Quantum Cosmology with a Complex ø⁶ Field at Finite Temperature

Quantum cosmology with complex ø⁶ fields at finite temperature for the Vilenkin boundary conditions and Hartle-Hawking boundary conditions has been studied in this paper. The corresponding Wheeler-DeWitt equations and the Universe wave functions are obtained. At the same time, the probability density distribution is calculated and the effect of temperature on probability density distribution is found.