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IndisputableMonolith.Quantum.BekensteinHawking

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The module Quantum.BekensteinHawking supplies definitions for the Boltzmann constant, Planck units, BlackHole structures, horizon area, and Bekenstein-Hawking entropy expressed via ledger capacity in Recognition Science units. Quantum gravity researchers would cite these to link RS cost functions to thermodynamic area laws. The module consists entirely of definitions with no theorems or proofs.

claim$k_B = 1.380649 \times 10^{-23} \, \mathrm{J/K}$, $\ell_p$ the Planck length, $A$ the horizon area, and $S_{BH} = k_B A / (4 \ell_p^2)$ together with its bit-count form from ledger capacity.

background

The module sits in the quantum domain and imports the RS time quantum $\tau_0 = 1$ tick from Constants plus cost primitives from Cost. It defines Planck length, area, mass, and temperature from RS-native units ($c=1$, $\hbar = \phi^{-5}$), then introduces the BlackHole type with schwarzschildRadius and horizonArea. Entropy definitions follow, including proportionality to area and conversion to bits via ledger capacity.

The setting uses the Recognition Composition Law to express information capacity at the horizon. No upstream theorems beyond the imported modules are invoked.

proof idea

this is a definition module, no proofs

why it matters in Recognition Science

The module supplies the entropy and area primitives that support later Recognition Science results on quantum information bounds and black hole thermodynamics. It fills the interface between Cost ledger accounting and horizon geometry, consistent with the eight-tick octave and $D=3$ spatial dimensions. No downstream theorems are recorded in the current graph.

scope and limits

depends on (2)

Lean names referenced from this declaration's body.

declarations in this module (28)