Gravity-Assisted Emergent Higgs Mechanism in the Post-Inflationary Epoch
Eduardo Guendelman, Emil Nissimov, Svetlana Pacheva

TL;DR
This paper proposes a novel gravity model with non-Riemannian volume-forms that naturally generates a Higgs-like potential and flat inflationary regions, offering insights into early universe symmetry breaking.
Contribution
It introduces a gravity framework using non-Riemannian volume-forms that dynamically produce Higgs-like symmetry breaking without additional degrees of freedom.
Findings
Emergence of flat regions in the inflaton potential.
Dynamical generation of Higgs-like symmetry breaking potential.
No additional propagating degrees of freedom introduced.
Abstract
We consider a non-standard model of gravity coupled to a neutral scalar "inflaton" as well as to SU(2)xU(1) iso-doublet scalar with positive mass squared and without self-interaction, and to SU(2)xU(1) gauge fields. The principal new ingredient is employing two alternative non-Riemannian space-time volume-forms (covariant integration measure densitities) independent of the metric. The latter have a remarkable impact - although not introducing any additional propagating degrees of freedom, their dynamics triggers a series of important features: appearance of infinitely large flat regions of the effective "inflaton" potential as well as dynamical generation of Higgs-like spontaneous symmetry breaking effective potential for the SU(2)xU(1) iso-doublet scalar.
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