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Strong Coupling and Classicalization

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arxiv 1607.07422 v1 pith:GIX4ZUI7 submitted 2016-07-25 hep-th gr-qchep-exhep-ph

classification hep-thgr-qchep-exhep-ph
keywords classicalizationmustquantasoftcouplingstrongelementaryenergies
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Classicalization is a phenomenon in which a theory prevents itself from entering into a strong-coupling regime, by redistributing the energy among many weakly-interacting soft quanta. In this way, the scattering process of some initial hard quanta splits into a large number of soft elementary processes. In short, the theory trades the strong coupling for a high-multiplicity of quanta. At very high energies, the outcome of such a scattering experiment is a production of soft states of high occupation number that are approximately classical. It is evident that black hole creation in particle collision at super-Planckian energies is a result of classicalization, but there is no a priory reason why this phenomenon must be limited to gravity. If the hierarchy problem is solved by classicalization, the LHC has a chance of detecting a tower of new resonances. The lowest-lying resonances must appear right at the strong coupling scale in form of short-lived elementary particles. The heavier members of the tower must behave more and more classically: they must be longer lived and decay into higher numbers of soft quanta.

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  1. Light scalars in light of UV/IR mixing: classicalization via synergy between Vainshtein and chameleon screenings

    hep-ph 2025-11 conditional novelty 5.0 of 10

    Classicalizing k-essence scalars need m << Λ* and, when potentials or fermion couplings are present, a chameleon-like screening layer to keep Vainshtein screening and classicalon stability intact.

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