Computer Vision, Neural Radiance Fields, Astronomy, Synthetic Computer Vision, 3d Computer Graphics.
time-dependant angle are: Φ (t, r) = tω(r) where r is the distance of the object (emissions) from the Black Hole center, and t is the time. This model depends on Gravitationally-Lensed Ray Tracing to describe the integration of 3D emission along curved rays forming a 2D image. For N×N pixels, the