Kinematics and Generalized Raychaudhuri equation in f(G) gravity in imperfect fluid case
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arXiv
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| Auteurs principaux: | , , |
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| Format: | Preprint |
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2024
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| _version_ | 1866913483649449984 |
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| author | Fakhri, Y. Alipour Safdarian, MOjtaba Moghaddam, S. Zamani |
| author_facet | Fakhri, Y. Alipour Safdarian, MOjtaba Moghaddam, S. Zamani |
| contents | The equation of motion is the important equation for obtain the extra force and Raychaudhuri equation. By considering an explicitly coupling between an arbitrary function of the scalar Gauss-Bonnet, G and the Lagrangian density of matter, it is shown that an extra force normal to their four-velocities arises. In this paper, we obtain the extra force and the generalized Raychaudhuri equation in F(G) modified theory of gravity in an imperfect fluid for the massive particle by divergence of energy momentum tensor so we earn extra force an Raychaudhuri equation in a compared with f(R) modified gravity for perfect fluid this conclusion giving the evolution of the kinematical quantities and describing the relative accelerations of nearby particles . |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2408_15606 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Kinematics and Generalized Raychaudhuri equation in f(G) gravity in imperfect fluid case Fakhri, Y. Alipour Safdarian, MOjtaba Moghaddam, S. Zamani General Relativity and Quantum Cosmology 58E11, 53B30, 53C50 The equation of motion is the important equation for obtain the extra force and Raychaudhuri equation. By considering an explicitly coupling between an arbitrary function of the scalar Gauss-Bonnet, G and the Lagrangian density of matter, it is shown that an extra force normal to their four-velocities arises. In this paper, we obtain the extra force and the generalized Raychaudhuri equation in F(G) modified theory of gravity in an imperfect fluid for the massive particle by divergence of energy momentum tensor so we earn extra force an Raychaudhuri equation in a compared with f(R) modified gravity for perfect fluid this conclusion giving the evolution of the kinematical quantities and describing the relative accelerations of nearby particles . |
| title | Kinematics and Generalized Raychaudhuri equation in f(G) gravity in imperfect fluid case |
| topic | General Relativity and Quantum Cosmology 58E11, 53B30, 53C50 |
| url | https://arxiv.org/abs/2408.15606 |