Singularities in Cosmological Loop Correlators II : Non Local Interactions and Flat Space limits

Fuente: arXiv
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Main Authors: Ansari, Elaf, Bhowmick, Supritha, Ghosh, Diptimoy
Format: Preprint
Published: 2025
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author Ansari, Elaf
Bhowmick, Supritha
Ghosh, Diptimoy
author_facet Ansari, Elaf
Bhowmick, Supritha
Ghosh, Diptimoy
contents Non-local interactions naturally arise in the ADM formalism after solving the constraint equations and substituting their solutions back into the action. However, the effects of these non-local operators on loop corrections to cosmological correlators remain largely unexplored. Extending the analysis of arXiv:2503.21880 , in this work we compute the $1$-loop bispectrum during slow-roll inflation, including the inverse-Laplacian operators present at cubic and quartic order in the ADM action (in the spatially flat gauge). These non-local vertices introduce non-trivial angular dependencies that significantly complicate the evaluation of loop integrals. We find that the diagrammatic rules of arXiv:2503.21880 for identifying poles and branch cuts in correlators without explicit integration remain valid even in the presence of such non-local interactions. Finally, we derive the flat-space limit of the $1$-loop inflationary correlator and verify it with explicit examples, thereby establishing a direct correspondence between its leading total-energy singularities ($ω_T\rightarrow0$) and the flat-space scattering amplitude.
format Preprint
id arxiv_https___arxiv_org_abs_2512_11040
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Singularities in Cosmological Loop Correlators II : Non Local Interactions and Flat Space limits
Ansari, Elaf
Bhowmick, Supritha
Ghosh, Diptimoy
High Energy Physics - Theory
General Relativity and Quantum Cosmology
High Energy Physics - Phenomenology
Non-local interactions naturally arise in the ADM formalism after solving the constraint equations and substituting their solutions back into the action. However, the effects of these non-local operators on loop corrections to cosmological correlators remain largely unexplored. Extending the analysis of arXiv:2503.21880 , in this work we compute the $1$-loop bispectrum during slow-roll inflation, including the inverse-Laplacian operators present at cubic and quartic order in the ADM action (in the spatially flat gauge). These non-local vertices introduce non-trivial angular dependencies that significantly complicate the evaluation of loop integrals. We find that the diagrammatic rules of arXiv:2503.21880 for identifying poles and branch cuts in correlators without explicit integration remain valid even in the presence of such non-local interactions. Finally, we derive the flat-space limit of the $1$-loop inflationary correlator and verify it with explicit examples, thereby establishing a direct correspondence between its leading total-energy singularities ($ω_T\rightarrow0$) and the flat-space scattering amplitude.
title Singularities in Cosmological Loop Correlators II : Non Local Interactions and Flat Space limits
topic High Energy Physics - Theory
General Relativity and Quantum Cosmology
High Energy Physics - Phenomenology
url https://arxiv.org/abs/2512.11040