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On the one loop corrections to inflation and the CMB anisotropies

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arxiv astro-ph/0604488 v2 pith:7KDL7HHG submitted 2006-04-24 astro-ph gr-qchep-th

classification astro-phgr-qchep-th
keywords loopinflationcorrectioncorrectionsapproximationbackgroundeffectiveinflaton
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We investigate the one loop effective potential of inflation in a standard model of chaotic inflation. The leading one loop corrections to the effective inflaton potential are evaluated in the quasi de Sitter background, and we estimate the one loop correction to the two-point function of the inflaton perturbations in the Hartree approximation. In this approximation, the one loop corrections depends on the total number of e-foldings of inflation and the maximal effect is estimated to be a correction to the power spectrum of a few percent. However, such a correction may be difficult to disentangle from the background in the simplest scenario.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Strongly Coupled Sectors in Inflation: Gapped Theories of Unparticles

    hep-th 2025-12 unverdicted novelty 7.0 of 10

    Compactified 5D unparticle theories generate gapped excitations whose exchange in inflationary correlators yields oscillations modulated by anomalous dimensions and possible interference patterns under brane-localized...

  2. Confronting infrared divergences in de Sitter: loops, logarithms and the stochastic formalism

    hep-th 2025-07 conditional novelty 7.0 of 10

    The authors show that loop corrections do not alter tree-level time dependence in de Sitter correlators, so secular growth is a regularization artifact, not a physical effect.

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