Effect of a quintessence model on the energy of the Reissner-Nordstrom black hole
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Publication:2353811
DOI10.1007/S10714-015-1883-7zbMath1317.83069arXiv1408.3111OpenAlexW3101815824MaRDI QIDQ2353811
Publication date: 9 July 2015
Published in: General Relativity and Gravitation (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1408.3111
Black holes (83C57) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Approximation procedures, weak fields in general relativity and gravitational theory (83C25) Einstein-Maxwell equations (83C22)
Related Items (3)
2nd order approximate Noether and Lie symmetries of Gibbons-Maeda-Garfinkle-Horowitz-Strominger charged black hole in the Einstein frame ⋮ More insight into microscopic properties of RN-AdS black hole surrounded by quintessence via an alternative extended phase space ⋮ Black holes surrounded by modified Chaplygin gas in Lovelock theory of gravity
Cites Work
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- Energy of the Bardeen model using an approximate symmetry method
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- Energy in the spacetime field of the charged rotating BTZ black hole via approximate Lie symmetries
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
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