“…Deep ultraviolet photodetectors (DUV PDs) (<280 nm), also known as solar-blind PDs, have piqued interest due to their wide range of applications in defense, space communication, civil, agriculture, healthcare, UV astronomy, high-temperature flame detection, solar-blind imaging for missile tracking, ozone hole monitoring, and other fields. − Wide-band-gap and ultrawide-band-gap semiconductor materials such as GaN, AlGaN, diamond, Lu 2 O 3 , and Ga 2 O 3 have emerged as promising candidates for solar-blind PDs because of their wide- and ultrawide band gap due to which they exhibit intrinsic solar-blindness. Unlike commercially available UV PDs based on narrow-band-gap semiconductor materials such as Si and GaAs, they do not require any additional optical filter or large cooling systems. ,− Among these, β-Ga 2 O 3 has received a lot of attention because of its excellent material properties such as an ultrawide direct band gap of about 4.9 eV, superior radiation hardness, high chemical and thermal stability, and high absorption coefficient (>10 5 cm –1 ). In addition, to date, high-crystalline-quality Ga 2 O 3 single-crystal substrates, epilayers, and thin films could be grown quite maturely and cost-effectively by various melt growth and thin-film techniques including edge-defined film-fed growth (EFG), Czochralski (CZ) method, MOCVD, halide vapor-phase epitaxy (HVPE), atomic layer deposition (ALD), pulsed laser deposition (PLD), and molecular beam epitaxy (MBE) without any doping complexity in comparison to other wide and ultrawide-band-gap semiconductor materials. − Apart from the β-phase, DUV PDs have also been demonstrated on amorphous and ε-phases of Ga 2 O 3 . ,,− …”