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module module high

IndisputableMonolith.Gravity.UltramassiveBH

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The module defines black hole quantities such as Schwarzschild radius and horizon area for an ultramassive black hole in RS-native units with ℓ₀ = τ₀ = c = 1. Gravity researchers cite these when computing entropy or temperature from the J-cost framework. The module consists entirely of definitions and elementary lemmas with no complex proofs.

claimIn RS-native units where the fundamental length ℓ₀, time τ₀ and speed of light c are all set to 1, a black hole is characterized by its Schwarzschild radius $r_s$, horizon area $A$, and related J-cost quantities.

background

Recognition Science derives all physics from the J functional equation and the Recognition Composition Law. The module imports the definition τ₀ = 1 tick from Constants and the core J-cost machinery from JcostCore. It introduces black-hole-specific objects (RSBH, schwarzschildRadius, horizonArea, horizonCells, rs_entropy, rs_hawkingTemp) expressed directly in these units.

proof idea

This is a definition module, no proofs.

why it matters in Recognition Science

The definitions supply the RS-native foundation for black-hole thermodynamics and feed the sibling lemmas rs_entropy and rs_hawkingTemp. They connect the J-cost lower-bound results to gravitational horizons within the Gravity domain.

scope and limits

depends on (2)

Lean names referenced from this declaration's body.

declarations in this module (26)