Anisotropic cosmological models in terms of Raychaudhuri and Wheeler-DeWitt equations
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Classical anisotropic cosmological models are described in terms of the Raychaudhuri equation for a perfect fluid. Quantum ones are considered using the Wheeler-DeWitt equation. The Universe birth probability has been calculated for a flat model with dust and de Sitter vacuum.
PACS numbers98.80.Jk 98.80.Qc
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