An Examination of the General Relativity of the Bianchi type V Holographic Dark Energy Model Using the Hybrid Expansion Law

Abstract

This examination presents an investigation of the qualities of anisotropic and homogeneous Bianchi type V space-time inside the setting of general relativity, while considering the consideration of dark matter and holographic dark energy model parts. The arrangements of the differential condition fields have been determined by looking at two unmistakable situations: one where the extension scalar in the model is straightforwardly relative to the shear scalar, and one more where the typical scale factor is expected to follow a half breed development structure. The answers for the field conditions are inferred inside the system of general relativity. A similar to peculiarity was found with regards to the tension and condition of state boundary of the holographic dark energy model inside their separate settings. This study researches the physical and mathematical parts of a few factors that hold infinite importance, including the jerk boundary inside our model. The noticed boundaries line up with the cosmological models that portray the present status of the universe, described by sped up extension. All in all, we state that our model looks very similar to the ΛCDM cosmological model all through the later stages and lines up with the most recent discoveries of cosmological information.