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Fifth-Force Constraints from UV-Complete Scalar-Tensor Gravity

Alfio M. Bonanno1,2 and Emiliano M. Glaviano1,2,3

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Phys. Rev. Lett. 136, 201501 – Published 20 May, 2026

DOI: https://doi.org/10.1103/q1gq-sgy3

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 αY and range λY. 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 (αY,λY) 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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Phys. Rev. Lett. 136, 201501– Published 20 May, 2026
  • Received 13 January 2026
  • Revised 27 April 2026
  • Accepted 1 May 2026
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