Anisotropic viable solutions of stellar structures in modified teleparallel gravity

Abstract

The commitment behind this work is to find the solutions of compact stellar models by using the spherically symmetric static space-time and anisotropic matter distribution in the framework of [Formula: see text] gravity. In this study, we used the new type of metric functions [Formula: see text] and evaluated other functions [Formula: see text] by the well-known Karmarkar condition. In this work, we use the rotated and spinning tetrad named as off-diagonal and most generic function of [Formula: see text] gravity. We find the strange stellar solutions by incorporating the MIT bag equation of state [Formula: see text] to evaluate cosmological constant. Aiming at the simplicity of solutions we utilize the given data for masses and radii of compact objects PSR J1416-2230, 4 U 1608-52, Cen X-3, EXO 1785-248, SMC X-1. By graphical presentation of the core properties of compact models, we show by concluding that our solutions are graphically fit and physically admissible and interesting by having the compatibility with the compact stars study.