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Revising the observable consequences of slow-roll inflation

2009

We study the generation of primordial perturbations in a (single-field) slow-roll inflationary Universe. In momentum space, these (Gaussian) perturbations are characterized by a zero mean and a nonzero variance Delta(2) (k, t). However, in position space the variance diverges in the ultraviolet. The requirement of a finite variance in position space forces one to regularize Delta(2) (k, t). This can (and should) be achieved by proper renormalization in an expanding Universe in a unique way. This affects the predicted scalar and tensorial power spectra (evaluated when the modes acquire classical properties) for wavelengths that today are at observable scales. As a consequence, the imprint of…

AstrofísicaPhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Slow roll010308 nuclear & particles physicsFOS: Physical sciencesUnivers inflacionariPrivate communicationGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyManagementHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Quantum mechanics0103 physical sciences010306 general physicsUltraviolet radiationAstrophysics - Cosmology and Nongalactic Astrophysics
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