Non-Forward UV/IR Relations
Carl Beadle, Giulia Isabella, Davide Perrone, Sara Ricossa, Francesco Riva, Francesco Serra
TL;DR
This work develops a forward-limit–free program to derive positivity bounds on EFT Wilson coefficients in theories with massless particles and gravity by employing non-forward dispersion relations defined at finite momentum transfer. It introduces smeared dispersion relations and a systematic finite-t improvement algorithm that cancels higher UV contributions, reducing the problem to a semidefinite program over a finite basis (e.g., Legendre polynomials) to bound coefficients like $g_{2,0}$, $g_{3,1}$, and $g_{4,0}$. The analysis covers both strictly tree-level and loop-corrected amplitudes, clarifying how gravity induces non-analyticities that invalidate Taylor expansions near $t=0$ and how the finite-t approach remains robust by treating loop effects perturbatively. The results demonstrate convergence to known forward-limit bounds in the absence of gravity, quantify gravity-induced relaxations, and provide a practical framework for extracting UV-reliability constraints in EFTs with massless particles.
Abstract
We study bounds arising from the analyticity and unitarity of scattering amplitudes in the context of effective field theories with massless particles. We provide an approach that only uses dispersion relations away from the forward limit. This is suitable to derive constraints in the presence of gravity, in a way that is robust with respect to radiative corrections. Our method not only allows us to avoid the Coulomb pole, but also the singularities associated with calculable loop effects, which would otherwise diverge.
