Crossing Symmetric Dispersion Relations in QFTs
Aninda Sinha, Ahmadullah Zahed
TL;DR
The paper develops a crossing-symmetric dispersion framework for 2-2 scattering by mapping the Mandelstam variables to a cubic z-variable, achieving manifest three-channel crossing symmetry. It derives a general, nonperturbative set of positivity constraints and null constraints on Wilson coefficients, expressed via Gegenbauer partial waves, and presents a Feynman-block (Dyson-block) representation that illustrates how exchange and contact contributions emerge from the crossing-symmetric data. The approach yields practical results, including a method to locate the first massive string pole from a low-energy dilaton amplitude in type II strings and a numerical Froissart-type bound valid at all energies, with convergence demonstrated through string-theory amplitudes and spin truncations. The framework connects to EFT-hedron ideas and higher-dimensional S-matrix bootstrap, offering a unified, crossing-symmetric avenue to constrain EFTs and relate low-energy data to high-energy spectrum.
Abstract
For 2-2 scattering in quantum field theories, the usual fixed $t$ dispersion relation exhibits only two-channel symmetry. This paper considers a crossing symmetric dispersion relation, reviving certain old ideas in the 1970s. Rather than the fixed $t$ dispersion relation, this needs a dispersion relation in a different variable $z$, which is related to the Mandelstam invariants $s,t,u$ via a parametric cubic relation making the crossing symmetry in the complex $z$ plane a geometric rotation. The resulting dispersion is manifestly three-channel crossing symmetric. We give simple derivations of certain known positivity conditions for effective field theories, including the null constraints, which lead to two sided bounds and derive a general set of new non-perturbative inequalities. We show how these inequalities enable us to locate the first massive string state from a low energy expansion of the four dilaton amplitude in type II string theory. We also show how a generalized (numerical) Froissart bound, valid for all energies, is obtained from this approach.
