Universal Secular External Leg Corrections for Gauge Independent Scalar Self-Mass on de Sitter
gr-qc, astro-ph.CO, hep-th
Submitted: 2026-09-09
Updated: 2026-09-09
Comments: 34 pages, 10 figures, uses LaTeX2e
License: http://creativecommons.org/licenses/by/4.0/
The gist: This work concerns a procedure for removing gauge dependence from graviton corrections to the effective field equations for a massless, minimally coupled scalar on de Sitter background.
Terminology
Abstract
This work concerns a procedure for removing gauge dependence from graviton corrections to the effective field equations for a massless, minimally coupled scalar on de Sitter background. The procedure involves combining diagrams in the same way as the scattering amplitude for the t-channel exchange of the massless scalar between two massive particles, but without taking the asymptotic limits which are problematic in cosmology. Implementing this at 1-loop on flat space background requires five classes of diagrams, in addition to the naive exchange, and the combination of those diagrams does eliminate dependence on the graviton gauge fixing functional. When those same diagrams are generalized to de Sitter background, their combination cancels the most important (``nonlocal'') secular gauge dependence, but it leaves (``local'') secular gauge dependence that is associated with external legs. Local secular gauge dependence can be removed by adding two additional classes of diagrams, and making secular corrections to the external wavefunctions. The purpose of this paper is to include these additional corrections on de Sitter background in order to derive fully gauge independent effective field equations at 1-loop order.
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