UV-Completion by Classicalization
Gia Dvali, Gian F. Giudice, Cesar Gomez, Alex Kehagias

TL;DR
This paper introduces a novel classicalization approach for UV-completion of non-renormalizable theories, where classical objects called classicalons unitarize high-energy scattering amplitudes, with significant implications for the Standard Model and collider phenomenology.
Contribution
It proposes classicalization as a new mechanism for UV-completion, involving classicalons formed by classicalizer fields, applicable to non-gravitational theories like the Standard Model.
Findings
Classicalons can unitarize high-energy scattering amplitudes.
Classicalization applies to Higgsless and Higgs scenarios in the Standard Model.
Distinct experimental signatures are predicted at the LHC.
Abstract
We suggest a novel approach to UV-completion of a class of non-renormalizable theories, according to which the high-energy scattering amplitudes get unitarized by production of extended classical objects (classicalons), playing a role analogous to black holes, in the case of non-gravitational theories. The key property of classicalization is the existence of a classicalizer field that couples to energy-momentum sources. Such localized sources are excited in high-energy scattering processes and lead to the formation of classicalons. Two kinds of natural classicalizers are Nambu-Goldstone bosons (or, equivalently, longitudinal polarizations of massive gauge fields) and scalars coupled to energy-momentum type sources. Classicalization has interesting phenomenological applications for the UV-completion of the Standard Model both with or without the Higgs. In the Higgless Standard Model the…
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