IndisputableMonolith.Physics.NoHairTheorem
The module defines the three conserved charges forced by the Recognition Science J-cost for asymptotically flat spacetimes and shows that these charges fix the black hole state. Physicists studying black hole uniqueness theorems cite the resulting charge triple and state equivalence. The module proceeds by introducing charge and state types, then cost and entropy functions that enforce non-negativity and uniqueness.
claimAn asymptotically flat spacetime carries three RS-forced conserved charges whose values completely determine the black hole state, with the associated cost functional nonnegative and zero precisely when two states share identical charges.
background
Recognition Science derives all physics from the single functional equation whose J-cost satisfies the composition law J(xy) + J(x/y) = 2J(x)J(y) + 2J(x) + 2J(y). This module imports the JcostCore definitions of that functional and applies them to black hole physics in asymptotically flat geometries. It therefore works inside the forcing chain that yields J-uniqueness, the self-similar fixed point phi, the eight-tick octave, and D = 3 spatial dimensions.
proof idea
This is a definition module, no proofs.
why it matters in Recognition Science
The module supplies the charge and state infrastructure that supports the black-hole entropy lemmas defined among its siblings, including bekenstein_hawking_entropy and entropy_linear_in_area. It thereby realizes the uniqueness implied by J-uniqueness (T5) for spacetime configurations and closes one concrete step of the unified forcing chain inside the Physics domain.
scope and limits
- Does not treat spacetimes with nonzero cosmological constant.
- Does not compute explicit numerical values for the three charges.
- Does not address higher-dimensional or non-asymptotically flat geometries.
- Does not incorporate quantum corrections or dynamical stability.
depends on (1)
declarations in this module (17)
-
structure
BHCharges -
def
BHState -
def
hair_cost -
theorem
hair_cost_nonneg -
theorem
hair_cost_zero_iff -
theorem
no_hair_field_decay -
theorem
bh_state_determined_by_charges -
theorem
bh_state_eq_of_charges_eq -
def
bekenstein_hawking_entropy -
theorem
entropy_nonneg -
theorem
entropy_linear_in_area -
def
schwarzschild_entropy -
theorem
schwarzschild_entropy_eq -
theorem
schwarzschild_entropy_monotone -
def
hawking_temperature -
theorem
hawking_temp_positive -
theorem
hawking_temp_decreases