Abstract
When are two collider events similar? Despite the simplicity and generality of this question, there is no established notion of the distance between two events. To address this question, we develop a metric for the space of collider events based on the earth mover's distance: the "work" required to rearrange the radiation pattern of one event into another. We expose interesting connections between this metric and the structure of infrared- and collinear-safe observables, providing a novel technique to quantify event modifications due to hadronization, pileup, and detector effects. We showcase how this metrization unlocks powerful new tools for analyzing and visualizing collider data without relying upon a choice of observables. More broadly, this framework paves the way for data-driven collider phenomenology without specialized observables or machine learning models.
Highlights
When are two collider events similar? Despite the simplicity and generality of this question, there is no established notion of the distance between two events
We develop a metric for the space of collider events based on the earth mover’s distance: the “work” required to rearrange the radiation pattern of one event into another
In this Letter, we advocate for the earth mover’s distance (EMD) [18,19,20,21,22] as a metric for the space of collider events
Summary
We expose interesting connections between this metric and the structure of infrared- and collinear-safe observables, providing a novel technique to quantify event modifications due to hadronization, pileup, and detector effects. We showcase how this metrization unlocks powerful new tools for analyzing and visualizing collider data without relying upon a choice of observables. High-energy particle collisions produce a tremendous number of intricately correlated particles, especially when energetic quarks and gluons are involved Behind this apparent complexity, the overall flow of energy in an event is a robust memory of its simpler partonic origins [1,2,3,4,5,6,7,8].
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