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 1/W(r)=K+Cr2K(1+Cr2)1/W(r)=K+Cr2K(1+Cr2) 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 K. Furthermore, we predicted the radii and obtained the compactness factor of different self-bound compact objects for different K. 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.
