Cosmological perturbations and short distance physics from Noncommutative Geometry
arXiv:hep-th/0203099 · doi:10.1088/1126-6708/2002/06/049
Abstract
We investigate the possible effects on the evolution of perturbations in the inflationary epoch due to short distance physics. We introduce a suitable non local action for the inflaton field, suggested by Noncommutative Geometry, and obtained by adopting a generalized star product on a Friedmann-Robertson-Walker background. In particular, we study how the presence of a length scale where spacetime becomes noncommutative affects the gaussianity and isotropy properties of fluctuations, and the corresponding effects on the Cosmic Microwave Background spectrum.
Published version, 16 pages
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Cited by in corpus (108)
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