Relativistic anisotropic solution satisfying vanishing complexity condition

Abstract

In this paper, we investigated anisotropic solution for a self-bound compact star model. The solution is obtained via Vaidya–Tikekar metric function [Formula: see text] and the vanishing complexity factor condition. The physical analysis of the solution has been discussed in detail which includes mass-radius ratio, and stability analysis via adiabatic index for a secondary component of the GW190814 event for different values [Formula: see text]. Furthermore, we predicted the radii and obtained the compactness factor of different self-bound compact objects for different [Formula: see text]. Moreover, the hydrostatic equilibrium condition of the solution is also checked. The physical result shows that the solution so obtained is well behaved and may be useful for modeling the self-bound compact objects as far as observational data is concerned.