Abstract
This paper deals with the exploration of collapse rate and Tolman mass function for spherical system under the influence of [Formula: see text] modified gravity theory after using Herrera technique. We have taken the matter configuration to be anisotropic as well as dissipative due to diffusion and streaming out radiations. The modified field equations and dynamical equations are explored for a systematic investigation of Tolman mass. An explicit link among the matter profile, Weyl tensor and mass function is exhibited in this scenario. We found that the anisotropic pressure and density inhomogeneity tends to increase the Tolman mass within the sphere radius, while [Formula: see text] terms stabilize the system.
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