Effective potentials for de Sitter and anti de Sitter quantum fields
Alfio Bonanno, Sergio Luigi Cacciatori, Ugo Moschella

TL;DR
This paper develops a systematic method for calculating one-loop effective potentials for scalar fields in curved spacetimes, with explicit results for de Sitter and anti-de Sitter backgrounds, including two-loop calculations in certain cases.
Contribution
It provides a general formula for effective potentials in arbitrary geometries and extends calculations to two loops in de Sitter space, matching flat-space results and exploring AdS space.
Findings
Effective potentials derived for scalar fields in curved spacetimes.
Two-loop beta function and anomalous mass dimension match flat-space results.
Flat limit recovers Coleman-Weinberg potential, confirming consistency.
Abstract
We derive a systematic treatment of one-loop effective potentials for interacting scalar fields in curved spacetimes, providing a general formula valid in arbitrary geometries and explicit results for de Sitter and anti-de Sitter backgrounds. We then compute the effective potential for a scalar theory on a de Sitter space in any integer dimension. In and dimensional regularization, we extend the calculation up to two loops and compute the -function and the anomalous mass dimension. They coincide exactly with flat-space results, despite dramatic curvature modifications to physical masses/couplings. The flat limit recovers Coleman-Weinberg, confirming consistency. Working in dimensions, we repeat the calculation for by using point-splitting regularization, obtaining analogous results for the -function and anomalous mass dimension.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Quantum Electrodynamics and Casimir Effect
