I. Introduction
Ultraviolet photodetectors (UV PDs), particularly those operating within the solar-blind range (200–280 nm), have garnered significant attention due to their broad applications in environmental monitoring, flame detection, space exploration, and communication systems [1], [2], [3], [4], [5], [6]. As the demand for such devices continues to grow, higher sensitivity, compact integration, and enhanced performance are required [7], [8], [9]. While photomultiplier tubes (PMTs) have traditionally offered high sensitivity, their drawbacks such as large size, high operating voltages (>1000 V), fragility, and the necessity for external filters, limit their use in modern and compact systems. Moreover, their susceptibility to saturation under intense light further restricts their application range [10], [11], [12].