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Bianchi-III cosmological model with BVDP in modified \(f(R,T)\) theory

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Abstract

In present paper, we have investigated Bianchi type-III cosmological model in modified \(f(R,T)\) theory of gravity as proposed by Harko et al. (Phys. Rev. D 84:024020, 2011). To find the solution of field equations, we have used i) bilinear varying deceleration parameter (BVDP) (Mishra et al. in Astrophys. Space Sci. 361:259, 2016b) ii) the fact that expansion scalar of the space-time is proportional to the one of the components of the shear scalar. Physical and geometrical properties of the model have also been discussed along with the pictorial representation of various parameters. We have observed that presented model is compatible with the recent cosmological observations.

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Acknowledgements

The authors are highly thankful to the anonymous referees for their valuable comments and suggestions to improve this manuscript.

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Authors and Affiliations

  1. Department of Mathematics, Sant Longowal Institute of Engineering and Technology, Deemed University, Under MHRD, Govt. of India, Longowal, 148 106, Punjab, India

    R. K. Mishra, Heena Dua & Avtar Chand

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  1. R. K. Mishra
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  2. Heena Dua
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  3. Avtar Chand
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Correspondence to R. K. Mishra.

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Mishra, R.K., Dua, H. & Chand, A. Bianchi-III cosmological model with BVDP in modified \(f(R,T)\) theory. Astrophys Space Sci 363, 112 (2018). https://doi.org/10.1007/s10509-018-3336-8

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