Quantum Cosmology with a Complex phi6 Field at Finite Temperature

Details Quantum Cosmology with a Complex phi6 Field at Finite Temperature Quantum Cosmology with a Complex phi6 Field at Finite Temperature

Jan 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999chphl..16...76s&link_type=abstract

Chinese Physics Letters, Volume 16, Issue 1, pp. 76-78 (1999).

Physics

1

Scientific paper

Quantum cosmology with complex phi6 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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