The key role of Lagrangian multiplier in mimetic gravitational theory in the frame of isotropic compact star

Abstract

Recently, the mimetic gravitational theory has gained much attention in the frame of cosmology as well as in the domain of astrophysics. In this study, we show that in the frame of mimetic gravitation theory we are not able to derive an isotropic model. As a result, our focus shifts towards combining mimetic gravitational theory with the Lagrangian multiplier. The field equations of a static isotropic gravitational system that controls the geometry and dynamics of star structure are studied in the frame of mimetic theory coupled with a Lagrangian multiplier using a non-linear equation of state. An energy density is assumed from where all the other unknowns are fixed and a new isotropic model is derived. The physical analysis of this model is studied from different viewpoints and consistent results compatible with a realistic isotropic star are investigated analytically and graphically. Ultimately, we demonstrate the stability of the model in question by employing the adiabatic index technique.

12 pages 6 figures

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Cited by in corpus (4)

• Event Horizon Telescope observations exclude compact objects in baseline mimetic gravity
• Anisotropic Stellar Models with Tolman IV Spacetime in Non-minimally Coupled Theory
• Mimetic Weyl geometric gravity
• Holographic description of unified early and late universe in viscous mimetic gravity