On the Physical Significance of Infra-red Corrections to Inflationary Observables
N. Bartolo (1, 2), S. Matarrese (1, 2), M. Pietroni (2), A., Riotto (2, 3), D. Seery (4) ((1) Physics Dept. Padova, Italy; (2) INFN,, Padova, Italy; (3) CERN, Switzerland; (4) Centre for Theoretical Cosmology,, Cambridge, UK)

TL;DR
This paper argues that large infra-red corrections in inflationary observables are only present in unobservable quantities, aligning with theoretical expectations about infra-red effects in cosmology.
Contribution
It clarifies that significant infra-red corrections do not affect directly observable inflationary quantities, resolving apparent discrepancies in theoretical calculations.
Findings
Infra-red corrections are large only in non-observable quantities
Observable inflationary power spectrum remains unaffected by large infra-red effects
Supports the view that infra-red effects do not compromise physical predictions
Abstract
Inflationary observables, like the power spectrum, computed at one- and higher-order loop level seem to be plagued by large infra-red corrections. In this short note, we point out that these large infra-red corrections appear only in quantities which are not directly observable. This is in agreement with general expectations concerning infra-red effects.
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