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The weighted radial Jacobian row retains the actual wall amplitudes

Proved
BianchiIX.coreWeightedJacobian_amplitude_bounds

by trppppp · Nov 5, 2026 · Mathlib 0df444a (Lean v4.33.1)

bianchi-ix-era-statisticsdynamical-systems

For real variables p,s,a,b,cp,s,a,b,cp,s,a,b,c, set

K=a2+b2+c2−2(ab+bc+ca),S=p2+s2,C=S+K.K=a^2+b^2+c^2-2(ab+bc+ca),\qquad S=p^2+s^2,\qquad C=S+K.K=a2+b2+c2−2(ab+bc+ca),S=p2+s2,C=S+K.

The shear components and wall rates are

P=Kp−2a2+b2+c2+ab−2bc+ac,P=Kp-2a^2+b^2+c^2+ab-2bc+ac,P=Kp−2a2+b2+c2+ab−2bc+ac, Q=Ks+3(−b2+c2+ab−ac),Q=Ks+\sqrt{3}(-b^2+c^2+ab-ac),Q=Ks+3​(−b2+c2+ab−ac), r1=−S+2p,r2=−S−p+3s,r3=−S−p−3s.r_1=-S+2p,\qquad r_2=-S-p+\sqrt{3}s,\qquad r_3=-S-p-\sqrt{3}s.r1​=−S+2p,r2​=−S−p+3​s,r3​=−S−p−3​s.

These functions define the normalized vacuum Bianchi IX vector field (P,Q,r1a,r2b,r3c)(P,Q,r_1a,r_2b,r_3c)(P,Q,r1​a,r2​b,r3​c). For y=(m,u,v,w)∈R4y=(m,u,v,w)\in\mathbb R^4y=(m,u,v,w)∈R4, define

K(u,v,w)=u2+v2+w2−2(uv+vw+wu),κ=u(v+w−u),K(u,v,w)=u^2+v^2+w^2-2(uv+vw+wu),\qquad \kappa=u(v+w-u),K(u,v,w)=u2+v2+w2−2(uv+vw+wu),κ=u(v+w−u), Fm=−v2+w2+u(v−w)−mκ,Fu=12(1−m2−(v−w)2+u2)u,F_m=-v^2+w^2+u(v-w)-m\kappa,\qquad F_u=\tfrac12(1-m^2-(v-w)^2+u^2)u,Fm​=−v2+w2+u(v−w)−mκ,Fu​=21​(1−m2−(v−w)2+u2)u, Fv=(m−1−κ)v,Fw=(−m−1−κ)w,F=(Fm,Fu,Fv,Fw),F_v=(m-1-\kappa)v,\qquad F_w=(-m-1-\kappa)w,\qquad F=(F_m,F_u,F_v,F_w),Fv​=(m−1−κ)v,Fw​=(−m−1−κ)w,F=(Fm​,Fu​,Fv​,Fw​),

and E(m,v)=(m−1)2+v2E(m,v)=(m-1)^2+v^2E(m,v)=(m−1)2+v2.

For x=(p,s,a,b,c)x=(p,s,a,b,c)x=(p,s,a,b,c), put

ψ(p,z)=3 z1+p,Π(x)=(ψ(p,s),ψ(p,a),ψ(p,b),ψ(p,c)).\psi(p,z)=\frac{\sqrt3\,z}{1+p},\qquad \Pi(x)=(\psi(p,s),\psi(p,a),\psi(p,b),\psi(p,c)).ψ(p,z)=1+p3​z​,Π(x)=(ψ(p,s),ψ(p,a),ψ(p,b),ψ(p,c)).

For y=(m,u,v,w)y=(m,u,v,w)y=(m,u,v,w), set D(y)=3+m2+K(u,v,w)D(y)=3+m^2+K(u,v,w)D(y)=3+m2+K(u,v,w) and

ΞA(y)=(A−1,Am3,Au3,Av3,Aw3),Ξ(y)=Ξ6/D(y)(y).\Xi_A(y)=\left(A-1,\frac{Am}{\sqrt3},\frac{Au}{\sqrt3}, \frac{Av}{\sqrt3},\frac{Aw}{\sqrt3}\right),\qquad \Xi(y)=\Xi_{6/D(y)}(y).ΞA​(y)=(A−1,3​Am​,3​Au​,3​Av​,3​Aw​),Ξ(y)=Ξ6/D(y)​(y).

Write N(x)=(P,Q,r1a,r2b,r3c)N(x)=(P,Q,r_1a,r_2b,r_3c)N(x)=(P,Q,r1​a,r2​b,r3​c) for the normalized vector field and C(x)=C(p,s,a,b,c)\mathcal C(x)=C(p,s,a,b,c)C(x)=C(p,s,a,b,c) for its constraint.

The normalized and projective state spaces are R5\mathbb R^5R5 and R4\mathbb R^4R4 with their finite-product norms. The maps Π,Ξ,D,F\Pi,\Xi,D,FΠ,Ξ,D,F act on these state spaces.

Define the core radius, angle, and clock factor by

r(m,v)=(m−1)2+v2,θ(m,v)=arsinh⁡1−mv,d(r,u,w)=1−(u−w)2r2.r(m,v)=\sqrt{(m-1)^2+v^2},\qquad \theta(m,v)=\operatorname{arsinh}\frac{1-m}{v},\qquad d(r,u,w)=1-\frac{(u-w)^2}{r^2}.r(m,v)=(m−1)2+v2​,θ(m,v)=arsinhv1−m​,d(r,u,w)=1−r2(u−w)2​.

For y=(m,u,v,w)y=(m,u,v,w)y=(m,u,v,w), write ry=r(m,v)r_y=r(m,v)ry​=r(m,v), θy=θ(m,v)\theta_y=\theta(m,v)θy​=θ(m,v), and dy=d(ry,u,w)d_y=d(r_y,u,w)dy​=d(ry​,u,w). All quotients use the total convention x/0=0x/0=0x/0=0.

The core state space is R3\mathbb R^3R3 with coordinates Y=(r,u,p)Y=(r,u,p)Y=(r,u,p). Define

η(m,u,v,w)=(r(m,v),u,vw),ιz(r,u,p)=(1−rtanh⁡z,u,rcosh⁡z,pr/cosh⁡z).\eta(m,u,v,w)=(r(m,v),u,vw),\qquad \iota_z(r,u,p)=\left(1-r\tanh z,u,\frac r{\cosh z}, \frac p{r/\cosh z}\right).η(m,u,v,w)=(r(m,v),u,vw),ιz​(r,u,p)=(1−rtanhz,u,coshzr​,r/coshzp​).

For fixed (z,Y)(z,Y)(z,Y) put v=r/cosh⁡zv=r/\cosh zv=r/coshz, w=p/vw=p/vw=p/v, d=d(r,u,w)d=d(r,u,w)d=d(r,u,w), and define

V(z,Y)=(−κ(u,v,w)−tanh⁡z (u−w)2/rd,u[−r/2+tanh⁡z+w/cosh⁡z+(u2−w2)/(2r)]d,−2p(1+κ(u,v,w))rd).\mathcal V(z,Y)=\left( \frac{-\kappa(u,v,w)-\tanh z\,(u-w)^2/r}{d},\quad \frac{u[-r/2+\tanh z+w/\cosh z+(u^2-w^2)/(2r)]}{d},\quad \frac{-2p(1+\kappa(u,v,w))}{rd}\right).V(z,Y)=(d−κ(u,v,w)−tanhz(u−w)2/r​,du[−r/2+tanhz+w/coshz+(u2−w2)/(2r)]​,rd−2p(1+κ(u,v,w))​).

At (z,Y)(z,Y)(z,Y) use the abbreviations

s=1/cosh⁡z,c=−tanh⁡z,δ=u−w,s=1/\cosh z,\quad c=-\tanh z,\quad \delta=u-w,s=1/coshz,c=−tanhz,δ=u−w, C=u(v+w−u),a=−r/2+tanh⁡z+w/cosh⁡z+(u2−w2)/(2r),g=−C+cδ2/r.C=u(v+w-u),\quad a=-r/2+\tanh z+w/\cosh z+(u^2-w^2)/(2r), \quad g=-C+c\delta^2/r.C=u(v+w−u),a=−r/2+tanhz+w/coshz+(u2−w2)/(2r),g=−C+cδ2/r.

Let Q(z,Y)=(C,d,a,g)\mathcal Q(z,Y)=(C,d,a,g)Q(z,Y)=(C,d,a,g). Define the 4×34\times34×3 matrix H(z,Y)H(z,Y)H(z,Y) by its rows, in the order (C,d,a,g)(C,d,a,g)(C,d,a,g) and columns (r,u,p)(r,u,p)(r,u,p):

HC=(u(s−w/r), v−2u+w, u/v),H_C=(u(s-w/r),\ v-2u+w,\ u/v),HC​=(u(s−w/r), v−2u+w, u/v), Hd=(2δ(u−2w)/r3, −2δ/r2, 2δ/(vr2)),H_d=(2\delta(u-2w)/r^3,\ -2\delta/r^2,\ 2\delta/(vr^2)),Hd​=(2δ(u−2w)/r3, −2δ/r2, 2δ/(vr2)), Ha=(−1/2−sw/r+(3w2−u2)/(2r2), u/r, (1−w/v)/r),H_a=(-1/2-sw/r+(3w^2-u^2)/(2r^2),\ u/r,\ (1-w/v)/r),Ha​=(−1/2−sw/r+(3w2−u2)/(2r2), u/r, (1−w/v)/r), Hg=(−u(s−w/r)+cδ(3w−u)/r2, −(v−2u+w)+2cδ/r, −u/v−2cδ/(rv)).H_g=(-u(s-w/r)+c\delta(3w-u)/r^2,\ -(v-2u+w)+2c\delta/r,\ -u/v-2c\delta/(rv)).Hg​=(−u(s−w/r)+cδ(3w−u)/r2, −(v−2u+w)+2cδ/r, −u/v−2cδ/(rv)).

For j=0,1,2j=0,1,2j=0,1,2, define the 3×33\times33×3 matrix A(z,Y)A(z,Y)A(z,Y) by

A0j=Hgj/d−gHdj/d2,A_{0j}=H_{gj}/d-gH_{dj}/d^2,A0j​=Hgj​/d−gHdj​/d2, A1j=δj1a/d+uHaj/d−uaHdj/d2,A_{1j}=\delta_{j1}a/d+uH_{aj}/d-uaH_{dj}/d^2,A1j​=δj1​a/d+uHaj​/d−uaHdj​/d2, A2j=δj02p(1+C)r2d−δj22(1+C)rd−2pHCjrd+2p(1+C)Hdjrd2,A_{2j}=\delta_{j0}\frac{2p(1+C)}{r^2d} -\delta_{j2}\frac{2(1+C)}{rd}-\frac{2pH_{Cj}}{rd} +\frac{2p(1+C)H_{dj}}{rd^2},A2j​=δj0​r2d2p(1+C)​−δj2​rd2(1+C)​−rd2pHCj​​+rd22p(1+C)Hdj​​,

where δij\delta_{ij}δij​ is the Kronecker symbol.

For real kkk, define Sk(ξ0,ξ1,ξ2)=(ξ0,kξ1,ξ2)S_k(\xi_0,\xi_1,\xi_2)=(\xi_0,k\xi_1,\xi_2)Sk​(ξ0​,ξ1​,ξ2​)=(ξ0​,kξ1​,ξ2​) and

Bk(z,Y)=(A00A01/kA02kA10A11kA12A20A21/kA22).B_k(z,Y)=\begin{pmatrix} A_{00}&A_{01}/k&A_{02}\\ kA_{10}&A_{11}&kA_{12}\\ A_{20}&A_{21}/k&A_{22} \end{pmatrix}.Bk​(z,Y)=​A00​kA10​A20​​A01​/kA11​A21​/k​A02​kA12​A22​​​.

In the following coefficient estimate, assume

k≥6,99k100≤r≤101k100,v=rcosh⁡z≥1,k\geq6,\qquad \frac{99k}{100}\leq r\leq\frac{101k}{100}, \qquad v=\frac r{\cosh z}\geq1,k≥6,10099k​≤r≤100101k​,v=coshzr​≥1, 0≤u,w≤εk,εk=110000k,w=p/v.0\leq u,w\leq\varepsilon_k,\qquad \varepsilon_k=\frac1{10000k},\qquad w=p/v.0≤u,w≤εk​,εk​=10000k1​,w=p/v.

For B=Bk(z,Y)B=B_k(z,Y)B=Bk​(z,Y),

∣B00∣≤8(u+w2/k2),∣B01+v/k∣≤8(u+w)/k,∣B02∣≤8(u+w/k)/v.|B_{00}|\leq8(u+w^2/k^2),\qquad |B_{01}+v/k|\leq8(u+w)/k,\qquad |B_{02}|\leq8(u+w/k)/v.∣B00​∣≤8(u+w2/k2),∣B01​+v/k∣≤8(u+w)/k,∣B02​∣≤8(u+w/k)/v.
Preamble
import Definitions.Def_BianchiIX_Dynamics_CoreAngle
import Definitions.Def_BianchiIX_Dynamics_CoreAuxiliary
import Definitions.Def_BianchiIX_Dynamics_CoreWeightedVariation
import Mathlib.Analysis.Calculus.Deriv.Pow
import Mathlib.Analysis.Calculus.Deriv.Mul
import Mathlib.Analysis.Calculus.Deriv.Add
import Mathlib.Analysis.Real.Sqrt
import Mathlib.Tactic.Linarith
import Mathlib.Tactic.Ring
import Mathlib.Analysis.SpecialFunctions.Arsinh
import Mathlib.Analysis.SpecialFunctions.Sqrt
import Mathlib.Tactic.FieldSimp
import Mathlib.Analysis.Calculus.ContDiff.Operations
import Mathlib.Analysis.Calculus.Deriv.Prod
import Mathlib.Analysis.Calculus.MeanValue
import Mathlib.Data.Fin.VecNotation
import Mathlib.Tactic.FinCases
import Mathlib.Tactic.FunProp
import Mathlib.Analysis.Calculus.Deriv.Inv
import Mathlib.Tactic.LinearCombination
import Mathlib.Analysis.SpecialFunctions.Arcosh
import Mathlib.MeasureTheory.Integral.IntervalIntegral.FundThmCalculus
import Mathlib.Analysis.Calculus.InverseFunctionTheorem.Deriv
import Mathlib.Analysis.Calculus.Deriv.MeanValue
import Mathlib.Analysis.SpecialFunctions.Pow.Deriv
import Mathlib.Analysis.SpecialFunctions.Integrals.Basic
import Mathlib.Analysis.ODE.ExistUnique
import Mathlib.Data.Matrix.Mul
import Mathlib.Algebra.BigOperators.Fin
import Mathlib.Topology.Instances.Real.Lemmas
import Mathlib.Analysis.Calculus.FDeriv.Partial
import Mathlib.MeasureTheory.Integral.IntervalIntegral.DistLEIntegral
import Mathlib.Tactic.GCongr
import Mathlib.Analysis.Calculus.Deriv.Slope
import Mathlib.Topology.Order.OrderClosed

noncomputable section
open BianchiIX

Formal statement
theorem BianchiIX.coreWeightedJacobian_amplitude_bounds {k z : ℝ} {y : CoreAngleState}
    (hk : 6 ≤ k) (hr : 99 / 100 * k ≤ y 0 ∧ y 0 ≤ 101 / 100 * k)
    (hv : 1 ≤ y 0 / Real.cosh z)
    (hu : 0 ≤ y 1 ∧ y 1 ≤ (1 / 10000) / k)
    (hw : 0 ≤ y 2 / (y 0 / Real.cosh z) ∧ y 2 / (y 0 / Real.cosh z) ≤ (1 / 10000) / k) :
    let v := y 0 / Real.cosh z
    let w := y 2 / v
    let b := coreWeightedJacobian k z y
    |b 0 0| ≤ 8 * (y 1 + w ^ 2 / k ^ 2) ∧
    |b 0 1 + v / k| ≤ 8 * (y 1 + w) / k ∧
    |b 0 2| ≤ 8 * (y 1 + w / k) / v := by sorry
Source
https://github.com/l46430640-del/ERA-STATISTICS-FORMAL/blob/d74c241819f896ab8d050b21ace80c8e90eabd9e/BianchiIX/Dynamics/CoreAmplitudeBounds.lean#L46-L110

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