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Amplitude and radial scales of the corrected phase coefficients

Proved
BianchiIX.stableCorrectedPhase_coefficient_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.

The projective vector field in normalized time is

G(y)=6D(y)F(y).G(y)=\frac6{D(y)}F(y).G(y)=D(y)6​F(y).

Write X=R5X=\mathbb R^5X=R5, Y=R4Y=\mathbb R^4Y=R4, and let αx,t0\alpha_{x,t_0}αx,t0​​ be the maximal solution of α′=N(α)\alpha'=N(\alpha)α′=N(α) with initial value xxx at t0t_0t0​ and domain Imax⁡(x,t0)I_{\max}(x,t_0)Imax​(x,t0​). Put

Jx,t0(t)=dxαx,t0(t),Ψt0(y,t)=Π(αΞ(y),t0(t)),J_{x,t_0}(t)=d_x\alpha_{x,t_0}(t),\qquad \Psi_{t_0}(y,t)=\Pi(\alpha_{\Xi(y),t_0}(t)),Jx,t0​​(t)=dx​αx,t0​​(t),Ψt0​​(y,t)=Π(αΞ(y),t0​​(t)), Jy,t0(t)=dΠαΞ(y),t0(t)∘JΞ(y),t0(t)∘dΞy.\mathcal J_{y,t_0}(t)=d\Pi_{\alpha_{\Xi(y),t_0}(t)} \circ J_{\Xi(y),t_0}(t)\circ d\Xi_y.Jy,t0​​(t)=dΠαΞ(y),t0​​(t)​∘JΞ(y),t0​​(t)∘dΞy​.

On the invariant plane with zero active wall, use y=(m,u,w)∈R3y=(m,u,w)\in\mathbb R^3y=(m,u,w)∈R3, the inclusion ι(m,u,w)=(m,u,0,w)\iota(m,u,w)=(m,u,0,w)ι(m,u,w)=(m,u,0,w) and the restriction πs(m,u,v,w)=(m,u,w)\pi_s(m,u,v,w)=(m,u,w)πs​(m,u,v,w)=(m,u,w). Define

f(y)=(mu2−(m+1)uw+w2,1−m2−w2+u22u,−(m+1+uw−u2)w),f(y)=\left(mu^2-(m+1)uw+w^2, \frac{1-m^2-w^2+u^2}{2}u,-(m+1+uw-u^2)w\right),f(y)=(mu2−(m+1)uw+w2,21−m2−w2+u2​u,−(m+1+uw−u2)w), Δ(y)=3+m2+(u−w)2,fo(y)=6f(y)/Δ(y).\Delta(y)=3+m^2+(u-w)^2,\qquad f_o(y)=6f(y)/\Delta(y).Δ(y)=3+m2+(u−w)2,fo​(y)=6f(y)/Δ(y).

Write J=dfJ=dfJ=df, H=d2fH=d^2fH=d2f, Jo=dfoJ_o=df_oJo​=dfo​, Ho=d2foH_o=d^2f_oHo​=d2fo​ for their explicit Jacobian and Hessian expressions. The denominator derivatives are dΔ=(2m,2(u−w),2(w−u))d\Delta=(2m,2(u-w),2(w-u))dΔ=(2m,2(u−w),2(w−u)) and d2Δ(v,z)=2v0z0+2(v1−v2)(z1−z2)d^2\Delta(v,z)=2v_0z_0+2(v_1-v_2)(z_1-z_2)d2Δ(v,z)=2v0​z0​+2(v1​−v2​)(z1​−z2​). The exact original-time boundary flow and its projected variation are

Φ(y,t)=πsΨ0(ιy,t),L(y,t)=πsJιy,0(t)ι.\Phi(y,t)=\pi_s\Psi_0(\iota y,t),\qquad L(y,t)=\pi_s\mathcal J_{\iota y,0}(t)\iota.Φ(y,t)=πs​Ψ0​(ιy,t),L(y,t)=πs​Jιy,0​(t)ι.

For a fixed scale KKK, set ΦK(y,s)=Φ(y,Ks)\Phi_K(y,s)=\Phi(y,Ks)ΦK​(y,s)=Φ(y,Ks), LK(y,s)=L(y,Ks)L_K(y,s)=L(y,Ks)LK​(y,s)=L(y,Ks) and QK(y,s)=dyLK(y,s)Q_K(y,s)=d_yL_K(y,s)QK​(y,s)=dy​LK​(y,s). For directions v,zv,zv,z, define

SK(y,s;v,z)=K[Ho(ΦK)(LKv,LKz)+Jo(ΦK)QK(v,z)].S_K(y,s;v,z)=K\left[H_o(\Phi_K)(L_Kv,L_Kz)+J_o(\Phi_K)Q_K(v,z)\right].SK​(y,s;v,z)=K[Ho​(ΦK​)(LK​v,LK​z)+Jo​(ΦK​)QK​(v,z)].

All vector norms are sup norms, and operator norms are induced by them. Write b(y)=∣u∣+∣w∣b(y)=|u|+|w|b(y)=∣u∣+∣w∣, E(y)=e512b(y)E(y)=e^{512b(y)}E(y)=e512b(y), vs=(v1,v2)v_s=(v_1,v_2)vs​=(v1​,v2​), and

H(y;v,z)=b(y)∥v∥∥z∥+∥vs∥∥z∥+∥v∥∥zs∥,\mathcal H(y;v,z)=b(y)\|v\|\|z\|+\|v_s\|\|z\|+\|v\|\|z_s\|,H(y;v,z)=b(y)∥v∥∥z∥+∥vs​∥∥z∥+∥v∥∥zs​∥, B2(y)=192b(y)(40000E(y)3)+10000E(y)2.B_2(y)=192b(y)(40000E(y)^3)+10000E(y)^2.B2​(y)=192b(y)(40000E(y)3)+10000E(y)2.

The closed boundary region is Sc={(m,u,0,w):∣m−c∣≤1/10, ∣u∣,∣w∣≤1/100}\mathcal S_c=\{(m,u,0,w):|m-c|\leq1/10,\ |u|,|w|\leq1/100\}Sc​={(m,u,0,w):∣m−c∣≤1/10, ∣u∣,∣w∣≤1/100}. The boundary projection P(m,u,w)P(m,u,w)P(m,u,w) is the limit of Φ(m,u,w;t)0\Phi(m,u,w;t)_0Φ(m,u,w;t)0​ as t→∞t\to\inftyt→∞, using the total limit convention of the formal definitions.

Set r=(m+1)2+w2r=\sqrt{(m+1)^2+w^2}r=(m+1)2+w2​ and

A(m)=mm2−1,C(m)=−2m+1,Θ(m,u,w)=r−1+A(m)u2+C(m)uw.A(m)=\frac{m}{m^2-1},\quad C(m)=-\frac2{m+1},\quad \Theta(m,u,w)=r-1+A(m)u^2+C(m)uw.A(m)=m2−1m​,C(m)=−m+12​,Θ(m,u,w)=r−1+A(m)u2+C(m)uw.

Its explicit gradient is used together with the residual R=r4u4+r3u3w+r2u2w2+r1uw3R=r_4u^4+r_3u^3w+r_2u^2w^2+r_1uw^3R=r4​u4+r3​u3w+r2​u2w2+r1​uw3, where

r4=−2m(m2−1)2,r3=2(3m−1)(m2−1)2,r_4=-\frac{2m}{(m^2-1)^2},\quad r_3=\frac{2(3m-1)}{(m^2-1)^2},r4​=−(m2−1)22m​,r3​=(m2−1)22(3m−1)​, r2=−m2+1(m2−1)2−mm2−1+r+1r(r+m+1),r1=2(m+1)2+1m+1−1r+m+1.r_2=-\frac{m^2+1}{(m^2-1)^2}-\frac m{m^2-1} +\frac{r+1}{r(r+m+1)},\quad r_1=\frac2{(m+1)^2}+\frac1{m+1}-\frac1{r+m+1}.r2​=−(m2−1)2m2+1​−m2−1m​+r(r+m+1)r+1​,r1​=(m+1)22​+m+11​−r+m+11​.

Write L=m+1L=m+1L=m+1, b=∣u∣+∣w∣b=|u|+|w|b=∣u∣+∣w∣, vs=(v1,v2)v_s=(v_1,v_2)vs​=(v1​,v2​), and set

Wb(v)=b∥v∥+∥vs∥,Hs(y;v,z)=∣u∣∥v∥∥z∥+∣v0∣∣z1∣+∣v1∣∣z0∣+b(∣v1∣∥z∥+∥v∥∣z1∣).W_b(v)=b\|v\|+\|v_s\|,\quad H_s(y;v,z)=|u|\|v\|\|z\|+|v_0||z_1|+|v_1||z_0| +b(|v_1|\|z\|+\|v\||z_1|).Wb​(v)=b∥v∥+∥vs​∥,Hs​(y;v,z)=∣u∣∥v∥∥z∥+∣v0​∣∣z1​∣+∣v1​∣∣z0​∣+b(∣v1​∣∥z∥+∥v∥∣z1​∣).

The corrected and quadratic remainders are

Rc=P−Θ,Rq=P−(m+A(m)u2+C(m)uw+w22L).R_c=P-\Theta,\quad R_q=P-\left(m+A(m)u^2+C(m)uw+\frac{w^2}{2L}\right).Rc​=P−Θ,Rq​=P−(m+A(m)u2+C(m)uw+2Lw2​).

For K∈RK\in\mathbb RK∈R, let ai(K,y)=6Kr4−i(m,w)/Δ(y)a_i(K,y)=6K r_{4-i}(m,w)/\Delta(y)ai​(K,y)=6Kr4−i​(m,w)/Δ(y), where r4,r3r_4,r_3r4​,r3​ are independent of www, and put

M(y)=(u3,u2w,uw2,w3),CK(y)=∑i=03ai(K,y)Mi(y),M(y)=(u^3,u^2w,uw^2,w^3),\quad C_K(y)=\sum_{i=0}^3a_i(K,y)M_i(y),M(y)=(u3,u2w,uw2,w3),CK​(y)=i=0∑3​ai​(K,y)Mi​(y), gK,s(y)=6KΔ(ΦK(y,s))R(ΦK(y,s)).g_{K,s}(y)=\frac{6K}{\Delta(\Phi_K(y,s))}R(\Phi_K(y,s)).gK,s​(y)=Δ(ΦK​(y,s))6K​R(ΦK​(y,s)).

The cubic derivative budgets are

B1(y;v)=b3∥v∥+3b2∥vs∥,B_1(y;v)=b^3\|v\|+3b^2\|v_s\|,B1​(y;v)=b3∥v∥+3b2∥vs​∥, B2c(y;v,z)=b3∥v∥∥z∥+3b2(∥v∥∥zs∥+∥vs∥∥z∥)+6b∥vs∥∥zs∥.B_2^c(y;v,z)=b^3\|v\|\|z\| +3b^2(\|v\|\|z_s\|+\|v_s\|\|z\|)+6b\|v_s\|\|z_s\|.B2c​(y;v,z)=b3∥v∥∥z∥+3b2(∥v∥∥zs​∥+∥vs​∥∥z∥)+6b∥vs​∥∥zs​∥.

A direction is radial if its last two coordinates vanish, and transverse if its zeroth coordinate vanishes. For m≥2m\geq2m≥2 and arbitrary signed u,wu,wu,w,

∣Θm−1∣≤8b2/L2,∣Θu∣≤6b/L,∣Θw∣≤3b/L,|\Theta_m-1|\leq8b^2/L^2,\quad|\Theta_u|\leq6b/L,\quad|\Theta_w|\leq3b/L,∣Θm​−1∣≤8b2/L2,∣Θu​∣≤6b/L,∣Θw​∣≤3b/L, ∣Θmm∣≤33b2/L3,∣Θmu∣≤12b/L2,∣Θmw∣≤3b/L2.|\Theta_{mm}|\leq33b^2/L^3,\quad |\Theta_{mu}|\leq12b/L^2,\quad|\Theta_{mw}|\leq3b/L^2.∣Θmm​∣≤33b2/L3,∣Θmu​∣≤12b/L2,∣Θmw​∣≤3b/L2.
Preamble
import Definitions.Def_BianchiIX_Algebra_MatchingPhase
import Definitions.Def_BianchiIX_CompactPhaseExpansionData
import Definitions.Def_BianchiIX_StableProjectionRefinementData
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.Calculus.Deriv.Inv
import Mathlib.Tactic.FieldSimp
import Mathlib.Tactic.LinearCombination
import Mathlib.Analysis.SpecialFunctions.Sqrt
import Mathlib.Analysis.SpecialFunctions.Pow.Deriv
import Mathlib.Analysis.Calculus.ContDiff.Comp
import Mathlib.Analysis.Calculus.Deriv.Comp

noncomputable section
open BianchiIX

Formal statement
theorem BianchiIX.stableCorrectedPhase_coefficient_bounds {m u w : ℝ} (hm : 2 ≤ m) :
    let b := |u| + |w|
    |stableCorrectedGradient m u w 0 - 1| ≤ 8 / (m + 1) ^ 2 * b ^ 2 ∧
      |stableCorrectedGradient m u w 1| ≤ 6 / (m + 1) * b ∧
      |stableCorrectedGradient m u w 2| ≤ 3 / (m + 1) * b ∧
      |w ^ 2 / stableWeakRadius m w ^ 3 + stableCorrectionASecond m * u ^ 2 +
        stableCorrectionCSecond m * u * w| ≤ 33 / (m + 1) ^ 3 * b ^ 2 ∧
      |2 * stableCorrectionADeriv m * u + stableCorrectionCDeriv m * w| ≤ 12 / (m + 1) ^ 2 * b ∧
      |-(m + 1) * w / stableWeakRadius m w ^ 3 + stableCorrectionCDeriv m * u| ≤ 3 / (m + 1) ^ 2 * b := by sorry
Source
https://github.com/l46430640-del/ERA-STATISTICS-FORMAL/blob/d74c241819f896ab8d050b21ace80c8e90eabd9e/BianchiIX/Algebra/StablePhaseJetBounds.lean#L7-L72

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