Statefinder Parameters for Different Dark Energy Models with Variable G Correction in Kaluza-Klein Cosmology

Abstract

In this work, we have calculated the deceleration parameter, statefinder parameters and EoS parameters for different dark energy models with variable $G$ correction in homogeneous, isotropic and non-flat universe for Kaluza-Klein Cosmology. The statefinder parameters have been obtained in terms of some observable parameters like dimensionless density parameter, EoS parameter and Hubble parameter for holographic dark energy, new agegraphic dark energy and generalized Chaplygin gas models.

9 pages, no figure, accepted for publication in IJTP. arXiv admin note: text overlap with arXiv:1104.2366 by other authors

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Cited by in corpus (8)

• FRW Cosmology in F(R,T) gravity
• Anisotropic massive strings in scalar-tensor theory of gravitation
• Reconstructing $f(T)$ modified gravity from ECHDE and ECNADE models
• Reconstructions of $f(\mathcal{P})$ and $f(\mathcal{Q})$ gravity models from $(m,n)$-type Barrow Holographic Dark Energy: Analysis and Observational Constraints
• Observational constraints on G-corrected holographic dark energy using a Markov chain Monte Carlo method
• Reconstructions of Einstein-Aether Gravity from Barrow Agegraphic and New Barrow Agegraphic Dark Energy models: Examinations and Observational Limits
• Observational constraints on models of the Universe with time variable Gravitational and Cosmological constants along MOG
• Loop Quantum Corrections to Statefinder Parameters of Dark Energy