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Mass Gap in Infinite Derivative Non-local Higgs: Dyson-Schwinger Approach

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arxiv 2011.10586 v3 pith:K2KSRSZW submitted 2020-11-20 hep-th

classification hep-th
keywords non-localhiggstheorydyson-schwingerinfinitelocalmassnon-perturbative
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We investigate the non-perturbative degrees of freedom in the class of non-local Higgs theories that have been proposed as an ultraviolet completion 4-D Quantum Field Theory (QFT) generalizing the kinetic energy operators to an infinite series of higher derivatives inspired by string field theory. At the perturbative level, the degrees of freedom of non-local Higgs are the same of the local theory. We prove that, at the non-perturbative level, the physical spectrum of the Higgs mass is actually corrected from the "infinite number of derivatives" present in the action. The technique we use permits to derive the set of Dyson-Schwinger equations in differential form. This proves essentially useful when exact solutions to the local equations are known. We show that all the formalism of the local theory involving the Dyson-Schwinger approach extends quite naturally to the non-local case. Using these methods, the spectrum of non-local theories become accessible and predictable in the non-perturbative regimes. We calculate the N-point correlation functions and predict the mass-gap in the spectrum arising purely from the self-interaction and the non-local scale M. The mass gap generated gets damped in the UV and it reaches conformal limit. We discuss some implications of our result in particle physics and cosmology.

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  1. Quintessence Dark Energy from non-perturbative Higgs-Yang-Mills mass gap

    astro-ph.CO 2025-05 reject novelty 4.0 of 10

    A strongly coupled Higgs-Yang-Mills dark sector with a cosmic-triad gauge field can mimic quintessence dark energy with an equation of state approaching -1, provided the solution phase is tuned.

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