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Inflation, braneworlds and quintessence

Greg Huey·James E. Lidsey
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Abstract

Inflationary cosmology is developed in the second Randall-Sundrum braneworld scenario, where the accelerated expansion arises through potentials that are too steep to drive inflation in conventional cosmology. A relationship between the scalar and tensor perturbation spectra is derived that is independent of both the inflaton potential and the brane tension. It is found that a single field with an inverse power law potential can act as both the inflaton and the quintessence field for suitable values of the brane tension.

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Greg Huey, James E. Lidsey. 2001-03-31. Inflation, braneworlds and quintessence. https://doi.org/10.1016/s0370-2693(01)00808-5

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