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Related papers: Progress on Cherenkov Reconstruction in MICE

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Cosmic rays interacting with the Earth's atmosphere generate extensive air showers, which produce Cherenkov, fluorescence and radio emissions. These emissions are key signatures for detection by ground-based, sub-orbital, and…

High Energy Astrophysical Phenomena · Physics 2025-10-07 Diksha Garg , Laksha Pradip Das , Mary Hall Reno

The pion-production target that serves the MICE Muon Beam consists of a titanium cylinder that is dipped into the halo of the ISIS proton beam. The design and construction of the MICE target system are described along with the…

The IceCube Neutrino Observatory, located at the geographic South Pole, uses the glacial ice volume to detect astrophysical neutrinos. Detection of the neutrinos from the northern sky provides the opportunity to use a large effective…

High Energy Astrophysical Phenomena · Physics 2025-07-11 Najia Moureen Binte Amin , David Seckel

This paper presents several approaches to deal with the problem of identifying muons in a water Cherenkov detector with a reduced water volume and 4 PMTs. Different perspectives of information representation are used and new features are…

Instrumentation and Detectors · Physics 2021-01-29 B. S. González , R. Conceição , M. Pimenta , B. Tomé , A. Guillén

We report on the construction, operation, and performance of the Time-of-Propagation detector with imaging used for the Belle II experiment running at the Super-KEKB $e^+e^-$ collider. This detector is located in the central barrel region…

Cosmic ray muons present a large part of the radiation background and depending on the application of interest muons can be seen as background noise, e.g., radiation mapping, radiation protection, dosimetry, or as a useful interrogation…

Instrumentation and Detectors · Physics 2022-01-10 Junghyun Bae , Stylianos Chatzidakis

A Ring Imaging \v{C}erenkov detector built for the BRAHMS experiment at the Brookhaven RHIC is described. This detector has a high index of refraction gas radiator. \v{C}erenkov light is focused on a photo-multiplier based photon detector…

Instrumentation and Detectors · Physics 2008-11-26 R. Debbe , C. E. Jorgensen , J. Olness , Z. Yin

High-efficiency and high-purity particle identification are fundamental requirements for the success of the Belle II experiment, whose main goal is to explore the new-physics scenarios in the CP-violating decays of the B mesons. To achieve…

High Energy Physics - Experiment · Physics 2018-11-13 Umberto Tamponi

Muon accelerators offer an attractive option for a range of future particle physics experiments. They can enable high energy (TeV+) high energy lepton colliders whilst mitigating the difficulty of synchrotron losses, and can provide intense…

The international Muon Ionization Cooling Experiment (MICE) aims to demonstrate muon beam ionization cooling for the first time and constitutes a key part of the R&D towards a future neutrino factory or muon collider. Beam cooling reduces…

Accelerator Physics · Physics 2019-08-15 Tanaz Angelina Mohayai , Pavel Snopok , David Neuffer , Chris Rogers

Experimental and theoretical activities are underway at CERN with the aim of examining the feasibility of a very-high-flux neutrino source. In the present scheme, a high-power proton beam (some 4 MW) bombards a target where pions are…

Accelerator Physics · Physics 2014-11-18 G. Franchetti , S. Gilardoni , P. Gruber , K. Hanke , H. Haseroth , E. B. Holzer , D. Kuechler , A. M. Lombardi , R. Scrivens

Cherenkov light from cosmic-ray muons is a significant source of background for the Imaging Atmospheric Cherenkov Technique. However, muon events are also valuable as a diagnostic tool because they produce distinctive ring images, and the…

Astrophysics · Physics 2019-08-14 T. B. Humensky

The CLEO detector has been upgraded to include a state of the art particle identification system, based on the Ring Imaging Cherenkov Detector (RICH) technology, in order to take data at the upgraded CESR electron positron collider. The…

High Energy Physics - Experiment · Physics 2009-10-31 M. Artuso , R. Ayad , A. Efimov , S. Kopp , G. Majumder , R. Mountain , S. Schuh , T. Skwarnicki , S. Stone , G. Viehhauser , J. Wang , S. Anderson , Y. Kubota , A. Smith , T. Coan , V. Fadeyev , J. Ye

A high-repetition-rate pulsed muon source operating at approximately 50\,kHz holds the potential to improve the sensitivity of various particle physics and material science experiments involving muons. In this article, we propose utilizing…

In the forward end-cap of the Belle II spectrometer, particle identification is provided by a proximity focusing RICH detector with an aerogel radiator (ARICH). The ARICH's primary function is to effectively distinguish between pions and…

Instrumentation and Detectors · Physics 2023-08-09 Luka Santelj

We describe the design, construction and performance of a Ring Imaging Cherenkov Detector (RICH) constructed to identify charged particles in the CLEO experiment. Cherenkov radiation occurs in LiF crystals, both planar and ones with a novel…

We discuss the design and performance of a threshold Cerenkov counter for identification of charged hadrons. The radiator is pressurized gas, which is contained in thin-walled cylindrical modules. A mirror system of novel design transports…

High Energy Physics - Experiment · Physics 2008-11-26 Michael Sivertz , Bruce Berger , Richard Ehrlich , John Bartlet , Steven Csorna , Vivek Jain , Szabolcs Marka , Kay Kinoshita , Paula Pomianowski

The experimental requirements in near future accelerators (e.g. High Luminosity-LHC) has stimulated intense interest in development of detectors with high precision timing capabilities. With this as a goal, a new detection concept called…

This article presents the timing performance of materials with fast light emission, tested as Minimum Ionizing Particle detectors using 150 GeV hadron beams in Monte Carlo simulations and at the CERN SPS North Area. Pixels of cross-section…

Kilometer-scale deep under-ice or -water Cherenkov neutrino detectors may detect muon and electron neutrinos from astrophysical sources at energies of a TeV and above. Tau neutrinos are also expected from these sources due to neutrino…

Astrophysics · Physics 2008-11-26 T. DeYoung , S. Razzaque , D. F. Cowen