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Anisotropic Massive Gauge-flation

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arxiv 1803.07168 v2 pith:E24J4T23 submitted 2018-03-19 astro-ph.CO gr-qchep-th

classification astro-ph.COgr-qchep-th
keywords spacetimeanisotropicacceleratingbianchidynamicalgauge-flationhairmassive
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abstract

We study anisotropic inflationary solutions in massive Gauge-flation. We work with the theory in both the Stueckelberg and dynamical symmetry-breaking limits and demonstrate that extended periods of accelerated anisotropic expansion are possible. In the case of dynamical symmetry breaking, we show that spacetime can transition from isotropic quasi-de Sitter space to an accelerating Bianchi spacetime due to a rolling Higgs field - the spacetime can develop hair. Similarly, symmetry restoring transitions are possible from accelerating Bianchi spacetime to quasi-de Sitter space - the spacetime can lose its hair. These transitions can be arranged to occur quickly, within an $e$-folding or so, or over tens of $e$-folds.

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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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