KN parameter tangents solve the linearised equations on the exterior
ProvedExactVacuumAtlas.Variation.KN.param_tangent_exterioreinstein-maxwellexact-spacetime-atlas-ivexact-vacuum-atlasgeneral-relativity
KN parameter tangents solve the linearised equations on the exterior
For all real M, a, Q, m, α, q with M > 0 and x ∈ domKN M a Q: with h = paramTangent (ε ↦ gKN (M + εm) (a + εα) (Q + εq)) and f = paramTangent (ε ↦ faradayKN (a + εα) (Q + εq)) (componentwise ε-derivative at 0), the linearised residuals LE, LJ, LH of the KN background vanish at x.
Scope. The tangent is represented by the genuine paramTangent of the family; no separate explicit closed form of all tangent components is claimed. No derivative of rPlus is taken and nothing is divided by a or Q.
中文摘要 KN 三参数切向(用真实 paramTangent 表示)在外域满足线性化方程。
Preamble
import Mathlib import Definitions.Def_Atlas_Core_Basic import Definitions.Def_Atlas_Core_Certificate import Definitions.Def_Atlas_Core_Lift import Definitions.Def_Atlas_EinsteinMaxwell_Basic import Definitions.Def_Atlas_EinsteinMaxwell_Certificate import Definitions.Def_Atlas_EinsteinMaxwell_KN_Defs import Definitions.Def_Atlas_EinsteinMaxwell_KN_Domain import Definitions.Def_Atlas_EinsteinMaxwell_Variation_Defs import Definitions.Def_Atlas_EinsteinMaxwell_Variation_KN import Definitions.Def_Atlas_Kerr_Frame import Definitions.Def_Atlas_Kerr_InAtoms import Definitions.Def_Atlas_Transport_MatrixCalc import Definitions.Def_KerrBL_CoordGeometry import Definitions.Def_KerrBL_Kerr_Metric open Real open scoped ContDiff open ExactVacuumAtlas.EinsteinMaxwell ExactVacuumAtlas.EinsteinMaxwell.KN
Formal statement
theorem ExactVacuumAtlas.Variation.KN.param_tangent_exterior (M a Q m α q : ℝ) (hM : 0 < M) {x : Pt 4} (hx : x ∈ domKN M a Q) :
(∀ i j, linEinstein (gKN M a Q) (giKN M a Q) (faradayKN a Q)
(paramTangent fun ε => gKN (M + ε * m) (a + ε * α) (Q + ε * q))
(paramTangent fun ε => faradayKN (a + ε * α) (Q + ε * q)) i j x = 0) ∧
(∀ j, linMaxwell (gKN M a Q) (giKN M a Q) (faradayKN a Q)
(paramTangent fun ε => gKN (M + ε * m) (a + ε * α) (Q + ε * q))
(paramTangent fun ε => faradayKN (a + ε * α) (Q + ε * q)) j x = 0) ∧
(∀ i j k, linFaraday (paramTangent fun ε => faradayKN (a + ε * α) (Q + ε * q)) i j k x = 0) := by sorrySource
He Wang, Exact Spacetime Atlas IV: Certified Einstein–Maxwell Backgrounds and First Variations. Local source, no public repository; commit 543904bfcfa3bb169f43fc4d9dbd569999b71886; Atlas/EinsteinMaxwell/Variation/KN.lean#L86-L95; SHA-256 dba90888f19cb0f545a02c26c83f1e3649e4fb4f71e4bbf5f3c1b37ebc3fa51f. Registered definitions and literature: mission/PHYSICS_BOUNDARY.md (§H–§J); Müller–Grave arXiv:0904.4184; Newman et al., J. Math. Phys. 6 (1965) 918.
Human review
Confirmed by the mission captain (proposal self-audit).
Confirmed by the moderator at approval.