboration

AU - Yano, Takatomi

AU - Abe, K.

AU - Adrich, P.

AU - Aihara, H.

AU - Akutsu, R.

AU - Alekseev, I.

AU - Ali, A.

AU - Alj Hakim, Y. I.

AU - Ameli, F.

AU - Anthony, L. H.V.

AU - Araya, A.

AU - Asaoka, Y.

AU - Aushev, V.

AU - Ballester, F.

AU - Bandac, I.

AU - Barbi, M.

AU - Barr, G.

AU - Batkiewicz-Kwasniak, M.

AU - Bellato, M.

AU - Berardi, V.

AU - Bernard, L.

AU - Bernardini, E.

AU - Berns, L.

AU - Bhadra, S.

AU - Bian, J.

AU - Blanchet, A.

AU - Blondel, A.

AU - Boiano, A.

AU - Bolognesi, S.

AU - Bonavera, L.

AU - Booth, N.

AU - Bordoni, S.

AU - Borjabad, S.

AU - Boschi, T.

AU - Bose, D.

AU - Boyd, S. B.

AU - Bozza, C.

AU - Bravar, A.

AU - Bronner, C.

AU - Brown, L.

AU - Bubak, A.

AU - Buchowicz, A.

AU - Buizza Avanzini, M.

AU - Cafagna, F. S.

AU - Calabria, N. F.

AU - Calvo-Mozota, J. M.

AU - Drapier, O.

AU - Gonin, M.

AU - Paganini, P.

AU - Quilain, B.

PY - 2022/3/18

Y1 - 2022/3/18

N2 - Hyper-Kamiokande is a multi-purpose next generation neutrino experiment. The detector is a two-layered cylindrical shape ultra-pure water tank, with its height of 64 m and diameter of 71 m. The inner detector will be surrounded by tens of thousands of twenty-inch photosensors and multi-PMT modules to detect water Cherenkov radiation due to the charged particles and provide our fiducial volume of 188 kt. This detection technique is established by Kamiokande and Super-Kamiokande. As the successor of these experiments, Hyper-K will be located deep underground, 600 m below Mt. Tochibora at Kamioka in Japan to reduce cosmic-ray backgrounds. Besides our physics program with accelerator neutrino, atmospheric neutrino and proton decay, neutrino astrophysics is an important research topic for Hyper-K. With its fruitful physics research programs, Hyper-K will play a critical role in the next neutrino physics frontier. It will also provide important information via astrophysical neutrino measurements, i.e., solar neutrino, supernova burst neutrinos and supernova relic neutrino. Here, we will discuss the physics potential of Hyper-K neutrino astrophysics.

AB - Hyper-Kamiokande is a multi-purpose next generation neutrino experiment. The detector is a two-layered cylindrical shape ultra-pure water tank, with its height of 64 m and diameter of 71 m. The inner detector will be surrounded by tens of thousands of twenty-inch photosensors and multi-PMT modules to detect water Cherenkov radiation due to the charged particles and provide our fiducial volume of 188 kt. This detection technique is established by Kamiokande and Super-Kamiokande. As the successor of these experiments, Hyper-K will be located deep underground, 600 m below Mt. Tochibora at Kamioka in Japan to reduce cosmic-ray backgrounds. Besides our physics program with accelerator neutrino, atmospheric neutrino and proton decay, neutrino astrophysics is an important research topic for Hyper-K. With its fruitful physics research programs, Hyper-K will play a critical role in the next neutrino physics frontier. It will also provide important information via astrophysical neutrino measurements, i.e., solar neutrino, supernova burst neutrinos and supernova relic neutrino. Here, we will discuss the physics potential of Hyper-K neutrino astrophysics.

M3 - Conference article

AN - SCOPUS:85144593385

SN - 1824-8039

VL - 395

JO - Proceedings of Science

JF - Proceedings of Science

M1 - 1193

T2 - 37th International Cosmic Ray Conference, ICRC 2021

Y2 - 12 July 2021 through 23 July 2021

ER -

Prospects for neutrino astrophysics with Hyper-Kamiokande

Résumé

Empreinte digitale

Contient cette citation