Abstract
The spatially homogeneous shear-free, rotating and expanding Bianchi type-IX universe has been considered in the presence of perfect fluid in \(f(R,T)\) theory of gravity. The exact solution of the field equations has been obtained and the functional form of \(f(R,T)=R+2f(T)\) gravity has been reconstructed. The existence of such a solution suggests that the general relativistic shear-free perfect fluid conjecture which claims that a shear-free perfect fluid cannot rotate and expand at the same time, is not valid in this modified theory.
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Acknowledgements
I would like to thank the anonymous referee for fruitful suggestions. The author is supported by Istanbul University Scientific Research Projects (BAP) under project number 52210.
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Appendices
Appendix A: Evolution and constraint equations of \(f(R,T)\) gravity
1.1 A.1 Evolution equations
1.2 A.2 Constraint equations
where \(E_{ab}\) and \(H_{ab}\) are the electric (\(E_{ab} = C_{aebd}u^{e}u^{d}\)) and the magnetic (\(H_{ab} = (1/2){\varepsilon_{a}}^{cd}C_{cdbe}u^{e}\)) parts of the conformal Weyl curvature tensor \(C_{abcd}\).
Appendix B: Dynamic quantities of the rotating Bianchi type-IX model
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Sofuoğlu, D. Rotating and expanding Bianchi type-IX model in \(f(R,T)\) theory of gravity. Astrophys Space Sci 361, 12 (2016). https://doi.org/10.1007/s10509-015-2593-z
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DOI: https://doi.org/10.1007/s10509-015-2593-z