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arXiv:1002.4044·v6·High Energy Physics — Phenomenology

Inflatonless Inflation

Chiu Man Ho🇺🇸 · Thomas W. Kephart🇺🇸

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Abstract

We consider a 4+N dimensional Einstein gravity coupled to a non-linear sigma model. This theory admits a solution in which the N extra dimensions contract exponentially while the ordinary space expand exponentially. Physically, the non-linear sigma fields induce the dynamical compactification of the extra dimensions, which in turn drives inflation. No inflatons are required.

Comments: 12 pages, version to appear in IJMPA

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