Photon Regions and Shadows of Kerr-Newman-NUT Black Holes with a Cosmological Constant
- Phys.Rev.D 89 (2014) 12, 124004
- Published: Jun 6, 2014
- 1403.5234 [gr-qc]
Citations per year
We consider the Plebański class of electrovacuum solutions to the Einstein equations with a cosmological constant. These space-times, which are also known as the Kerr-Newman-NUT–(anti–)de Sitter space-times, are characterized by a mass
- 11 pages, 10 figures
- 04.70.-s
- 95.30.Sf
- 98.35.Jk
- space-time: de Sitter
- black hole: de Sitter
- anti-de Sitter
- charge: magnetic
- charge: electric
- cosmological constant
- photon
- [1]
- [2]
- [3]
- [4]
- [5]
- [6]
- [7]
- [8]
- [9]
- [10]
- [11]
- [12]
- [13]
- [14]
- [15]
- [16]
- [17]
- [18]
- [19]
- [20]
- [21]
- [22]
- [23]
- [24]
- [25]