Implications of f (R, T) gravity on the complexity factor of a physically consistent charged anisotropic stellar model
The present manuscript throws light on the existence of an electrically charged compact
stellar model and explores the behavior of complexity factor, proposed by Herrera (2018),
against the selected model in the background of f (R, T) gravity (R is the Ricci scalar, while T
is the trace of energy–momentum tensor). The set of f (R, T) field equations has been solved
by choosing Adler Finch–Skea solution, where the presence of electromagnetic radiations
have also been considered in the stellar interior. For the space–time continuity, the …
stellar model and explores the behavior of complexity factor, proposed by Herrera (2018),
against the selected model in the background of f (R, T) gravity (R is the Ricci scalar, while T
is the trace of energy–momentum tensor). The set of f (R, T) field equations has been solved
by choosing Adler Finch–Skea solution, where the presence of electromagnetic radiations
have also been considered in the stellar interior. For the space–time continuity, the …
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