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We first briefly describe the history and motivation behind Cherenkov and scintillation light detection. We then discuss the instrumentation needed to detect these photons as it applies to both photodetectors and readout electronics. One of…

Instrumentation and Detectors · Physics 2025-12-01 V. A. Li , O. A. Akindele , M. Bondin , S. R. Durham , J. A. Foot , M. J. Ford , S. -W. Stradleigh

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…

A number of exciting concepts are under development for Flagship, Probe class, Explorer class, and Suborbital class NASA missions in the ultraviolet/optical spectral ranges. These missions will depend on high performance silicon detector…

A completely new under-water dark-room test facility (UWDTF) has been built at the University of Winnipeg during 2021-2023, for the testing of the equipments, optical components and detectors before they might be used in different…

The construction of the Cherenkov Telescope Array is expected to start soon. We will present the baseline methods and their extensions currently foreseen to calibrate the observatory. These are bound to achieve the strong requirements on…

Instrumentation and Methods for Astrophysics · Physics 2019-08-14 Markus Gaug , Michael Daniel , David Berge , Raquel de los Reyes , Michele Doro , Andreas Foerster , Maria Concetta Maccarone , Dan Parsons , Christopher van Eldik

A long-baseline neutrino-oscillation experiment using a well-defined neutrino beam is in preparation at KEK. Neutrinos generated at KEK will be detected by the Super-kamiokande detector 250 km away. The design of the neutrino beam line,…

High Energy Physics - Experiment · Physics 2009-09-25 Yuichi Oyama

The Universe is awash with tens-of-MeV neutrinos of all species coming from all past core-collapse supernovae. These have never been observed, but this state of affairs will change in the near future. In the less than ten years, the…

High Energy Physics - Phenomenology · Physics 2021-01-04 André de Gouvêa , Ivan Martinez-Soler , Yuber F. Perez-Gonzalez , Manibrata Sen

We present the latest Hyper-Kamiokande sensitivity study showing that, with a total exposure of 13 MW $\times 10^{7}$ seconds integrated beam power, the CP phase - $\delta_{CP}$ - can be determined better than 21 degrees for all possible…

High Energy Physics - Experiment · Physics 2016-08-23 S. Bron

While neutrino physics enters precision era, several important unknowns remain. Atmospheric neutrinos allow to simultaneously test key oscillation parameters, with Super-Kamiokande experiment playing a central role. We discuss results from…

High Energy Physics - Experiment · Physics 2020-12-15 Volodymyr Takhistov

Measurement technology employing optical interference phenomena such as a fringe pattern or frequency shift has been evolving for more than a century. The systems are being designed better, and their components are being built better. But…

The addition of certain solutes to a water Cerenkov detector will introduce new charge-current channels for the detection of $\nu_e$s. The experimental conditions necessary to exploit such signals - large volumes and very low backgrounds -…

Nuclear Theory · Physics 2010-11-24 W. C. Haxton

Our knowledge of neutrino cross sections at the GeV scale, instrumental to test CP symmetry violation in the leptonic sector, has grown substantially in the last two decades. Still, their precision and understanding are far from the…

High Energy Physics - Experiment · Physics 2021-08-30 A. Branca , G. Brunetti , A. Longhin , M. Martini , F. Pupilli , F. Terranova

A new event reconstruction algorithm based on a maximum likelihood method has been developed for Super-Kamiokande. Its improved kinematic and particle identification capabilities enable the analysis of atmospheric neutrino data in a…

High Energy Physics - Experiment · Physics 2019-12-06 Kamiokande Collaboration , M. Jiang , K. Abe , C. Bronner , Y. Hayato , M. Ikeda , K. Iyogi , J. Kameda , Y. Kato , Y. Kishimoto , Ll. Marti , M. Miura , S. Moriyama , T. Mochizuki , M. Nakahata , Y. Nakajima , Y. Nakano , S. Nakayama , T. Okada , K. Okamoto , A. Orii , G. Pronost , H. Sekiya , M. Shiozawa , Y. Sonoda , A. Takeda , A. Takenaka , H. Tanaka , T. Yano , R. Akutsu , T. Kajita , Y. Nishimura , K. Okumura , R. Wang , J. Xia , L. Labarga , P. Fernandez , F. d. M. Blaszczyk , C. Kachulis , E. Kearns , J. L. Raaf , J. L. Stone , S. Sussman , S. Berkman , J. Bian , N. J. Griskevich , W. R. Kropp , S. Locke , S. Mine , P. Weatherly , M. B. Smy , H. W. Sobel , V. Takhistov , K. S. Ganezer , J. Hill , J. Y. Kim , I. T. Lim , R. G. Park , B. Bodur , K. Scholberg , C. W. Walter , O. Drapier , M. Gonin , J. Imber , Th. A. Mueller , P. Paganini , T. Ishizuka , T. Nakamura , J. S. Jang , K. Choi , J. G. Learned , S. Matsuno , R. P. Litchfield , A. A. Sztuc , Y. Uchida , M. O. Wascko , N. F. Calabria , M. G. Catanesi , R. A. Intonti , E. Radicioni , G. De Rosa , A. Ali , G. Collazuol , F. Iacob , L. Ludovici , S. Cao , M. Friend , T. Hasegawa , T. Ishida , T. Kobayashi , T. Nakadaira , K. Nakamura , Y. Oyama , K. Sakashita , T. Sekiguchi , T. Tsukamoto , KE. Abe , M. Hasegawa , Y. Isobe , H. Miyabe , T. Sugimoto , A. T. Suzuki , Y. Takeuchi , Y. Ashida , T. Hayashino , S. Hirota , T. Kikawa , M. Mori , KE. Nakamura , T. Nakaya , R. A. Wendell , L. H. V. Anthony , N. McCauley , A. Pritchard , K. M. Tsui , Y. Fukuda , Y. Itow , M. Murrase , P. Mijakowski , K. Frankiewicz , C. K. Jung , X. Li , J. L. Palomino , G. Santucci , C. Vilela , M. J. Wilking , C. Yanagisawa , D. Fukuda , K. Hagiwara , H. Ishino , S. Ito , Y. Koshio , M. Sakuda , Y. Takahira , C. Xu , Y. Kuno , C. Simpson , D. Wark , F. Di Lodovico , B. Richards , S. Molina Sedgwick , R. Tacik , S. B. Kim , M. Thiesse , L. Thompson , H. Okazawa , Y. Choi , K. Nishijima , M. Koshiba , M. Yokoyama , A. Goldsack , K. Martens , M. Murdoch , B. Quilain , Y. Suzuki , M. R. Vagins , M. Kuze , Y. Okajima , T. Yoshida , M. Ishitsuka , J. F. Martin , C. M. Nantais , H. A. Tanaka , T. Towstego , M. Hartz , A. Konaka , P. de Perio , S. Chen , L. Wan , A. Minamino

The optical properties of the Sudbury Neutrino Observatory (SNO) heavy water Cherenkov neutrino detector are measured in situ using a light diffusing sphere ("laserball"). This diffuser is connected to a pulsed nitrogen/dye laser via…

The time-integrated luminosity and average energy of the neutrino emission spectrum are essential diagnostics of core-collapse supernovae. The SN 1987A electron antineutrino observations by the Kamiokande-II and IMB detectors are only…

Astrophysics · Physics 2007-05-23 Hasan Yuksel , Shin'ichiro Ando , John Beacom

We review photodetectors used in present running neutrino telescopes. After a brief historical discourse, the photodetector requirements for the next generation deep underwater neutrino telescopes are discussed. It is shown that large area…

Instrumentation and Detectors · Physics 2010-11-30 B. K. Lubsandorzhiev

In this paper we describe the current status of the CALDER project, which is developing ultra-sensitive light detectors based on superconductors for cryogenic applications. When we apply an AC current to a superconductor, the Cooper pairs…

Recent neutrino oscillation results have shown that the existing long baseline experiments have some sensitivity to the effects of CP violation in the neutrino sector. This sensitivity is currently statistically limited, but the next…

Instrumentation and Detectors · Physics 2019-08-21 Mark Scott

Optical imaging systems are widely used in the drone industry (optical navigation, terrain scanners), industry (distance measurement, 3D visualization), security (optical scanners and motion sensors), robotics (motion sensors, terrain or…

Instrumentation and Detectors · Physics 2022-08-10 K. Khuseynzada , A. Sadigov , J. Naghiyev , F. Ahmadov , G. Ahmadov

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