Kerr Black Holes in Horizon-Generating Form
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Publication:2837611
DOI10.1103/PhysRevLett.92.191101zbMath1267.83059arXivgr-qc/0401111WikidataQ49257710 ScholiaQ49257710MaRDI QIDQ2837611
Publication date: 11 July 2013
Published in: Physical Review Letters (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/gr-qc/0401111
Related Items (3)
Rotating black holes embedded in a cosmological background for scalar-tensor theories ⋮ New formulation of the first law of black hole thermodynamics: a stringy analogy ⋮ Thermodynamics of dynamical wormholes
Cites Work
- The four laws of black hole mechanics
- Dynamical Horizons: Energy, Angular Momentum, Fluxes, and Balance Laws
- Stability of a Schwarzschild Singularity
- Completion and Embedding of the Schwarzschild Solution
- Maximal Extension of Schwarzschild Metric
- Gravitational Field of a Spinning Mass as an Example of Algebraically Special Metrics
- Dual-null dynamics of the Einstein field
- Gravitational-wave dynamics and black-hole dynamics: second quasi-spherical approximation
- The Kerr spacetime in generalized Bondi–Sachs coordinates
- Inequalities Relating Area, Energy, Surface Gravity, and Charge of Black Holes
- Quasi-local first law of black-hole dynamics
- Unified first law of black-hole dynamics and relativistic thermodynamics
- Gravitational waves, black holes and cosmic strings in cylindrical symmetry
- Maximal Analytic Extension of the Kerr Metric
- Global Structure of the Kerr Family of Gravitational Fields
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