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Numerically,k 0 ≃1 eV corresponds to a coarse-graining lengthℓ 0 ∼(ℏc)/k 0 ≈200 nm, well above microscopic interatomic scales, therefore, appropriate for a continuum, perfect

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gr-qc 1

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2026 1

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

gr-qc · 2026-05-11 · unverdicted · novelty 6.0 · 2 refs

UV completeness in scalar-tensor gravity restricts Yukawa fifth-force parameters α and λ to a finite wedge whose complement is ruled out, with part of the excluded domain below current experimental bounds.

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  • Fifth-Force Constraints from UV-Complete Scalar-Tensor Gravity gr-qc · 2026-05-11 · unverdicted · none · ref 30 · 2 links

    UV completeness in scalar-tensor gravity restricts Yukawa fifth-force parameters α and λ to a finite wedge whose complement is ruled out, with part of the excluded domain below current experimental bounds.