A Solar-blind UV photodetectors (SBPs) have been attracting great attention due to their widely used in missile tracking, fire detection, biochemical analysis, astronomical observations, space-to-space communications, etc. At present, scholars are found that wide bandgap semiconductor materials such as Al<sub>x</sub>Ga<sub>1-x</sub>N, Mg<sub>1</sub>Zn<sub>1-x</sub>O, diamond and β-Ga<sub>2</sub>O<sub>3</sub>are ideal semiconductor materials for developing high-performance SBPs. As the ultra-wide band gap semiconductor material, β-Ga<sub>2</sub>O<sub>3</sub>has the large band gap width of 4.9 eV, strong breakdown electric field, absorption edge located in the solar blind ultraviolet band (200-280 nm) and has high transmittance in the near ultraviolet and the whole visible band. Therefore, β-Ga<sub>2</sub>O<sub>3</sub> is a very suitable material for making solar blind UV photodetectors. However, the p-type β-Ga<sub>2</sub>O<sub>3</sub> is difficult to doping, which limits the further development of β-Ga<sub>2</sub>O<sub>3</sub> devices. In this paper, the β-Ga<sub>2</sub>O<sub>3</sub> thin films with different Cu doping contents were grown on sapphire substrates by chemical vapor deposition method, and the morphology, crystal structure and optical properties of β-Ga<sub>2</sub>O<sub>3</sub> films were measured. The test results show that the surface of β-Ga<sub>2</sub>O<sub>3</sub> films with different Cu contents is relatively smooth, and the (-201) diffraction peak positions shift to the lower degree side with increasing Cu content, which indicates that Cu<sup>2+</sup> is substituted for Ga<sup>3+</sup> into the β-Ga<sub>2</sub>O<sub>3</sub> lattice. The optical absorption spectrum measurement indicated that the energy gaps of samples were evidently narrowed with increasing Cu doping concentration. Hall measurements results indicated that the Cu doped β-Ga<sub>2</sub>O<sub>3</sub> thin films was p-type conductivity with a hole concentration of 7.36×10<sup>14</sup>, 4.83×10<sup>15</sup> and 1.69×10<sup>16</sup> cm<sup>−3</sup>, respectively. In addition, a photoconductive UV detector with MSM structure was prepared by evaporation of Au on a Cu-doped β-Ga<sub>2</sub>O<sub>3</sub>thin film, and its UV detection performance was studied. The results show that the photocurrent value of the devices increases with the increasing Cu contents. The <i>I</i><sub>l</sub>/<i>I</i><sub>d</sub> ratio is about 3.8×10<sup>2</sup> of 2.4% Cu content device under 254 nm light with at 10 V. The rise time and decay time of 0.11 s and 0.13 s, respectively. Furthermore, the responsivity and external quantum efficiency can reach up to 1.72 A/W and 841% under 254 nm light with a light intensity of 64 μW/cm<sup>2</sup>.