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arXiv · 1006.1624

Gravitational Collapse of Phantom Fluid in (2+1)-Dimensions

M. R. Martins·M. F. A. da Silva·Andrew D. Sheng
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Abstract

This investigation is devoted to the solutions of Einstein's field equations for a circularly symmetric anisotropic fluid, with kinematic self-similarity of the first kind, in $(2+1)$-dimensional spacetimes. In the case where the radial pressure vanishes, we show that there exists a solution of the equations that represents the gravitational collapse of an anisotropic fluid, and this collapse will eventually form a black hole, even when it is constituted by the phantom energy.

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BibTeXRIS

M. R. Martins, M. F. A. da Silva, Andrew D. Sheng. 2010-06-08. Gravitational Collapse of Phantom Fluid in (2+1)-Dimensions. https://doi.org/10.1007/s10714-009-0838-2

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