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module module moderate

IndisputableMonolith.Gravity.UltramassiveBH

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The module defines a black hole in Recognition Science using native units where fundamental length, time, and light speed equal one. It supplies the RS black hole object along with horizon radius, area, entropy, and temperature expressions built on the J-cost. Gravity researchers modeling discrete spacetime or thermodynamic limits would reference these. The module contains only definitions imported from the constants and J-cost core.

claimIn units with $\ell_0 = \tau_0 = c = 1$, defines the RS black hole together with Schwarzschild radius $r_s$, horizon area $A$, cell count, entropy $S$, and Hawking temperature $T$ via the J-cost function.

background

The module sits inside the Gravity domain of Recognition Science and imports the time quantum $\tau_0 = 1$ tick from Constants together with the J-cost core. It works entirely in RS-native units where length, time, and $c$ are set to unity, allowing direct application of the J-cost to horizon quantities. The setting extends the Recognition Composition Law to black-hole thermodynamics without invoking the full forcing chain.

proof idea

This is a definition module, no proofs.

why it matters in Recognition Science

The module supplies the black-hole primitives required by any downstream gravity theorems that link J-cost to horizon entropy or temperature. It fills the concrete object needed to apply the phi-ladder and eight-tick octave to ultramassive objects, though no used-by edges are recorded yet.

scope and limits

depends on (2)

Lean names referenced from this declaration's body.

declarations in this module (26)