Abstract
In this paper, we have constructed the cosmological models of the universe in a cylindrically symmetric space time in two classes of \(f(R,T)\) gravity (Harko et al. in Phys. Rev. D 84:024020, 2011). We have discussed two cases: one in the linear form and the other in the quadratic form of \(R\). The matter is considered to be in the form of perfect fluid. It is observed that in the first case, the pressure and energy density remain the same, which reduces to a Zeldovich fluid. In the second case we have studied the quadratic function of \(f(R,T)\) gravity in the form \(f(R)=\lambda(R+R^{2})\) and \(f(T)=\lambda T\). In the second case the pressure is in the negative domain and the energy density is in the positive domain, which confirms that the equation of state parameter is negative. The physical properties of the constructed models are studied.
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Acknowledgements
The authors are extremely grateful to the anonymous referee for his valuable suggestions to improve the quality and standard of the manuscript. The authors are also thankful to Mr. Pratik P. Ray and Mr. Sankarsan Tarai for their help in the revision process. BM acknowledges SERB-DST, New Delhi, India for financial support to carry out the Research project [No. SR/S4/MS:815/13].
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Mishra, B., Vadrevu, S. Cylindrically symmetric cosmological model of the universe in modified gravity. Astrophys Space Sci 362, 26 (2017). https://doi.org/10.1007/s10509-017-3006-2
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DOI: https://doi.org/10.1007/s10509-017-3006-2