# Tolman-Oppenheimer-Volkoff equations in the presence of the Chaplygin gas: Stars and wormholelike solutions

@article{Gorini2008TolmanOppenheimerVolkoffEI, title={Tolman-Oppenheimer-Volkoff equations in the presence of the Chaplygin gas: Stars and wormholelike solutions}, author={Vittorio Gorini and Alexander Yu Kamenshchik and Ugo Moschella and Vincent Pasquier and Alexei A. Starobinsky}, journal={Physical Review D}, year={2008}, volume={78}, pages={064064} }

We study static solutions of the Tolman-Oppenheimer-Volkoff equations for spherically symmetric objects (stars) living in a space filled with the Chaplygin gas. Two cases are considered. In the normal case, all solutions (excluding the de Sitter one) realize a three-dimensional spheroidal geometry because the radial coordinate achieves a maximal value (the 'equator'). After crossing the equator, three scenarios are possible: a closed spheroid having a Schwarzschild-type singularity with… Expand

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