Space-time diagrammatics
arXiv:1211.1718 · doi:10.1103/PhysRevD.86.124041
Abstract
We introduce a new class of two-dimensional diagrams, the \emph{projection diagrams}, as a tool to visualize the global structure of space-times. We construct the diagrams for several metrics of interest, including the Kerr-Newman - (anti) de Sitter family, with or without cosmological constant, and the Emparan-Reall black rings.
41 pages, minor changes and corrections
References in corpus (8)
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- Black ring with two angular momenta
- Supersymmetric Rotating Black Holes and Causality Violation
- Kerr-de Sitter Universe
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- Shadows of Kerr-Vaidya-like black holes
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- Anisotropic Schrödinger black holes with hyperscaling-violation
- On causality violation on a Kerr-de Sitter spacetime
- Kerr-AdS type higher dimensional black holes with non-spherical cross-sections of horizons
- On the role of closed timelike curves and confinement structure around Kerr-Newman singularity
- Two discs and a missing triangle: the maximally extended Kerr black hole revisited