Structure Scalars for Charged Dissipative Spherical Collapse in $f(R, T)$ Gravity
Uttaran Ghosh, Sarbari Guha

TL;DR
This paper explores how structure scalars derived from the Riemann tensor influence physical parameters in charged, dissipative spherical collapse within $f(R,T)$ gravity, highlighting effects of charge, dissipation, and modified gravity on collapse dynamics.
Contribution
It introduces the analysis of structure scalars in $f(R,T)$ gravity for charged dissipative collapse, revealing their impact on physical parameters and providing junction and energy condition conditions.
Findings
Structure scalar $X_{TF}$ influences energy density inhomogeneity.
Charge affects structure scalars and total mass-energy.
Physical parameters depend on structure scalars and complexity factors.
Abstract
We examine the structure scalars constructed from the orthogonal splitting of the Riemann tensor for the spacetime metric describing the interior of a charged matter configuration undergoing dissipative collapse in the framework of gravity (where and are the Ricci scalar and the trace of energy-momentum tensor, respectively), and also the way these quantities influence the various physical parameters of the collapsing matter. In absence of dissipation, the energy density inhomogeneity is found to be influenced by the structure scalar and the mass-function of the collapsing matter. Further, the presence of charge affects the structure scalars and the total mass-energy content. The dependence of the various physical parameters like heat dissipation, energy density inhomogeneity, evolution of the expansion scalar, the shear scalar, effective homogeneous energy…
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Taxonomy
TopicsCosmology and Gravitation Theories · Pulsars and Gravitational Waves Research · Black Holes and Theoretical Physics
