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IR divergence does not affect the gauge-invariant curvature perturbation

2 Pith papers cite this work. Polarity classification is still indexing.

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abstract

We address the infrared(IR) divergence problem during inflation that appears in the loop corrections to the primordial perturbations. In our previous paper, we claimed that, at least in single field models, the IR divergence is originating from the gauge artifact. Namely, diverging IR corrections should not appear in genuine gauge-invariant observables. We propose here one simple but explicit example of such gauge-invariant quantities. Then, we explicitly calculate such a quantity to find that the IR divergence is absent at the leading order in the slow-roll approximation for the usual scale invariant vacuum state. At the same time we notice that there is a subtle issue on the gauge-invariance in how to specify the initial vacuum state.

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fields

gr-qc 2

years

2026 2

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UNVERDICTED 2

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background 1

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background 1

representative citing papers

Locality in effective field theory for inflationary soft modes

gr-qc · 2026-05-19 · unverdicted · novelty 6.0

The authors define a locality condition for hard-mode states during inflation that unifies local effective dynamics for soft modes, suppression of loop corrections, generalized soft theorems, and absence of infrared divergences in observable correlators.

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Showing 2 of 2 citing papers.

  • Locality in effective field theory for inflationary soft modes gr-qc · 2026-05-19 · unverdicted · none · ref 25 · internal anchor

    The authors define a locality condition for hard-mode states during inflation that unifies local effective dynamics for soft modes, suppression of loop corrections, generalized soft theorems, and absence of infrared divergences in observable correlators.

  • Fixing the Renormalization of Inflationary Loops via Ward Identities gr-qc · 2026-05-13 · unverdicted · none · ref 100 · internal anchor

    Ward identities from large gauge symmetry impose model-independent constraints on renormalizing inflationary loops and non-perturbatively govern the infrared power spectrum evolution.