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 holographic 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 holographic intensity distribution of such an arrangement.
DOI:https://doi.org/10.1103/PhysRevD.64.044020
©2001 American Physical Society