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Wave Function in Quantum Cosmology of Bergmann-Wagoner Scalar-Tensor Gravitational Theory |
LIU Zixin*;CHEN Xiaojia |
Department of Physics, He’nan Normal University, Xinxiang 453002
*also Institute of Fundamental and Applied Science, Zhengzhou 450052
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Cite this article: |
LIU Zixin, CHEN Xiaojia 1992 Chin. Phys. Lett. 9 673-676 |
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Abstract The semiclassical cosmological wave function in quantum cosmology of the Bergrnann-Wagoner scalar tensor gravitational theory is given in Vilenkin approach and Hartle-Hawking approach. The initial condition for inflation is given, we show there exists an extended inflationary phase in a hopeful particular model.
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98.80.Dr
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Published: 01 December 1992
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