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Early Universe Dynamics in Semi-Classical Loop Quantum Cosmology

James E. Lidsey
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Abstract

Within the framework of loop quantum cosmology, there exists a semi-classical regime where spacetime may be approximated in terms of a continuous manifold, but where the standard Friedmann equations of classical Einstein gravity receive non-perturbative quantum corrections. An approximate, analytical approach to studying cosmic dynamics in this regime is developed for both spatially flat and positively-curved isotropic universes sourced by a self-interacting scalar field. In the former case, a direct correspondence between the classical and semi-classical field equations can be established together with a scale factor duality that directly relates different expanding and contracting universes. Some examples of non-singular, bouncing cosmologies are presented together with a scaling, power-law solution.

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BibTeXRIS

James E. Lidsey. 2004-11-26. Early Universe Dynamics in Semi-Classical Loop Quantum Cosmology. https://doi.org/10.1088/1475-7516%2F2004%2F12%2F007

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