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arxiv: 1103.5623 · v3 · pith:P4YKQ2JAnew · submitted 2011-03-29 · ✦ hep-th · astro-ph.CO· hep-ph

Warming up brane-antibrane inflation

classification ✦ hep-th astro-ph.COhep-ph
keywords inflationadditionalbrane-antibraneconstructionsalleviatingamountassociatedbranes
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We show that, in constructions with additional intersecting D-branes, brane-antibrane inflation may naturally occur in a warm regime, such that strong dissipative effects damp the inflaton's motion, greatly alleviating the associated eta-problem. We illustrate this for D3-antiD3 inflation in flat space with additional flavor D7-branes, where for both a Coulomb-like or a quadratic hybrid potential a sufficient number of e-folds may be obtained for perturbative couplings and O(10-10^4) branes. This is in clear contrast with the corresponding cold scenarios, thus setting the stage for more realistic constructions within fully stabilized compactifications. Such models generically predict a negligible amount of tensor perturbations and non-gaussianity f_NL \sim O(10).

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