Statefinder Parameters for Five-Dimensional Cosmology

Abstract

We study the statefinder parameter in the five-dimensional big bounce model, and apply it to differentiate the attractor solutions of quintessence and phantom field. It is found that the evolving trajectories of these two attractor solutions in the statefinder parameters plane are quite different, and that are different from the statefinder trajectories of other dark energy models.

8 pages, 12 figures. accepted by MPLA

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Cited by in corpus (9)

• Statefinder Diagnosis for Ricci Dark Energy
• Interacting model of new agegraphic dark energy: Cosmological evolution and statefinder diagnostic
• Dynamical systems methods and statefinder diagnostic of interacting vacuum energy models
• Growth index and statefinder diagnostic of Oscillating Dark Energy
• Statefinder diagnosis for the extended holographic Ricci dark energy model without and with interaction
• Reconstructions of $f(\mathcal{P})$ and $f(\mathcal{Q})$ gravity models from $(m,n)$-type Barrow Holographic Dark Energy: Analysis and Observational Constraints
• Scalar field descriptions of two dark energy models
• Reconstructions of Einstein-Aether Gravity from Barrow Agegraphic and New Barrow Agegraphic Dark Energy models: Examinations and Observational Limits
• Thermodynamics of Apparent Horizon and Friedmann Equations in Big Bounce Universe