Speaker
Description
The stability of the inner structure of an irrotational charged black hole is a significant issue in relativity, serving as a prototype for the much more complicated problem of internal stability of a rotating charged black hole. Linear results suggest that the inner structure of a charged black hole is unstable under gravitational and electromagnetic perturbations. However, non-linear work on the problem has yet to reach a definitive conclusion on the stability. I aim to use a numerical approach based on Friedrich’s general conformal field equations to investigate the stability in the full non-linear picture. I will discuss previous works as well as the current status of the problem. Further, I will outline the numerical approach I am taking and the results obtained so far.
| Research Area | Mathematical and Numerical Relativity |
|---|