Quantum Cosmology with a Complex ø6 Field at Finite Temperature
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Abstract
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.
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References
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