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• W2395583211 abstract "It is believed that soon after the Planck era, spacetime should have a semi-classical nature. In this context we consider quantum fields propagating in a classical gravitational field and study the backreaction of these fields, using the expected value of the energy-momentum tensor as source of the gravitational field. According to this theory, the escape from General Relativity theory is unavoidable. Two geometric counter-term are needed to regularize the divergences which come from the expected value. There is a parameter associated to each counter-term and in this work we found numerical solutions of this theory to particular initial conditions, for general Bianchi Type I spaces. We show that even though there are spurious solutions some of them can be considered physical. These physical solutions include de Sitter and Minkowski that are obtained asymptotically." @default.
• W2395583211 created "2016-06-24" @default.
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• W2395583211 date "2006-09-08" @default.
• W2395583211 modified "2023-09-27" @default.
• W2395583211 title "Numerical Bianchi type I solutions in semiclassical gravitation" @default.
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• W2395583211 doi "https://doi.org/10.1103/physrevd.74.063508" @default.
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