pith:PXA5EF2O
Finite parts of inflationary loops II: A streamlined UV in-in algorithm and distinguishable signatures
A streamlined algorithm for in-in loop integrals reveals an apparent difficulty renormalizing with Hamiltonian counterterms and isolates distinguishable finite parts in the one-loop bispectrum.
arxiv:2512.20467 v2 · 2025-12-23 · hep-th · astro-ph.CO · gr-qc · hep-ph
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Claims
The method leads us to identify an apparent difficulty to renormalize with Hamiltonian counterterms within the in-in formalism. We also discuss the importance of the finite parts of loop corrections that can be distinguished from their associated counterterm contributions.
That the streamlined UV extraction via dimensional regularization fully captures the finite parts without residual scheme dependence or that the chosen interactions in EFT inflation produce a genuinely distinguishable one-loop bispectrum contribution independent of counterterm choices.
A new UV in-in algorithm for inflationary loops identifies renormalization difficulties and distinguishable finite corrections to the one-loop bispectrum in EFT inflation.
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| First computed | 2026-05-17T23:39:04.559382Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
7dc1d2174ed2c4346b10e97964b98324526df40dd1194fcb9095893b215c2570
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Canonical record JSON
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