A Double Layered Water Cherenkov Detector Array for Gamma-Ray Astronomy

TL;DR

This paper proposes a double-layered water Cherenkov detector design for gamma-ray astronomy, enhancing background rejection and angular resolution while being cost-effective for future observatories.

Contribution

It introduces a novel double-chamber water Cherenkov detector configuration with reflective surfaces, improving performance and muon tagging capabilities for gamma-ray detection.

Findings

Enhanced gamma/hadron separation with the new design

Improved angular resolution in the double-layer configuration

Cost-effective approach for large-scale gamma-ray observatories

Abstract

Ground-level particle detection is now a well-established approach to TeV gamma-ray astronomy. Detection of Cherenkov light produced in water-filled detection units is a proven and cost-effective method. Here we discuss the optimization of the units towards the future Southern Wide-field Gamma-ray Observatory (SWGO). In this context, we investigate a new type of configuration in which each water Cherenkov detector (WCD) unit in the array comprises two chambers with black or reflective walls and a single photomultiplier tube (PMT) in each chamber. We find that this is a cost-effective approach that improves the performance of the WCD array with respect to current approaches. A shallow lower chamber with a PMT facing downwards enables muon tagging and the identification of hadron-induced air showers, which are the primary source of background in gamma-ray astronomy. We investigate how gamma/hadron separation power and achievable angular resolution depend on the geometry and wall reflectivity of the detector units in this configuration. We find that excellent angular resolution, background rejection power and low-energy response are achievable in this double-layer configuration, with the aid of reflective surfaces in both chambers.