A New Type of Isotropic Cosmological Models Without Singularity
19804 pages
Published in:
- Phys.Lett.B 91 (1980) 99-102,
- Adv.Ser.Astrophys.Cosmol. 3 (1987) 130-133
- Published: 1980
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Abstract: (Elsevier)
The Einstein equations with quantum one-loop contributions of conformally covariant matter fields are shown to admit a class of nonsingular isotropic homogeneous solutions that correspond to a picture of the Universe being initially in the most symmetric (de Sitter) state.- COSMOLOGICAL MODEL
- GRAVITATION: QUANTIZATION
- QUANTIZATION: APPROXIMATION
- Einstein equation
- INVARIANCE: CONFORMAL
- INVARIANCE: DE SITTER
- invariance: conformal
- field theory: de Sitter
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