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Wednesday December 03, 2008
Start: 2008-12-03 16:00
End: 2008-12-03 18:00

It has been theoretically accepted for a few decades that the entropy of a black hole is equal to a quarter of its surface area (in suitable units). And since around that time ideas have been developed about an entropy limit, similarly depending on the surface area, for any physical system. This research has developed into precise statements about a 'holographic principle,' which can crudely be summarized as follows.

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