pith. sign in
module module high

IndisputableMonolith.Gravity.UltramassiveBH

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The UltramassiveBH module supplies type definitions and basic properties for black holes expressed in Recognition Science native units with ℓ₀ = τ₀ = c = 1. Gravity modelers working inside the RS framework would cite these objects when computing horizon quantities from J-cost. The module is purely definitional with no proof obligations or tactic steps.

claimAn RS black hole RSBH(M) of mass parameter M together with the associated Schwarzschild radius $r_s = 2M$, horizon area, cell count, and entropy expressed via the J-cost function in units where $c=1$, $τ_0=1$.

background

The module imports Constants, which fixes the RS time quantum τ₀ = 1 tick, and JcostCore, which supplies the J-cost function obeying the Recognition Composition Law J(xy) + J(x/y) = 2J(x)J(y) + 2J(x) + 2J(y). These imports set the native-unit convention ℓ₀ = τ₀ = c = 1 used throughout the black-hole definitions. Sibling declarations inside the module introduce RSBH, schwarzschildRadius, horizonArea, k_R, horizonCells, rs_entropy, and rs_hawkingTemp, all built directly on the J-cost primitives.

proof idea

this is a definition module, no proofs

why it matters in Recognition Science

The module supplies the black-hole primitives required for any RS-native treatment of gravity and entropy. It sits downstream of the J-cost core and the forcing chain (T5–T8) that fixes the phi-ladder and D = 3. No downstream theorems are recorded yet, so the definitions remain available for future gravity or cosmology results.

scope and limits

depends on (2)

Lean names referenced from this declaration's body.

declarations in this module (26)