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Bekenstein bound
In Binary Pulse Theory: BPT Modified Bekenstein Bound
Same thing, new nameIn standard physics
The maximum entropy, and so information, a region can hold, set by the area of its boundary in Planck units.
In Binary Pulse Theory
The same limit counted in bits: one bit for every 4·ln 2 Planck areas of the horizon.
The BPT terms behind it
The BPT Modified Bekenstein Bound is the book's entropy limit for a Null Well, counted in bits: S∅ ≤ A▣/(4 l_P² · ln 2) · ℨᵇ, the effective encoding area in Planck-area units divided by the natural logarithm of 2, which converts nats to bits.
The Standard Bekenstein Bound is the classical limit on the entropy, and so the information, a gravitational system can hold: the entropy of a Null Well is at most its event horizon area divided by four Planck areas, S ≤ A/(4l_P²).
The Bekenstein-Hawking Entropy Bounds are the limits on how much entropy a Null Well, or in BPT a null well, can hold in terms of its boundary area; the book keeps the standard bound and adds a modified one that includes a binary information factor.
Also known as
Bekenstein-Hawking entropy · black hole entropy · entropy bound
Related
The standard physics term is here to help you find your way in; the book itself writes in BPT's own terms. Read them in the lexicon, or start the book at Binary Pulse Theory.