Author(s)

B. C. Tewari¹, Kali Charan², Jyoti Rani¹

¹Department of Mathematics, Kumaun University, SSJ Campus, Almora, India.
²Department of Mathematics, SRMS College of Engineering and Technology, Bareilly, India.

We here present a relativistic model for a spherically symmetric anisotropic fluid to study the various factors of physical and thermal phenomenon during the evolution of a collapsing star dissipating energy in the form of radial heat flow. We also proposed a table of some new parametric class of solutions which will be useful for constructing the new compact star models. The constructed algorithm obeys all the relevant requirements of a realistic model and matched with Vaidya exterior metric over the boundary. At the initial stage the interior solutions represent a static configuration of perfect fluid which then gradually starts evolving into radiating collapse. The apparent luminosity as observed by the distant observer at rest at infinity and the effective surface temperature are zero in remote past at the instant when collapse begins and at the stage when collapsing configuration reaches the horizon of the black hole.

Exact Solutions, Anisotropic Fluid, Spherical Gravitational Collapse, Black Hole

Tewari, B. , Charan, K. and Rani, J. (2016) Spherical Gravitational Collapse of Anisotropic Radiating Fluid Sphere. International Journal of Astronomy and Astrophysics, 6, 155-165. doi: 10.4236/ijaa.2016.62013.