Novel Photo Multiplier Tubes for the Cherenkov Telescope Array Project
Takeshi Toyama, Razmik Mirzoyan, Hugh Dickinson, Christian Fruck,, J\"urgen Hose, Hanna Kellermann, Max Kn\"otig, Eckart Lorenz, Uta Menzel,, Daisuke Nakajima, Reiko Orito, David Paneque, Thomas Schweizer, Masahiro, Teshima, Tokonatsu Yamamoto (for the CTA Consortium)

TL;DR
This paper discusses the development of advanced photo multiplier tubes with significantly improved quantum efficiency, collection efficiency, and reduced after-pulsing, tailored for the Cherenkov Telescope Array project in gamma astrophysics.
Contribution
It presents the latest advancements in PMT technology, achieving peak QE of around 40% and enhanced collection efficiency, marking a major upgrade over previous generations for Cherenkov telescopes.
Findings
Peak quantum efficiency increased to approximately 40%.
Photoelectron collection efficiency improved to 95-98%.
After-pulsing reduced to 0.02%.
Abstract
Currently the standard light sensors for imaging atmospheric Cherenkov telescopes are the classical photo multiplier tubes that are using bialkali photo cathodes. About eight years ago we initiated an improvement program with the Photo Multiplier Tube (PMT) manufacturers Hamamatsu (Japan), Electron Tubes Enterprises (England) and Photonis (France) for the needs of imaging atmospheric Cherenkov telescopes. As a result, after about 40 years of stagnation of the peak Quantum Efficiency (QE) on the level of 25-27%, new PMTs appeared with a peak QE of 35%. These have got the name super-bialkali. The second significant upgrade has happened very recently, as a result of a dedicated improvement program for the candidate PMT for Cherenkov Telescope Array. The latter is going to be the next generation major instrument in the field of very high energy gamma astrophysics and will consist of over…
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Taxonomy
TopicsPhotocathodes and Microchannel Plates · Radiation Detection and Scintillator Technologies · Astrophysics and Cosmic Phenomena
