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Intermediate inflation on the brane and warped DGP models

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Abstract

Brane and warped Dvali–Gabadadze–Porrati inflationary universe models in the context of intermediate inflation are studied. In both models we consider that the energy density is a standard scalar field and we discuss the evolution of the universe during the slow-roll inflation. Also, we describe the conditions for these models. The corresponding Wilkinson Microwave Anisotropy Probe seven-year data are utilized to fix some parameters in our models. Our results are compared to those found in general relativity.

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Notes

  1. A complete description of inflationary scenarios can be found in [3].

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Acknowledgements

R.H. was supported by COMISION NACIONAL DE CIENCIAS Y TECNOLOGIA through FONDECYT grant N0 1130628 and by DI-PUCV grant 123.724. M.O. was supported by Proyecto D.I. PostDoctorado 2012 PUCV. N.V. was supported by Proyecto Beca-Doctoral CONICYT N0 21100261.

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  1. Instituto de Física, Pontificia Universidad Católica de Valparaíso, Casilla, 4059, Valparaíso, Chile

    Ramón Herrera, Marco Olivares & Nelson Videla

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  1. Ramón Herrera
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  2. Marco Olivares
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  3. Nelson Videla
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Correspondence to Ramón Herrera.

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Herrera, R., Olivares, M. & Videla, N. Intermediate inflation on the brane and warped DGP models. Eur. Phys. J. C 73, 2475 (2013). https://doi.org/10.1140/epjc/s10052-013-2475-x

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