Classical Effective Field Theory for Weak Ultra Relativistic Scattering
Barak Kol

TL;DR
This paper develops a classical effective field theory for weak ultra relativistic scattering, capturing instantaneous transverse field propagation and localizing particle equations of motion at the passing instant, applicable to scalar, electromagnetic, and gravitational interactions.
Contribution
It introduces a novel classical effective field theory framework for ultra relativistic scattering, including power counting, subleading corrections, and a gravitational field decomposition.
Findings
Reproduces leading scattering angles for various fields
Computes subleading corrections and interaction duration
Provides a gravitational field decomposition with non-linear action
Abstract
Inspired by the problem of Planckian scattering we describe a classical effective field theory for weak ultra relativistic scattering in which field propagation is instantaneous and transverse and the particles' equations of motion localize to the instant of passing. An analogy with the non-relativistic (post-Newtonian) approximation is stressed. The small parameter is identified and power counting rules are established. The theory is applied to reproduce the leading scattering angle for either a scalar interaction field or electro-magnetic or gravitational; to compute some subleading corrections, including the interaction duration; and to allow for non-zero masses. For the gravitational case we present an appropriate decomposition of the gravitational field onto the transverse plane together with its whole non-linear action. On the way we touch upon the relation with the eikonal…
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