Back Reaction and Semiclassical Approximation of cosmological models coupled to matter

Details Back Reaction and Semiclassical Approximation of cosmological models coupled to matter Back Reaction and Semiclassical Approximation of cosmological models coupled to matter

1997-03-04

arxiv.org/abs/gr-qc/9703009v1

Nucl.Phys.Proc.Suppl.57:299-302,1997

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

4 pages, Latex, to appear in: Proceedings of the Second Meeting on constrained Dynamics and Quantum Gravity (Santa Margherita

Scientific paper

10.1016/S0920-5632(97)00394-0

Bianchi -I, -III, and FRW type models minimally coupled to a massive spatially homogeneous scalar field (i.e. a particle) are studied in the framework of semiclassical quantum gravity. In a first step we discuss the solutions of the corresponding equation for a Schr\"odinger particle propagating on a classical background. The back reaction of the Schr\"odinger particle on the classical metric is calculated by means of the Wigner function and by means of the expectation value of the energy-momentum-tensor of the field as a source. Both methods in general lead to different results.

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