Interactive visualization of a thin disc around a Schwarzschild black hole
arXiv:1206.4259 · doi:10.1088/0143-0807/33/4/955
Abstract
In the first course of general relativity, the Schwarzschild spacetime is the most discussed analytic solution to Einstein's field equations. Unfortunately, there is rarely enough time to study the optical consequences of the bending of light for some advanced examples. In this paper, we present how the visual appearance of a thin disc around a Schwarzschild black hole can be determined interactively by means of an analytic solution to the geodesic equation processed on current high performance graphical processing units. This approach can, in principle, be customized for any other thin disc in a spacetime with geodesics given in closed form. The interactive visualization discussed here can be used either in a first course of general relativity for demonstration purposes only or as a thesis for an enthusiastic student in an advanced course with some basic knowledge of OpenGL and a programming language.
9 pages, 4 figures
Cited by in corpus (7)
- Image of the Janis-Newman-Winicour naked singularity with a thin accretion disk
- Gravitational Lensing by Spinning Black Holes in Astrophysics, and in the Movie Interstellar
- Thin Accretion Disk around a four-dimensional Einstein-Gauss-Bonnet Black Hole
- Observational signatures of strongly naked singularities: image of the thin accretion disk
- Review of scientific topics for Millimetron space observatory
- Images and Spectral Properties of Two Component Advective Flows Around Black Holes: Effects of Photon Bending
- Image of the thin accretion disk around compact objects in the Einstein-Gauss-Bonnet gravity