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Higher order corrections of the extended Chaplygin gas cosmology with varying G and Λ

  • E. O. Kahya
  • , M. Khurshudyan
  • , B. Pourhassan*
  • , R. Myrzakulov
  • , A. Pasqua
  • *Bu çalışma için yazışmadan sorumlu yazar
  • Max Planck Institute of Colloids and Interfaces
  • Damghan University
  • L.N. Gumilyov Eurasian National University
  • University of Trieste

Araştırma sonucu: Dergiye katkıMakalebilirkişi

65 Atıf (Scopus)

Özet

In this paper, we study two different models of dark energy based on the Chaplygin gas equation of state. The first model is the variable modified Chaplygin gas, while the second one is the extended Chaplygin gas. Both models are considered in the framework of higher order f(R) modified gravity. We also consider the case of time-varying gravitational constant G and Λ for both models. We investigate some cosmological parameters such as the Hubble, the deceleration, and the equation of state parameters. Then we show that the model that we consider, the extended Chaplygin gas with time-dependent G and Λ, is consistent with the observational data. Finally we conclude with the discussion of cosmological perturbations of our model.

Orijinal dilİngilizce
Makale numarası43
Sayfa (başlangıç-bitiş)1-12
Sayfa sayısı12
DergiEuropean Physical Journal C
Hacim75
Basın numarası2
DOI'lar
Yayın durumuYayınlandı - 2015

Bibliyografik not

Publisher Copyright:
© 2015, The Author(s).

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