Stability of Higher Dimensional Plane Symmetric Space-Time with Wet Dark Fluid Within the Framework of π(πΉ,π») Theory of Gravity.
Abstract In this research article, we focus on the investigation of the stability of five-dimensional Planesymmetric space-time with Wet Dark Fluid in the presence of f(R, T) theory of gravitation. Weuse Hubbleβs law to find the exact solution. Also, we studied the physical parameters of the modelin terms of redshift and explained the energy conditions, stability of the model, and statefinderparameter of the model. We also discussed look-back time, proper distance, luminosity distance,angular diameter, cosmic snap parameter, and jerk parameter and their graphical representation.
Institutions
- Shivaji University (IN)
Publication Details
- Journal
- Zenodo (CERN European Organization for Nuclear Research)
- Published
- 2025-10-25
- DOI
- https://doi.org/10.5281/zenodo.17441061
- Primary Topic
- Cosmology and Gravitation Theories
- Type
- article
- Field-Weighted Citation Impact
- 0.00