“…Wide band gap semiconductor materials are considered to be suitable for solar-blind photodetectors, such as AlN, AlGaN, , ZnMgO, − diamond, cubic BN, and Ga 2 O 3 . − However, a complex buffer layer is needed to reduce the lattice mismatch between the AlGaN film and the substrate. , Although MgZnO has a wide tunable range band gap (3.3–7.8 eV) by adjusting the composition of Mg, the problem of phase segregation at high Mg concentration needs to be further solved. , The band gap of diamond is fixed at 5.5 eV, which limits its detection wavelength range shorter than 225 nm. , Significantly, Ga 2 O 3 with a natural band gap of ∼4.9 eV without the alloying process has the advantages of low cost and excellent chemical and physical stabilities, which make it suitable for solar-blind photodetection. ,,− …”