Negative running of gravitational positivity
J. Fernandez, M. Ruhdorfer, J. Serra

TL;DR
This paper studies how certain effective operators involving scalars, photons, and gravitons evolve under renormalization group flow, revealing negative running effects influenced by gravitational interactions.
Contribution
It demonstrates that non-minimal three-point interactions cause negative Wilson coefficient running, with gravitational effects potentially dominating over this running.
Findings
Negative running of Wilson coefficients due to non-minimal interactions.
Gravitational loops generate positive infrared contributions.
The dominance of gravitational effects depends on the number of coupled particles.
Abstract
We investigate the one-loop renormalization group evolution in four dimensions of the leading operators in the effective field theories of shift-symmetric scalars, photons, and gravitons. We show that certain non-minimal three-point interactions induce a negative running of the corresponding Wilson coefficients, with beta-functions suppressed by the Planck scale. The decrease of the coefficients toward the infrared prompts us to revisit their dispersive bounds, in particular accounting for graviton loops. Gravitational interactions generate positive infrared contributions which, after smearing over the momentum transfer, are argued to dominate over the negative running, provided the number of non-minimally coupled particles is bounded from above according to the species bound.
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