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Anisotropic Model with Constant Jerk Parameter in \(\boldsymbol{f(R,T)}\) Gravity

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Abstract

In the context of \(f(R,T)\) modified gravity theory, we consider a homogeneous and anisotropic Bianchi type-I cosmological model which relies on the condition of a constant jerk parameter, \(j=1\), corresponding to a flat \(\Lambda\)CDM model. Under this condition, we obtain two different solutions, one is power-law and the other one is exponential. The power-law solution gives a decelerating model, while the exponential one yields an accelerating cosmology. We discuss the physical and geometric properties of both models, validity of the solutions, and the significance of modified \(f(R,T)\) gravity for the models.

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ACKNOWLEDGMENTS

We are grateful to the reviewer for illuminating suggestions that have improved our study.

Funding

D.S. is supported by the Istanbul University Scientific Research Projects (BAP) Unit under project number BYP-2019-34605.

Author information

Authors and Affiliations

  1. Department of Mathematics,Government Model Science College, Rewa-486 001, Madhya Pradesh, India

    R. K. Tiwari & S. K. Mishra

  2. Department of Physics,Faculty of Science, Istanbul University, Vezneciler, 34134, Fatih, Istanbul, Turkey

    D. Sofuoglu

  3. Department of Mathematical Sciences, University of Zululand, 3886, Kwa-Dlangezwa, South Africa

    A. Beesham

  4. Faculty of Natural Sciences, Mangosuthu University of Technology, 4026, Umlazi, South Africa

    A. Beesham

Authors
  1. R. K. Tiwari
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  2. D. Sofuoglu
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  3. S. K. Mishra
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  4. A. Beesham
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Corresponding authors

Correspondence to R. K. Tiwari, D. Sofuoglu, S. K. Mishra or A. Beesham.

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Tiwari, R.K., Sofuoglu, D., Mishra, S.K. et al. Anisotropic Model with Constant Jerk Parameter in \(\boldsymbol{f(R,T)}\) Gravity. Gravit. Cosmol. 28, 196–203 (2022). https://doi.org/10.1134/S0202289322020141

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  • DOI: https://doi.org/10.1134/S0202289322020141

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