Talk detail

Participant	sadia, haleema
Institution	university of management and technology sialkot - city campus shahab pura road sialkot - sialkot - pakistan - Pakistan

Session	PS	Accepted		Order	Time
Talk	Oral abstract	Title	THE MATHEMATICAL MODELING OF RADIATING STARS AND THEIR ANALYTICAL ANALYSIS
Coauthors
Abstract	The thesis is devoted to analyze the effects of dark source polynomial curvature corrections in the mathematical modeling of radiating stars. In this scenario, we have used a particular $f(R,T)$ model and consider the spherically symmetric geometry of relativistic interior. We assumed that our geometry is coupled with anisotropic shearing matter distribution undergoing radiating epoch with free streaming and diffusion approximation. We have calculated spherically symmetric total matter content with the help of Misner-Sharp formalism. A particular relation among anisotropic pressure, shearing viscosity, radiating parameters, energy density and tidal forces is obtained. We then expressed this equation with the help of $f(R,T)$ structure scalar, the scalar obtained by orthogonal decomposition of the Riemann tensor. The role of the logarithmic Ricci and trace of stress energy tensor terms are also observed through Weyl scalar, shear, expansion scalar differential equations. We have also discussed some dynamical properties in the background of dust relativistic ball with present Ricci scalar corrections.
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