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IndisputableMonolith.Physics.NoHairTheorem

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The module defines the no-hair theorem in Recognition Science by introducing the three RS-forced conserved charges for asymptotically flat spacetimes and the associated black hole states. Physicists deriving classical GR results from the RS functional equation would cite it. The module structures its content as definitions and lemmas built directly on J-cost non-negativity from the imported JcostCore.

claimThe three RS-forced conserved charges of an asymptotically flat spacetime are denoted $BHCharges$, with black hole state $BHState$ satisfying $bh_state_determined_by_charges$ when uniquely fixed by these charges; $hair_cost onneg 0$ with equality precisely when no additional hair is present.

background

The module sits inside the Recognition Science framework for physics and imports JcostCore to access the J-cost function used for measuring deviations. The supplied module doc-comment identifies the central object as the three RS-forced conserved charges. Sibling declarations introduce $BHCharges$, $BHState$, the cost function $hair_cost$, and supporting statements on non-negativity and state uniqueness.

proof idea

this is a definition module, no proofs

why it matters in Recognition Science

The module establishes the no-hair theorem and thereby feeds the entropy results listed among its siblings, including bekenstein_hawking_entropy and entropy_linear_in_area. It supplies the black-hole uniqueness step required by the broader Recognition Science derivation that begins from the functional equation and the forcing chain.

depends on (1)

Lean names referenced from this declaration's body.

declarations in this module (17)