Development of a blue-mirror multilayer coating on light concentrators for future SiPM cameras
Akira Okumura, Junya Haga, Chiaki Inoue, Keiji Nishimoto, Kazuhiro, Furuta, and Hiroyasu Tajima

TL;DR
This paper presents a multilayer coating on light concentrators that enhances photon collection efficiency for SiPMs in gamma-ray telescopes by reflecting more in the 300-500 nm range and less beyond 550 nm, improving signal-to-noise ratio.
Contribution
The study introduces a novel 8-layer multilayer coating design applied to light concentrators, optimizing photon reflection for SiPMs in Cherenkov telescope applications.
Findings
~50% improvement in photon collection efficiency at 403 nm
Reduced reflection at 830 nm by 30-50%
Successful demonstration with a prototype light concentrator
Abstract
Silicon photomultipliers (SiPMs) have a few advantages over conventional photomultiplier tubes (PMTs) used in imaging atmospheric Cherenkov telescopes. The first notable characteristic is their higher photon detection efficiency (PDE) of up to about 60%, which is roughly 1.2-1.5 times better than that of PMTs in the 300-450 nm range, enabling us to lower the energy threshold of gamma-ray observations and increase the photon statistics. The second advantage is that SiPMs are chemically stable after exposure to long and bright illumination, while PMTs can cause gain and quantum efficiency degradation after the same exposure. Therefore, the use of SiPMs under bright or full moon conditions may extend the total observation time in the highest energy coverage region of individual telescopes. However, the SiPM PDE is too high in wavelengths longer than 500 nm; hence, the signal-to-noise ratio…
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