arXiv · 1705.06988
Behaviour of Charged Collapsing Fluids after Hydrostatic Equilibrium in R^n Gravity
Abstract
The purpose of this paper is to study the transport equation and its coupling with Maxwell equation in the framework of R^n gravity. Using Muller-Israel-Stewart theory for the conduction of dissipative fluids, we analyze the temperature, heat flux, viscosity and thermal conductivity in the scenario of relaxation time. All these thermodynamical variables are appeared in the form of a single factor whose influence is discussed on the evolution of relativistic model for the heat conducting collapsing star.
Explore related subjects
Keep this discovery
Hafiza Rizwana Kausar. 2017-05-18. Behaviour of Charged Collapsing Fluids after Hydrostatic Equilibrium in R^n Gravity. https://arxiv.org/abs/1705.06988
Cite the original work for its findings. Save a collection to share your selection of sources.