Bekenstein bound

According to the Bekenstein bound, the entropy of a black hole is proportional to the number of Planck areas that it would take to cover the black hole's event horizon.

In physics, the Bekenstein bound (named after Jacob Bekenstein) is an upper limit on the thermodynamic entropy S, or Shannon entropy H, that can be contained within a given finite region of space which has a finite amount of energy—or conversely, the maximum amount of information required to perfectly describe a given physical system down to the quantum level.[1] It implies that the information of a physical system, or the information necessary to perfectly describe that system, must be finite if the region of space and the energy are finite.

  1. ^ Bekenstein, Jacob D. (1981). "Universal upper bound on the entropy-to-energy ratio for bounded systems" (PDF). Physical Review D. 23 (2): 287–298. Bibcode:1981PhRvD..23..287B. doi:10.1103/PhysRevD.23.287. S2CID 120643289.

© MMXXIII Rich X Search. We shall prevail. All rights reserved. Rich X Search