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Aspects of some new versions of pilgrim dark energy in DGP braneworld

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Abstract.

The illustration of cosmic acceleration under two interacting dark energy models (pilgrim dark energy with Granda-Oliveros cutoff and its generalized ghost version) in the DGP braneworld framework is presented. In the current scenario, the equation of state parameter, deceleration parameter, \( \omega_{D}\) - \( \omega^{\prime}_{D}\) plane and statefinder diagnosis are investigated. The equation of state parameter behaves like the phantom era of the universe. The deceleration parameter shows the accelerated expansion of the universe in both models. The cosmological planes, like \( \omega_{D}\) - \( \omega^{\prime}_{D}\), and the statefinder correspond to the \( \Lambda\) CDM limit. To conclude, we remark that our results support the phenomena of pilgrim dark energy and cosmic acceleration. Also, the results are consistent with observational data.

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Authors and Affiliations

  1. Department of Mathematics, COMSATS Institute of Information Technology, Lahore, Pakistan

    Abdul Jawad & Shamaila Rani

  2. Institut de Mathématiques et de Sciences Physiques (IMSP), 01 BP 613, Porto-Novo, Benin

    Ines G. Salako

  3. Département de Physique, Université d’Agriculture de Kétou, BP 13, Kétou, Benin

    Ines G. Salako

  4. Department of Mathematics, Lahore Leads university, 54590, Lahore, Pakistan

    Faiza Gulshan

Authors
  1. Abdul Jawad
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  2. Shamaila Rani
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  3. Ines G. Salako
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  4. Faiza Gulshan
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Correspondence to Abdul Jawad.

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Jawad, A., Rani, S., Salako, I. et al. Aspects of some new versions of pilgrim dark energy in DGP braneworld. Eur. Phys. J. Plus 131, 236 (2016). https://doi.org/10.1140/epjp/i2016-16236-x

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  • DOI: https://doi.org/10.1140/epjp/i2016-16236-x

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