A tomographic description for classical and quantum cosmological perturbations

Details A tomographic description for classical and quantum cosmological perturbations A tomographic description for classical and quantum cosmological perturbations

2009-05-08

arxiv.org/abs/0905.1244v1

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

12 pages

Scientific paper

Classical and quantum perturbations can be described in terms of marginal distribution functions in the framework of tomographic cosmology. In particular, the so called Radon transformation and the mode-parametric quantum oscillator description can give rise to links between quantum and classical regimes. The approach results a natural scheme to discuss the transition from the quantum to the classical perturbations and then it could be a workable scheme to connect primordial fluctuations with the today observed large scale structure.

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