The Kiselev black hole's stress-energy is anisotropic, so it is neither a perfect fluid nor standard quintessence, despite a large literature saying otherwise.
Some generalizations of the Raychaudhuri equation
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abstract
The Raychaudhuri equation has seen extensive use in general relativity, most notably in the development of various singularity theorems. In this rather technical article we shall generalize the Raychaudhuri equation in several ways. First an improved version of the standard timelike Raychaudhuri equation is developed, where several key terms are lumped together as a divergence. This already has a number of interesting applications, both within the ADM formalism and elsewhere. Second, a spacelike version of the Raychaudhuri equation is briefly discussed. Third, a version of the Raychaudhuri equation is developed that does not depend on the use of normalized congruences. This leads to useful formulae for the "diagonal" part of the Ricci tensor. Fourth, a "two vector" version of the Raychaudhuri equation is developed that uses two congruences to effectively extract "off diagonal" information concerning the Ricci tensor.
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2019 1verdicts
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The Kiselev black hole is neither perfect fluid, nor is it quintessence
The Kiselev black hole's stress-energy is anisotropic, so it is neither a perfect fluid nor standard quintessence, despite a large literature saying otherwise.