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Observational Constraints on the Chaplygin Gas with Inverse Power Law Potential in Braneworld Inflation

  • Astronomy, Astrophysics, and Cosmology
  • Published:
Moscow University Physics Bulletin Aims and scope

Abstract

We study Chaplygin gas as a candidate for inflation in the context of braneworld inflationary model. We investigate this model in the framework of the Randall–Sundrum type II, considering a original and generalized Chaplygin gas. We use inverse power law potential to examine the behavior of some inflationary spectrum parameters such as the spectral index ns, the ratio r and the running of the scalar spectral index dns/dlnk, our results are in agreement with recent observational data for a particular choice of e-folding number N and parameters space of the model.

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Authors and Affiliations

  1. Equipe Physique Quantique et Applications, Laboratoire de Physique de la Matière Condensée, Faculté des Sciences Ben M’sik, Université Hassan II, Casablanca, Morocco

    F. Salamate, I. Khay, A. Safsafi, H. Chakir & M. Bennai

  2. Equipe de Recherche Subatomique et Applications, Laboratoire de Physique de la Matière Condensée, Faculté des Sciences Ben M’sik, Université Hassan II, Casablanca, Morocco

    F. Salamate, I. Khay, A. Safsafi & H. Chakir

  3. Groupement National de Physique des Hautes Energies, Focal point, LabUFR-PHE, Rabat, Morocco

    A. Safsafi, H. Chakir & M. Bennai

Authors
  1. F. Salamate
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  2. I. Khay
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  3. A. Safsafi
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  4. H. Chakir
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  5. M. Bennai
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Correspondence to A. Safsafi.

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Salamate, F., Khay, I., Safsafi, A. et al. Observational Constraints on the Chaplygin Gas with Inverse Power Law Potential in Braneworld Inflation. Moscow Univ. Phys. 73, 405–412 (2018). https://doi.org/10.3103/S0027134918040124

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  • DOI: https://doi.org/10.3103/S0027134918040124

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