Charged Stellar Models with Anisotropic Pressure Similar to Experimental Data

Malaver M

Published on: 2025-05-05

Abstract

In this research, we discovered a new class of solutions to the Einstein-Maxwell field equations with anisotropic distribution that take into account a linear equation of state and a specific choice of electric field strength. The new exact models meet key physical variables including mass, radial pressure, and measure of anisotropy, which can be expressed in terms of elementary and polynomial functions, because are physically plausible and behave well in the stellar interior. The values obtained are in agreement with the compact star limit mass of J1018-1523, J1946+2052, J0952-0607 and J1311-3430.