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arxiv: 1803.07168 · v2 · pith:E24J4T23new · submitted 2018-03-19 · 🌌 astro-ph.CO · gr-qc· hep-th

Anisotropic Massive Gauge-flation

classification 🌌 astro-ph.CO gr-qchep-th
keywords spacetimeanisotropicacceleratingbianchidynamicalgauge-flationhairmassive
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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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