The Kerr spacetime : rotating black holes in general relativity
By D. Wiltshire, Matt Visser, S. Scott. 2009
229 citations recorded by the source corpus.
View Paper: https://www.semanticscholar.org/paper/1174bb5a7a1af22d7027d474b89ee281bd24fc68
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Citations in the corpus
- Black holes in general relativity (2009, unknown): “43 65 v3 [ gr -q c] 5 F eb 2 00 9”
- Asymptotically flat black holes with scalar hair: a review (2015, background): “Linearizing the field equations of (1) (or (2)) in F (or Φ) around the Schwarzschild metric, yields the source free Maxwell (or Klein-Gordon) eq.”
- Superradiance: Energy Extraction, Black-Hole Bombs and Implications for Astrophysics and Particle Physics (2015, methodology): “Because we also wish to consider effect of a cosmological constant, we will enlarge it to the Kerr-(A)dS family of spinning BHs, which in standard Boyer-Lindquist coordinates reads (for details on the Kerr spacetime, we refer the reader to the monograph [145])”
- Construction and physical properties of Kerr black holes with scalar hair (2015, background): “The paradigm is supported on both a set of mathematical theorems—the uniqueness theorems [17, 18]—but also on a conjecture—the no-hair conjecture [19].”
- Superradiance (2015, unknown): “cal constant, we will enlarge it to the Kerr-(A)dS family of spinning BHs, which in standard Boyer-Lindquist coordinates reads (for details on the Kerr spacetime, we refer the reader to the monograph [145]) ds2 = 2r ˆ2 dt a sin2 #d’ + ˆ2 r dr2 + ˆ2 # d#2 + # ˆ2 sin2 # adt r2 + a2 d’ 2 ;(4.5) wit”
- Black holes, gravitational waves and fundamental physics: a roadmap (2018, methodology): “As a corollary of the GR uniqueness theorem [1514, 1515], the entire QNM spectrum of a Kerr BH eventually depends only on its mass and spin.”