pith. sign in
module module high

IndisputableMonolith.Quantum.BlackHoleInformation

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Black hole models in Recognition Science are built from a mass parameter, yielding the Schwarzschild radius, Bekenstein-Hawking entropy proportional to mass squared, Hawking temperature, and checks on holographic saturation. Quantum gravity researchers would cite these for information accounting in collapse. The module sequences definitions from the imported RS time quantum without proofs.

claimBlack hole characterized by mass $M$, with Schwarzschild radius $r_s(M)$, horizon area $A(M)$, Bekenstein-Hawking entropy $S_{BH}(M) = A/4$, Hawking temperature $T(M)$, information capacity, and holographic bound, all in RS units where $c=1$, $G = phi^5 / pi$, $hbar = phi^{-5}$.

background

The module sits in the quantum domain and imports the fundamental RS time quantum from Constants, described as: The fundamental RS time quantum (RS-native). τ₀ = 1 tick. It defines a black hole by its mass then derives radius, area, entropy, temperature, capacity, and bound, plus structures for falling entries and a ledger to track information.

proof idea

This is a definition module, no proofs.

why it matters in Recognition Science

Supplies black hole entropy and information capacity constructions that integrate with the phi-ladder mass formula and J-uniqueness from the forcing chain. It supports holographic bound analysis in the D=3 spatial setting and connects to the eight-tick octave periodicity.

scope and limits

depends on (1)

Lean names referenced from this declaration's body.

declarations in this module (25)