The apparent shape of a rotating charged black hole, closed photon orbits and the bifurcation set A 4
By A. Vries. 2000
203 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/8d6585f47da1baba93903397ea9dd8843f0a301d
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In Astronomy and Astrophysics
- O. Tsupko
- Rahul Kumar
- Sushant G. Ghosh
- V. Perlick
- Misba Afrin
- G. Bisnovatyi-Kogan
- M. Werner
- A. Rogers
In Nuclear and High Energy Physics
Citations in the corpus
- Parameter estimation of hairy Kerr black holes from its shadow and constraints from M87* (2021, background): “…aroused a flurry of activities in the analytical investigations, and numerical simulation of shadows for black holes in GR (Falcke et al. 2000; de Vries 2000; Shen et al. 2005; Yumoto et al. 2012; Atamurotov et al. 2013; Papnoi et al. 2014; Abdujabbarov et al. 2015; Atamurotov et al. 2016; Cunha…”
- Calculating black hole shadows: Review of analytical studies (2021, background): “The shadow is then completely different from a black-hole shadow; in particular, it is no longer a (two-dimensional) black disk on the observer’s sky but rather a (one-dimensional) black arc, see de Vries [108].”
- Black Hole Parameter Estimation from Its Shadow (2018, methodology): “…a shadow of a black hole in front of a planaremitting source was applied to several black hole models, e.g., Kerr–Newman black hole (Young 1976; De Vries 2000), ChernSimons modified gravity black hole (Amarilla et al. 2010), Kaluza–Klein rotating dilaton black hole (Amarilla & Eiroa 2013),…”