Abstract
A naive view of physics—classical or quantum—would have us believe that an infinite amount of information can be contained in a finite 3-D space. After all, matter can have an infinity of classical configurations there, and quantum fields have an infinity of modes in that region. ’ t Hooft and Susskind’s holographic principle [1, 2] has shattered this popular view: it holds that insofar as the information required to describe them is concerned, physical systems are inherently two-dimensional in space. In particular, the information or entropy (see Sec. 1.2 below for the relation) in an isolated system is expected to be bounded from above by one quarter the area of a circumscribing surface expressed in Planck units (holographic bound):
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Bekenstein, J.D. (2002). Quantum Information and Quantum Black Holes. In: Bergmann, P.G., de Sabbata, V. (eds) Advances in the Interplay Between Quantum and Gravity Physics. NATO Science Series, vol 60. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-0347-6_1
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