| Some photos |  | 
Black holes simulations
Kerr-Newman-de Sitter with and without an accretion disk (and parameters \(\Lambda=5\cdot 10^{-4},~a=0.99,~Q=0.14\)) :
 
  
 Several light wave frequency shifts (gravitational, Doppler, mixed and mixed with rotation of the camera) :
Cosmological effects on the shadow (\(a=0.95,~Q=0.3\)); observe the absence of horizon when \(\Lambda\ll 0\):
 
 Cosmological effects on the accretion disk (no rotation: \(a=0\)) :
 
 Simulations of M87* (with enlarged inner radius, from EHT's data, with added picture alteration, original photograph by the EHT) :
Some GIFs to observe the light distorsion, in Lorentzian signature (and same parameters as above), then Euclidean (with maximal charge and no rotation) :
 
  
 Oberwolfach (April 03-08, 2022)
Meeting photo
 
 Mathematisches Forschungsinstitut
 
  
 Walke
 
 Pines and rock in the Black Forest
 
  
  
 Urlaubsparadies Landeckhof (pendant la randonnée traditionnelle)
 
  
 Wallfahrtskirche St. Romanus
 
  
 In a chalk shell
 
 Defense (12/10/2021)
 
 
 
  
  
  
  
  
  
 