Warm inflation on the brane

M. Antonella Cid, Sergio Del Campo, Ramón Herrera

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34 Scopus citations


In this paper, warm inflationary models on a brane scenario are studied. Here we consider slow-roll inflation and a high-dissipation regime in a high-energy scenario. General conditions required for these models to be realizable are derived. We describe scalar and tensor perturbations for these scenarios. Specifically we study the power-law potentials considering a dissipation parameter to be a constant on the one hand and dependent on the other hand. We use recent astronomical observations to restrict the parameters appearing in our model.

Original languageEnglish
Article number005
JournalJournal of Cosmology and Astroparticle Physics
Issue number10
StatePublished - 1 Oct 2007


  • Cosmological perturbation theory
  • Cosmology with extra dimensions
  • Inflation
  • Physics of the early universe


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