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arxiv: 0903.5297 · v1 · submitted 2009-03-30 · 🌌 astro-ph.CO · astro-ph.HE· gr-qc· hep-ph· hep-th

Impact of Lorentz violation on the dynamics of inflation

classification 🌌 astro-ph.CO astro-ph.HEgr-qchep-phhep-th
keywords inflationlorentzdynamicsflatnessinflationaryinflatonmodelsnecessary
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This work deals with the dynamics of inflation in the context of a scalar-vector-tensor theory of gravity exhibiting spontaneous Lorentz violation at early times. We describe a first-order formalism which we use to obtain new exact Lorentz violating inflationary solutions for a broad family of models, some in the absence of a potential for the inflaton field. Our results show that different conditions are required to solve the horizon and flatness problems. In particular, we find a necessary condition for inflation to provide a solution to both problems and we show that in inflationary models with no inflaton potential a period of superinflation might be necessary to solve the flatness problem.

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