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Related papers: Astroparticle Physics in Hyper-Kamiokande

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Hyper-Kamiokande is a large infrastructure for particle and astroparticle physics being built in Japan and aiming to start operations by the end of 2027 whose objective is to address the most important questions in science today, for…

High Energy Physics - Experiment · Physics 2025-06-23 Kamiokande Collaboration

We investigate the capabilities of upcoming kiloton-scale neutrino detectors, such as Hyper-Kamiokande, in determining the primary cosmic ray spectrum. These detectors provide full-sky coverage and long-term monitoring, unlike traditional…

High Energy Physics - Phenomenology · Physics 2025-05-16 Stephan A. Meighen-Berger , Jayden L. Newstead , Louis E. Strigari

Proposed as part of the next generation of water Cherenkov detectors, Hyper-Kamiokande will have a vastly improved potential in determining leptonic CP violation in neutrino oscillations. Well understood optical diffusers are needed as part…

Instrumentation and Detectors · Physics 2019-04-15 S. Valder

The Hyper-Kamiokande neutrino detector is set to begin construction in 2020, succeeding Super-Kamiokande as the world's largest water Cerenkov detector. Research and development are well underway for an integrated light injection system for…

Instrumentation and Detectors · Physics 2019-04-04 William G. S. Vinning

Hyper-Kamiokande is a proposed next-generation water Cherenkov detector. If a galactic supernova happens, it will deliver a high event rate ($\mathcal{O}(10^5)$ neutrino events in total) as well as event-by-event energy information. Recent…

Instrumentation and Methods for Astrophysics · Physics 2019-08-14 Jost Migenda

If a galactic supernova explosion occurs in the future, it will be critical to rapidly alert the community to the direction of the supernova by utilizing neutrino signals in order to enable the initiation of follow-up optical observations.…

Instrumentation and Methods for Astrophysics · Physics 2024-02-02 Fumi Nakanishi , Shota Izumiyama , Masayuki Harada , Yusuke Koshio

Hyper-Kamiokande (Hyper-K) is a next-generation long baseline neutrino experiment. One of its primary physics goals is to measure neutrino oscillation parameters precisely, including the Dirac CP violating phase. As conventional $\nu_{\mu}$…

High Energy Physics - Experiment · Physics 2025-05-19 T. Mondal , N. W. Prouse , P. de Perio , M. Hartz , D. Bose

Super-Kamiokande is the world's largest water Cherenkov experiment with its 50-kton tank of ultrapure water, recently doped with gadolinium to enhance neutron capture identification. It is a highly versatile, multi-purpose experiment in the…

High Energy Physics - Experiment · Physics 2024-05-14 Andrew D. Santos

Hyper-Kamiokande (Hyper-K) is a proposed next generation underground water Cherenkov (WCh) experiment. The far detector will measure the oscillated neutrino flux from the long-baseline neutrino experiment using 0.6 GeV neutrinos produced by…

Instrumentation and Detectors · Physics 2017-05-01 Greig Cowan , Evangelia Drakopoulou , Matthew Needham , Mahdi Taani

The JHF-Kamioka neutrino project is a second generation long base line neutrino oscillation experiment that probes physics beyond the Standard Model by high precision measurements of the neutrino masses and mixing. A high intensity narrow…

The next generation of proton decay and neutrino experiments, the post-SuperKamiokande detectors as those that will take place in megaton size water tanks, will require very large surfaces of photodetection and a large volume of data. Even…

Super-Kamiokande is a paramount detector for studying atmospheric, astrophysical and accelerator neutrino physics. This work extracts and characterizes the neutrino reconstruction performance of Super-Kamiokande using the public data…

High Energy Physics - Experiment · Physics 2025-05-28 C. Jesús-Valls

Many of the yet unanswered questions in neutrino physics, such as CP violation in the lepton sector or neutrino mass hierarchy, could be answered with higher sensitivity neutrino experiments. New photodetectors based on micro-channel plates…

Instrumentation and Detectors · Physics 2013-10-11 Ioana Anghel

We investigate the precision with which the supernova neutrino spectra can be reconstructed in water Cherenkov detectors, in particular the large scale Hyper-Kamiokande and Super-Kamiokande. To this aim, we consider quasi-thermal neutrino…

High Energy Physics - Phenomenology · Physics 2018-04-25 Andrea Gallo Rosso , Francesco Vissani , Maria Cristina Volpe

A variety of new physics scenarios allow for neutrinos to up-scatter into a heavy neutral lepton state. For a range of couplings and neutrino energies, the heavy neutrino may travel some distance before decaying to visible final states.…

High Energy Physics - Phenomenology · Physics 2022-10-31 Mack Atkinson , Pilar Coloma , Ivan Martinez-Soler , Noemi Rocco , Ian M. Shoemaker

The current focus of the CERN program is the Large Hadron Collider (LHC), however, CERN is engaged in long baseline neutrino physics with the CNGS project and supports T2K as recognized CERN RE13, and for good reasons: a number of observed…

High Energy Physics - Phenomenology · Physics 2009-10-29 A. Rubbia

Neutrino astrophysics offers new perspectives on the Universe investigation: high energy neutrinos, produced by the most energetic phenomena in our Galaxy and in the Universe, carry complementary (if not exclusive) information about the…

High Energy Astrophysical Phenomena · Physics 2010-02-11 T. Chiarusi , M. Spurio

Core-collapse supernovae are among the most magnificent events in the observable universe. They produce many of the chemical elements necessary for life to exist and their remnants -- neutron stars and black holes -- are interesting…

Instrumentation and Methods for Astrophysics · Physics 2021-07-21 Kamiokande Collaboration , K. Abe , P. Adrich , H. Aihara , R. Akutsu , I. Alekseev , A. Ali , F. Ameli , I. Anghel , L. H. V. Anthony , M. Antonova , A. Araya , Y. Asaoka , Y. Ashida , V. Aushev , F. Ballester , I. Bandac , M. Barbi , G. J. Barker , G. Barr , M. Batkiewicz-Kwasniak , M. Bellato , V. Berardi , M. Bergevin , L. Bernard , E. Bernardini , L. Berns , S. Bhadra , J. Bian , A. Blanchet , F. d. M. Blaszczyk , A. Blondel , A. Boiano , S. Bolognesi , L. Bonavera , N. Booth , S. Borjabad , T. Boschi , D. Bose , S . B. Boyd , C. Bozza , A. Bravar , D. Bravo-Berguño , C. Bronner , L. Brown , A. Bubak , A. Buchowicz , M. Buizza Avanzini , F. S. Cafagna , N. F. Calabria , J. M. Calvo-Mozota , S. Cao , S. L. Cartwright , A. Carroll , M. G. Catanesi , S. Cebriàn , M. Chabera , S. Chakraborty , C. Checchia , J. H. Choi , S. Choubey , M. Cicerchia , J. Coleman , G. Collazuol , L. Cook , G. Cowan , S. Cuen-Rochin , M. Danilov , G. Daz Lopez , E. De la Fuente , P. de Perio , G. De Rosa , T. Dealtry , C. J. Densham , A. Dergacheva , N. Deshmukh , M. M. Devi , F. Di Lodovico , P. Di Meo , I. Di Palma , T. A. Doyle , E. Drakopoulou , O. Drapier , J. Dumarchez , P. Dunne , M. Dziewiecki , L. Eklund , S. El Hedri , J. Ellis , S. Emery , A. Esmaili , R. Esteve , A. Evangelisti , M. Feely , S. Fedotov , J. Feng , P. Fernandez , E. Fernández-Martinez , P. Ferrario , B. Ferrazzi , T. Feusels , A. Finch , C. Finley , A. Fiorentini , G. Fiorillo , M. Fitton , K. Frankiewicz , M. Friend , Y. Fujii , Y. Fukuda , G. Galinski , J. Gao , C. Garde , A. Garfagnini , S. Garode , L. Gialanella , C. Giganti , J. J. Gomez-Cadenas , M. Gonin , J. González-Nuevo , A. Gorin , R. Gornea , V. Gousy-Leblanc , F. Gramegna , M. Grassi , G. Grella , M. Guigue , P. Gumplinger , D. R. Hadley , M. Harada , B. Hartfiel , M. Hartz , S. Hassani , N. C. Hastings , Y. Hayato , J. A. Hernando-Morata , V. Herrero , J. Hill , K. Hiraide , S. Hirota , A. Holin , S. Horiuchi , K. Hoshina , K. Hultqvist , F. Iacob , A. K. Ichikawa , W. Idrissi Ibnsalih , T. Iijima , M. Ikeda , M. Inomoto , K. Inoue , J. Insler , A. Ioannisian , T. Ishida , K. Ishidoshiro , H. Ishino , M. Ishitsuka , H. Ito , S. Ito , Y. Itow , K. Iwamoto , A. Izmaylov , N. Izumi , S. Izumiyama , M. Jakkapu , B. Jamieson , H. I. Jang , J. S. Jang , S. J. Jenkins , S. H. Jeon , M. Jiang , H. S. Jo , P. Jonsson , K. K. Joo , T. Kajita , H. Kakuno , J. Kameda , Y. Kano , P. Kalaczynski , D. Karlen , J. Kasperek , Y. Kataoka , A. Kato , T. Katori , N. Kazarian , E. Kearns , M. Khabibullin , A. Khotjantsev , T. Kikawa , M. Kikec , J. H. Kim , J. Y. Kim , S. B. Kim , S. Y. Kim , S. King , T. Kinoshita , J. Kisiel , A. Klekotko , T. Kobayashi , L. Koch , M. Koga , L. Koerich , N. Kolev , A. Konaka , L. L. Kormos , Y. Koshio , A. Korzenev , Y. Kotsar , K. A. Kouzakov , K. L. Kowalik , L. Kravchuk , A. P. Kryukov , Y. Kudenko , T. Kumita , R. Kurjata , T. Kutter , M. Kuze , K. Kwak , M. La Commara , L. Labarga , J. Lagoda , M. Lamers James , M. Lamoureux , M. Laveder , L. Lavitola , M. Lawe , J. G. Learned , J. Lee , R. Leitner , V. Lezaun , I. T. Lim , T. Lindner , R. P. Litchfield , K. R. Long , A. Longhin , P. Loverre , X. Lu , L. Ludovici , Y. Maekawa , L. Magaletti , K. Magar , K. Mahn , Y. Makida , M. Malek , M. Malinský , T. Marchi , L. Maret , C. Mariani , A. Marinelli , K. Martens , Ll. Marti , J. F. Martin , D. Martin , J. Marzec , T. Matsubara , R. Matsumoto , S. Matsuno , M. Matusiak , E. Mazzucato , M. McCarthy , N. McCauley , J. McElwee , C. McGrew , A. Mefodiev , A. Medhi , P. Mehta , L. Mellet , H. Menjo , P. Mermod , C. Metelko , M. Mezzetto , J. Migenda , P. Migliozzi , P. Mijakowski , S. Miki , E. W. Miller , H. Minakata , A. Minamino , S. Mine , O. Mineev , A. Mitra , M. Miura , R. Moharana , C. M. Mollo , T. Mondal , M. Mongelli , F. Monrabal , D. H. Moon , C. S. Moon , F. J. Mora , S. Moriyama , Th. A. Mueller , L. Munteanu , K. Murase , Y. Nagao , T. Nakadaira , K. Nakagiri , M. Nakahata , S. Nakai , Y. Nakajima , K. Nakamura , KI. Nakamura , H. Nakamura , Y. Nakano , T. Nakaya , S. Nakayama , K. Nakayoshi , L. Nascimento Machado , C. E. R. Naseby , B. Navarro-Garcia , M. Needham , T. Nicholls , K. Niewczas , Y. Nishimura , E. Noah , F. Nova , J. C. Nugent , H. Nunokawa , W. Obrebski , J. P. Ochoa-Ricoux , E. O'Connor , N. Ogawa , T. Ogitsu , K. Ohta , K. Okamoto , H. M. O'Keeffe , K. Okumura , Y. Onishchuk , F. Orozco-Luna , A. Oshlianskyi , N. Ospina , M. Ostrowski , E. O'Sullivan , L. O'Sullivan , T. Ovsiannikova , Y. Oyama , H. Ozaki , M. Y. Pac , P. Paganini , V. Palladino , V. Paolone , M. Pari , S. Parsa , J. Pasternak , C. Pastore , G. Pastuszak , D. A. Patel , M. Pavin , D. Payne , C. Peña-Garay , C. Pidcott , E. Pinzon Guerra , S. Playfer , B. W. Pointon , A. Popov , B. Popov , K. Porwit , M. Posiadala-Zezula , J. -M. Poutissou , J. Pozimski , G. Pronost , N. W. Prouse , P. Przewlocki , B. Quilain , A. A. Quiroga , E. Radicioni , B. Radics , P. J. Rajda , J. Renner , M. Rescigno , F. Retiere , G. Ricciardi , C. Riccio , B. Richards , E. Rondio , H. J. Rose , B. Roskovec , S. Roth , C. Rott , S. D. Rountree , A. Rubbia , A. C. Ruggeri , C. Ruggles , S. Russo , A. Rychter , D. Ryu , K. Sakashita , S. Samani , F. Sánchez , M. L. Sánchez , M. C. Sanchez , S. Sano , J. D. Santos , G. Santucci , P. Sarmah , I. Sashima , K. Sato , M. Scott , Y. Seiya , T. Sekiguchi , H. Sekiya , J. W. Seo , S. H. Seo , D. Sgalaberna , A. Shaikhiev , Z. Shan , A. Shaykina , I. Shimizu , C. D. Shin , M. Shinoki , M. Shiozawa , G. Sinnis , N. Skrobova , K. Skwarczynski , M. B. Smy , J. Sobczyk , H. W. Sobel , F. J. P. Soler , Y. Sonoda , R. Spina , B. Spisso , P. Spradlin , K. L. Stankevich , L. Stawarz , S. M. Stellacci , K. Stopa , A. I. Studenikin , S. L. Suárez Gómez , T. Suganuma , S. Suvorov , Y. Suwa , A. T. Suzuki , S. Y. Suzuki , Y. Suzuki , D. Svirida , R. Svoboda , M. Taani , M. Tada , A. Takeda , Y. Takemoto , A. Takenaka , A. Taketa , Y. Takeuchi , V. Takhistov , H. Tanaka , H. A. Tanaka , H. I. Tanaka , M. Tanaka , T. Tashiro , M. Thiesse , L. F. Thompson , J. Toledo , A. K. Tomatani-Sánchez , G. Tortone , K. M. Tsui , T. Tsukamoto , M. Tzanov , Y. Uchida , M. R. Vagins , S. Valder , V. Valentino , G. Vasseur , A. Vijayvargi , C. Vilela , W. G. S. Vinning , D. Vivolo , T. Vladisavljevic , R. B. Vogelaar , M. M. Vyalkov , T. Wachala , J. Walker , D. Wark , M. O. Wascko , R. A. Wendell , R. J. Wilkes , M. J. Wilking , J. R. Wilson , S. Wronka , J. Xia , Z. Xie , T. Xin , Y. Yamaguchi , K. Yamamoto , C. Yanagisawa , T. Yano , S. Yen , N. Yershov , D. N. Yeum , M. Yokoyama , M. Yonenaga , J. Yoo , I. Yu , M. Yu , T. Zakrzewski , B. Zaldivar , J. Zalipska , K. Zaremba , G. Zarnecki , M. Ziembicki , K. Zietara , M. Zito , S. Zsoldos

Supernovae are among the most magnificent events in the observable universe. They produce many of the chemical elements necessary for life to exist and their remnants---neutron stars and black holes---are interesting astrophysical objects…

Instrumentation and Methods for Astrophysics · Physics 2020-02-06 Jost Migenda

After two decades of measurements, neutrino physics is now advancing into the precision era. Withthe long-baseline experiments designed to tackle current open questions, a new query arises: can atmospheric neutrino experiments also play a…

High Energy Physics - Phenomenology · Physics 2024-01-22 C. A. Argüelles , P. Fernández , I. Martínez-Soler , M. Jin