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module module high

IndisputableMonolith.Gravity.UltramassiveBH

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The module defines black hole structures in RS-native units with base length and time quanta set to unity and c equal to 1. It supplies RSBH together with the Schwarzschild radius, horizon area, cell count, entropy, and Hawking temperature built from the J-cost function. Gravity researchers working inside the Recognition Science derivation would cite these for black hole thermodynamics. The content consists of definitions and elementary lemmas on positivity and bounds.

claimThe RS black hole RSBH with mass parameter $M$ has Schwarzschild radius $r_s = 2M$, horizon area $A = 4π r_s^2$, entropy $S = A/4$, and Hawking temperature $T_H = 1/(8π M)$ in units where $ℓ_0 = τ_0 = c = 1$.

background

Recognition Science derives all physical laws from a single functional equation whose solution yields the J-cost $J(x) = (x + x^{-1})/2 - 1$. The Constants module fixes the RS time quantum at $τ_0 = 1$ tick. JcostCore supplies the core J-cost definitions and the Recognition Composition Law $J(xy) + J(x/y) = 2J(x)J(y) + 2J(x) + 2J(y)$. This module applies those tools to ultramassive black holes, introducing RSBH as the native black hole object and deriving its geometric and thermodynamic quantities from the J-cost lower bound.

proof idea

This is a definition module, no proofs.

why it matters in Recognition Science

The module supplies the black hole definitions required by the gravity sector of the Recognition framework. It connects the J-cost lower bound to horizon entropy and temperature, supporting the derivation of classical gravity from the forcing chain steps T5 through T8 that fix $D = 3$ spatial dimensions and the eight-tick octave. No downstream theorems are listed yet, indicating this is foundational scaffolding for black hole thermodynamics in RS units.

scope and limits

depends on (2)

Lean names referenced from this declaration's body.

declarations in this module (26)