Two Black Hole Holography, Lensing and Intensity
arXiv:gr-qc/0103078 · doi:10.1103/PhysRevD.64.044020
Abstract
We numerically verify the analysis of the "expanding horizon" theory of Susskind in relation to the 't Hooft holographic conjecture. By using a numerical simulation to work out the image formed by two black holes upon a screen very far away, it is seen that it is impossible for a horizon to hide behind another. We also compute the intensity distribution of such an arrangement.
10 pages