Compact relativistic geometries in gravity
arXiv:2203.08814 · doi:10.1142/S0219887822501262
Abstract
One of the possible potential candidates for describing the universe's rapid expansion is modified gravity. In the framework of the modified theory of gravity , the present work features the materialization of anisotropic matter, such as compact stars. Specifically, to learn more about the physical behavior of compact stars, the radial, and tangential pressures as well as the energy density of six stars namely , , , , , and are calculated. Herein, the modified theory of gravity is disintegrated into two parts i.e. the hyperbolic model and the three different model. The study focuses on graphical analysis of compact stars wherein the stability aspects, energy conditions, and anisotropic measurements are mainly addressed. Our calculation revealed that, for the positive value of parameter n of the model , all the six stars behave normally.
arXiv commentSome changes have been made. " To appear in International Journal of Geometric Methods in Modern Physics"
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