An analytical anisotropic compact stellar model of embedding class I

A class of solutions Einstein field equations satisfying Karmarkar embedding condition is presented which could describe static, spherical fluid configurations, and serve as models for compact stars. The under consideration has unequal principal stresses i.e. locally anisotropic. certain physically motivated geometry metric potential been chosen codependency the potentials outlines formation model. exterior spacetime assumed described by Schwarzschild solution. smooth matching interior to across boundary that radial pressure zero lead us determine model parameters. Physical requirements stability analysis demanded a realistic star are satisfied. developed investigated graphically exploring data from some known objects. mass-radius (M-R) relationship shows maximum mass admissible observed pulsars given surface density also investigated. Moreover, physical profile moment inertia (I) thus obtained confirmed Bejger–Haensel concept.