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This paper studies the effects of charge on a peculiar stellar object,recognized as gravastar, under the influence of $f(R,T)$ gravity by consideringthe conjecture of Mazur and Mottola in general relativity. The gravastar isalso known as an alternative to a black hole and is expressed by three distinctdomains named as (i) the interior domain, (ii) the intermediate shell and (iii)the exterior domain. We analyze these domains for a specific $f(R,T)$ gravitymodel conceding the conformal Killing vectors. In the interior domain, weassume that pressure is equal to negative energy density which leads to theexistence of repulsive force on the spherical shell. The intermediate shellconsists of ultra-relativistic plasma and pressure which shows a directrelation with energy density and counterbalances the repulsive force applied bythe interior domain. The exterior vacuum spherical domain is taken to be the deSitter spacetime illustrated by the Reissner-Nordstr\"{o}m metric. We concludethat non-singular solutions of charged gravastar with various physicalproperties such as length, energy, entropy and equation of state parameter arephysically consistent.

Charged Gravastars with Conformal Motion in f(R,T) Gravity