Development of a <scp>SiPM</scp>‐Based Water‐Cherenkov Detector for Astrophysics

ABSTRACT The Cherenkov effect is widely employed in experiments involving cosmic rays and neutrinos that utilize large sensitive volumes. The water is widely employed as the sensitive medium, with the primary particle to be detected being the muon. In this work, we present the development of a new water‐Cherenkov detector that utilizes a photon trapping system and silicon photomultipliers (SiPMs) to record the detector signals, which has been named C‐Arapuca. The utilization of SiPMs presents advantages over the traditional photomultiplier tube, PMT, such as a much lower operating voltages and the construction of more compact devices with greater geometric freedom. To study the performance of the C‐Arapuca, a tank containing 550 L of ultra‐pure water was utilized. The confinement of Cherenkov photons is achieved through a dichroic filter in the optical window and a light guide that shifts the photons wavelength and guide them to the eight SiPMs positioned along its sides. The results of the efficiency of muon detection from local cosmic radiation are presented, indicating the feasibility of employing the C‐Arapuca in future astroparticle experiments.