Kiselev, V. V. Quintessence and black holes. (English) Zbl 1026.83036 Classical Quantum Gravity 20, No. 6, 1187-1197 (2003). Summary: We present new static spherically symmetric exact solutions of the Einstein equations for quintessential matter surrounding a black hole, charged or uncharged, as well as for the case without a black hole. A condition of additivity and linearity in the energy-momentum tensor is introduced which allows one to obtain correct limits to known solutions for the electromagnetic static field, implying the relativistic relation between the energy density and pressure, as well as for the extraordinary case of the cosmological constant, i.e. de Sitter space. We classify the horizons, which evidently reveal themselves in static coordinates, and derive the Gibbons-Hawking temperatures. An example of quintessence with state parameter \(w=-2/3\) is discussed in detail. Cited in 1 ReviewCited in 143 Documents MSC: 83C57 Black holes 83F05 Relativistic cosmology Keywords:accelerating expansion of the universe; negative pressure; horizon; asymptotically flat space PDFBibTeX XMLCite \textit{V. V. Kiselev}, Classical Quantum Gravity 20, No. 6, 1187--1197 (2003; Zbl 1026.83036) Full Text: DOI arXiv