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This paper studies the influence of charge on a compact stellar structurealso regarded as vacuum condensate star in the background of$f(\mathfrak{R},\mathcal{T}^{2})$ gravity. This object is considered thealternate of black hole whose structure involves three distinct regions, i.e.,interior, exterior and thin-shell. We analyze these domains of a gravastar fora particular model of this modified theory. In the inner region of a gravastar,the considered equation of state defines that energy density is equal tonegative pressure which is the cause of repulsive force on the spherical shell.In the intermediate shell, pressure and energy density are equal and containultra-relativistic fluid. The inward-directed gravitational pull of thin-shellcounterbalance the force exerted by the inner region of a gravastar allowingthe formation of a singularity-free object. The Reissner-Nordstrom metricpresents the outer vacuum spherical domain. Moreover, we discuss the impact ofthe charge on physical attributes of a gravastar such as the equation of stateparameter, entropy, proper length and energy. We conclude that singularity-freesolutions of charged gravastar are physically consistent in this modifiedtheory.

Impact of Charge on Gravastars in $f(\mathfrak{R},\mathcal{T}^{2})$ Gravity