Effects of electromagnetic field on gravitational collapse in f(R, T) gravity

In this paper, we examine spherically symmetric collapse with perfect fluid matter under the effect of electromagnetic field in f(R, T) gravity. We used the Darmois as well as Senovilla matching conditions by considering static exterior and non-static interior spherically symmetric spacetimes. The analytical solutions of field equations are obtained. We investigate the apparent horizon and their physical importance. It is pointed out that electromagnetic field diminishes the bound of f(R, T) term by diminishing the pressure and hence the whole collapsing process accelerates. The time interval between the cosmological horizon and singularities are also effected by electromagnetic field.