PIRSA:07050019
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A Hamiltonian framework for cosmological perturbations to any order Speaker(s): Bianca Dittrich
Abstract: We introduce a framework that allows to calculate cosmological perturbations in a gauge invariant manner to any order. The two main features of this framework are to take physical observables as basic objects and to treat the variables describing the background geometry as fully dynamical. Backreaction effects can therefore naturally adressed. At the end I will mention applications to Loop Quantum Cosmology.
Date: 01/05/2007 - 11:00 am
Series: Cosmology & Gravitation
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