Boundary Conditions in Quantum Cosmology in the Brans-Dicke's Theory

Details Boundary Conditions in Quantum Cosmology in the Brans-Dicke's Theory Boundary Conditions in Quantum Cosmology in the Brans-Dicke's Theory

May 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992chphl...9..273z&link_type=abstract

Chinese Physics Letters, Volume 9, Issue 5, pp. 273-276 (1992).

Physics

5

Scientific paper

The Wheeler-DeWitt equation for the Brans-Dicke's theory of gravitation
is solved by two boundary condition proposals of Hartle-Hawking ("no
boundary") and Vilenkin ("tunneling from nothing"). It is found that all
classical expanding trajectories begin on the classical-quantum boundary
and the effective cosmological constant is very small.

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