On some solutions of Maxwell’s equations in a Schwarzschild–de Sitter black hole
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Publication:3544396
DOI10.1063/1.2767536zbMath1152.81336OpenAlexW2094458904MaRDI QIDQ3544396
Carlos H. G. Béssa, Valdir B. Bezerra
Publication date: 8 December 2008
Published in: Journal of Mathematical Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1063/1.2767536
Cites Work
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- Particle creation by black holes
- Particle motion in the spherically symmetric vacuum solution with positive cosmological constant
- Effects of a positive cosmological constant on circular orbits in the Reissner-Nordstroem, Schwarzschild, and Kerr fields
- Is the semi-classical analysis valid for extreme black holes?
- The structure of the extreme Schwarzschild-de Sitter space-time
- Black holes in which the electrostatic or scalar equation is solvable in closed form
- Vacuum solutions of Einstein's equations in double-null coordinates
- Quasi-normal modes of Schwarzschild–de Sitter black holes
- Electrostatics in a Schwarzschild black hole pierced by a cosmic string
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