Two black hole holography, lensing, and intensity

Mark G. Jackson
Phys. Rev. D 64, 044020 – Published 27 July 2001
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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

    Authors & Affiliations

    Mark G. Jackson*

    • Department of Physics, Columbia University, New York City, New York 10027

    • *Email address: markj@phys.columbia.edu

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    Issue

    Vol. 64, Iss. 4 — 15 August 2001

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