Viscous fluid accelerating model in modified gravity

Author:

Tarai Sankarsan1,Ray Pratik P.2,Mishra B.3ORCID,Tripathy S. K.4

Affiliation:

1. Centre of High Energy and Condensed Matter Physics, Department of Physics, Utkal University, Vani Vihar, Bhubaneswar 751004, India

2. Department of Mathematics (SSL), Vellore Institute of Technology-Andhra Pradesh University, Andhra Pradesh 522237, India

3. Department of Mathematics, Birla Institute of Technology and Science-Pilani, Hyderabad Campus, Hyderabad 500078, India

4. Department of Physics, Indira Gandhi Institute of Technology, Sarang, Dhenkanal, Odisha 759146, India

Abstract

In the framework of extended theory of gravity, an accelerating cosmological model has been presented in this paper in an anisotropic space-time. The extended gravity is considered as [Formula: see text] gravity with the matter field as viscous fluid. The role of viscous coefficient has been discussed on the cosmic expansion issue. In the developed formalism, a variable Hubble parameter has been incorporated to express the dynamical parameter with respect to redshift. The model is observed to be compatible with recent observational data.

Publisher

World Scientific Pub Co Pte Ltd

Subject

Physics and Astronomy (miscellaneous)

Cited by 6 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Bulk viscous cosmological model in F(T) gravity;International Journal of Geometric Methods in Modern Physics;2024-08-21

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3. Reconstruction of F(T,TG) gravity model with scalar fields;International Journal of Geometric Methods in Modern Physics;2024-04-30

4. Observational constraint in f(R, ∇R) gravity model in power-law cosmology;Canadian Journal of Physics;2024-04-01

5. Observational constraints for an axially symmetric transitioning model with bulk viscosity parameterization;Astronomy and Computing;2023-10

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