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Fifth-Force Constraints from UV-Complete Scalar-Tensor Gravity
Abstract
We study an O ( N ) scalar multiplet nonminimally coupled to gravity and follow its renormalization-group (RG) flow in the vicinity of an interacting, nonperturbatively UV-complete scaling regime of scalar-tensor theory. In the broken phase, the radial mode mediates a universal Yukawa correction to Newtonian gravity, parametrized by a strength α Y and range λ Y . Imposing UV completeness—regular RG trajectories that reach the UV scaling regime—restricts the infrared data to a finite wedge, which maps to a narrow region in the ( α Y , λ Y ) plane. Its complement is, therefore, ruled out by UV completeness alone. Remarkably, part of this theory-excluded domain lies below current experimental exclusion envelopes, so improved fifth-force searches can directly test and potentially falsify this class of UV-complete scalar-tensor models.
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Cited by 1
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Metadata
- Authors
- Bonanno, A. M., & Glaviano, E. M.
- Venue
- Physical Review Letters
- Publisher
- American Physical Society (APS)
- Published
- 2026-05-20
- Volume
- 136
- Issue
- 20
- ISSN
- 0031-9007
- 1079-7114
- Cited by
- 1
- Language
- en
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