Dynamics of tilted massive stellar object in high curvature gravity
| dc.contributor.author | Maria Arshad | |
| dc.date.accessioned | 2025-11-23T12:53:44Z | |
| dc.date.available | 2025-11-23T12:53:44Z | |
| dc.date.issued | 2023-07-26 | |
| dc.description.abstract | The dynamics of Lemaitre-Tolman-Bondi space-time is examined in the setting of a tilted viewer in a form of f(R) gravitation, and a significant connection between tilted and non-tilted observers is found. The addition of the non-universal function of the Ricci scalar in the Einstein-field action concludes to characterize f(R) theory, which stands for accelerated expansion, when determining the updated field equations. Now we determine the role of tilted and non-tilted coherence in the act of dissipative LTB in f(R). Now use kinematical and dynamical variables to discuss the inhomogeneity factors and its growth. It has been discovered that emergence of inhomogeneity factors which depends upon the heat transformation, shear tensor, and addition of scalar for tilted viewer, whereas for non-tilted observers, it depends only on the shear tensor. Additionally, we investigate the non-tilted congruence stability requirements in the presence of dark source terms and indicates that instability of the non-tilted coherence caused by expansion. | |
| dc.identifier.uri | https://escholar.umt.edu.pk/handle/123456789/12239 | |
| dc.language.iso | en | |
| dc.publisher | UMT Lahore | |
| dc.title | Dynamics of tilted massive stellar object in high curvature gravity | |
| dc.type | Thesis |
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