Study of some chaotic inflationary models in \(f(R)\) gravity
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In this paper, we discuss an inflationary scenario via scalar field and fluid cosmology for an anisotropic homogeneous universe model in \(f(R)\) gravity. We consider an equation of state which corresponds to a quasi-de Sitter expansion and investigate the effect of the anisotropy parameter for different values of the deviation parameter. We evaluate potential models like linear, quadratic and quartic models which correspond to chaotic inflation. We construct the observational parameters for a power-law model of \(f(R)\) gravity and construct the graphical analysis of tensor–scalar ratio and spectral index which indicates the consistency of these parameters with Planck 2015 data.
KeywordsInflation \(f(R)\) gravity Slow-roll approximation
This work has been supported by the Pakistan Academy of Sciences Project.
- Sharif, M., Nawazish, I.: Int. J. Mod. Phys. 26, 1750191 (2017b) Google Scholar