Collapse and Expansion of Anisotropic Plane Symmetric Source

Abstract

This paper deals with the collapse and expansion of relativistic anisotropic self-gravitating source. The field equations for non-radiating and non-static plane symmetric anisotropic source have been evaluated. The non-radiating property of the fluid leads to evaluation of the metric functions. We have classified the dynamical behavior of gravitational source as expansion and collapse. The collapse in this case leads to the final stage without the formation of apparent horizons while such horizons exists in case of spherical anisotropic source. The matching of interior and exterior regions provides the continuity of masses over the boundary surface.

12 Pages, 4 figures. Accepted for Publication in Astrophys. Space Sci

References in corpus (5)

• All static spherically symmetric anisotropic solutions of Einstein's equations
• String-inspired Gauss-Bonnet gravity reconstructed from the universe expansion history and yielding the transition from matter dominance to dark energy
• Fate of gravitational collapse in semiclassical gravity
• Expansion-free Cylindrically Symmetric Models
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