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Herrera, L., Di Prisco, A., Ospino, J., Fuenmayor, E. and Triconis, O. (2009) Structure and Evolution of Self-Gravi-tating Objects and the Orthogonal Splitting of the Riemann Tensor. Physical Review D, 79, Article ID: 064025.
http://dx.doi.org/10.1103/PhysRevD.79.064025

has been cited by the following article:

• TITLE: Spherical Gravitational Collapse of Anisotropic Radiating Fluid Sphere

  AUTHORS: B. C. Tewari, Kali Charan, Jyoti Rani

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

  JOURNAL NAME: International Journal of Astronomy and Astrophysics, Vol.6 No.2, May 18, 2016

  ABSTRACT: 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.