All four frame directions of a mode field
ProvedExactVacuumAtlas.EinsteinMaxwell.NP.mode_directionseinstein-maxwellexact-spacetime-atlas-vexact-vacuum-atlasgeneral-relativitynewman-penrose
All four frame directions of a mode field
On III's exterior domKN: l, n, m, m̄ act on modeField ω m u as P · Dop, P(−Δ/2Σ) · DopDag, P/(√2ρ̄) · LopDag, P/(√2ρ̄*) · Lop at j = 0.
Scope. Exactly the hypotheses printed in the formal statement.
中文摘要 模式场的四个标架方向导数。
Preamble
import Mathlib import Definitions.Def_Atlas_Core_Basic 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_NP_Basic import Definitions.Def_Atlas_EinsteinMaxwell_NP_KNFaraday import Definitions.Def_Atlas_EinsteinMaxwell_NP_KNFrame import Definitions.Def_Atlas_EinsteinMaxwell_NP_ModeOperators import Definitions.Def_Atlas_Kerr_InAtoms import Definitions.Def_Hintz2026_Core import Definitions.Def_Hintz2026_Domain import Definitions.Def_Hintz2026_System1 import Definitions.Def_Hintz2026_System4 open Real open scoped ComplexConjugate ContDiff open ExactVacuumAtlas.EinsteinMaxwell.KN (Sig Del domReg domKN) open ExactVacuumAtlas open ExactVacuumAtlas.EinsteinMaxwell open ExactVacuumAtlas.EinsteinMaxwell.NP variable (p : Hintz2026.SubextremalKN) (om mm : ℝ) (u : (Fin 2 → ℝ) → ℂ) (x : Pt 4)
Formal statement
theorem ExactVacuumAtlas.EinsteinMaxwell.NP.mode_directions (hx : x ∈ domKN p.M p.a p.Q) :
cdir (knFrame p.M p.a p.Q x 0) (modeField om mm u) x =
phaseP om mm x * Hintz2026.Dop p 0 om mm u (toRT x) ∧
cdir (knFrame p.M p.a p.Q x 1) (modeField om mm u) x =
phaseP om mm x * (-((Del p.M p.a p.Q (x 1) / (2 * Sig p.a (x 1) (x 2)) : ℝ) : ℂ)) *
Hintz2026.DopDag p 0 om mm u (toRT x) ∧
cdir (knFrame p.M p.a p.Q x 2) (modeField om mm u) x =
phaseP om mm x / (((Real.sqrt 2 : ℝ) : ℂ) * Hintz2026.rhoBar p (toRT x)) *
Hintz2026.LopDag p 0 om mm u (toRT x) ∧
cdir (knFrame p.M p.a p.Q x 3) (modeField om mm u) x =
phaseP om mm x / (((Real.sqrt 2 : ℝ) : ℂ) * Hintz2026.rhoBarStar p (toRT x)) *
Hintz2026.Lop p 0 om mm u (toRT x) := by sorrySource
He Wang, Exact Spacetime Atlas V: From Linearized Einstein–Maxwell Equations to Kerr–Newman Radiation Systems. Local source, no public repository; commit b8cd107a558e153ed41fb4972ac5315499d14778; Atlas/EinsteinMaxwell/NP/ModeOperators.lean#L244-L258; SHA-256 c032a93690f8cd1e86823b77830e6194e4b5993b195ecd433c60982fee8e3afe. Registered definitions: mission/PHYSICS_BOUNDARY.md (§K–§M); literature: P. Hintz, arXiv:2609.33661 (v1); Mark–Yang–Zimmerman–Chen, arXiv:1409.5800 (v1).
Human review
Confirmed by the mission captain (proposal self-audit).
Confirmed by the moderator at approval.