Warming up brane-antibrane inflation

Mar Bastero-Gil, Arjun Berera, and João G. Rosa
Phys. Rev. D 84, 103503 – Published 2 November 2011

Abstract

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 η-problem. We illustrate this for D3-D3¯ inflation in flat space with additional flavor D7 branes, where for a Coulomb-like or quadratic hybrid potential a sufficient number of e-folds may be obtained for perturbative couplings and O(10104) 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 fNLO(10).

  • Figure
  • Figure
  • Received 29 March 2011

DOI:https://doi.org/10.1103/PhysRevD.84.103503

© 2011 American Physical Society

Authors & Affiliations

Mar Bastero-Gil1,*, Arjun Berera2,†, and João G. Rosa2,‡

  • 1Departamento de Física Teórica y del Cosmos, Universidad de Granada, Granada-18071, Spain
  • 2SUPA, School of Physics and Astronomy, University of Edinburgh, Edinburgh, EH9 3JZ, United Kingdom

  • *mbg@ugr.es
  • ab@ph.ed.ac.uk
  • joao.rosa@ed.ac.uk

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Issue

Vol. 84, Iss. 10 — 15 November 2011

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