IndisputableMonolith.Gravity.UltramassiveBH
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
- Does not derive the Einstein equations from the J-cost functional equation.
- Does not treat charged or rotating black holes.
- Does not compute the mass spectrum for ultramassive objects.
- Does not address information loss or unitarity issues.
- Does not provide numerical predictions for specific astrophysical black holes.
depends on (2)
declarations in this module (26)
-
structure
RSBH -
def
schwarzschildRadius -
def
horizonArea -
def
k_R -
lemma
k_R_pos -
def
horizonCells -
def
rs_entropy -
def
rs_hawkingTemp -
theorem
Jcost_finite_on_pos -
theorem
Jcost_zero_iff_one -
theorem
Jcost_lower_bound -
theorem
nothing_costs_arbitrarily_large -
theorem
rs_entropy_eq -
theorem
rs_entropy_pos -
theorem
entropy_quadruples_on_double -
theorem
rs_hawkingTemp_pos -
theorem
temp_decreases_with_mass -
theorem
temp_halves_on_double -
theorem
hamiltonian_approximation_bound -
theorem
small_strain_hamiltonian_valid -
def
phiRung -
theorem
phi_ladder_recovery -
theorem
cosmic_censorship_automatic -
theorem
bh_interior_finite_cost -
structure
UltramassiveBHCert -
def
ultramassiveBHCert