Abstract
In this paper, we investigate the effects of torsion and shears within the framework of the gravitational field with torsion in early and late cosmology. General relativity and torsion field equations are constructed using absolute parallel geometry. The Big Rip model of the Universe has been presented using a special class of Riemann–Cartan geometry and the law of variation of Hubble’s parameter. The model does not depend on the curvature constant. The positive condition of the energy density of the matter is satisfied in this model. This cosmological model shows that the torsion and shear effect is strong at the beginning of the Big Bang and at the end of the universe. Through the examination of precise cases of the parameters and initial conditions, we can show that for suitable ranges of the parameters, the dynamic torsion scalar model can exhibit features similar to those of the currently observed accelerating universe. The relationship between the torsion and shear scalars is investigated, and their impact on the accelerating universe is addressed apart from the idea of dark energy.
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07 April 2023
The original version of this article has been revised: a typo in authors’ affiliations 2 and 4 has been corrected.
06 April 2023
A Correction to this paper has been published: https://doi.org/10.1007/s10509-023-04188-0
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Acknowledgements
The authors extend their appreciation to the Deanship of Scientific Research at Imam Mohammad Ibn Saud Islamic University, KSA for funding this work through Research Group no. RG-21-09-42. Also, the authors would like to express their deep gratitude to Prof. M. I. Wanas and Prof. M. I. Kahil for their deep interest and valuable comments during extraction of this work.
Funding
This research was funded by Imam Mohammad Ibn Saud Islamic University, KSA, Research Group no. RG-21-09-42.
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Conceptualization: M. A. Bakry and A. Eid; investigation: M. A. Bakry, A. Eid, and M. M. Khader; methodology: M. A. Bakry and A. Eid; formal analysis: M. A. Bakry and A. Eid; writing: M. A. Bakry and A. Eid; validation: M. A. Bakry, A. Eid, and M. M. Khader. All authors have read and agreed to the published version of the manuscript.
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Bakry, M.A., Eid, A. & Khader, M.M. Torsion and shear effect on a Big Rip model in a gravitational field. Astrophys Space Sci 366, 97 (2021). https://doi.org/10.1007/s10509-021-04002-9
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DOI: https://doi.org/10.1007/s10509-021-04002-9