The degree-two value for the root frame
Part of the conditional-fiber mechanism, Chapter Conditional fibers: inverse-variance frames of line resamplings ; the reading order is on the full proofs page.
Overview. This dossier proves Lemma 22.2 as Theorem D11.1 : for every m ≥ 3 m\ge3 m ≥ 3 , the root-frame pencil on the degree-two quotient V m , 2 V_{m,2} V m , 2 of the uniform simplex has λ min ( K , G ) = ( m + 2 ) ( m + 3 ) / ( 5 m 2 ) \lmin(K,G)=(m+2)(m+3)/(5m^2) λ m i n ( K , G ) = ( m + 2 ) ( m + 3 ) / ( 5 m 2 ) , attained exactly on the radial quadratic. The proof splits V m , 2 V_{m,2} V m , 2 into S m S_m S m -isotypic sectors, reduces the pencil on each to a small Gram matrix, and evaluates these exactly with Dirichlet moments. The corollary is conditional on the identification (D11.8) and lives inside the candidate degree-k k k dual-certificate framework. It rules out degree-two dual refuters and says nothing about degrees k ≥ 3 k\ge3 k ≥ 3 , non-polynomial tests or KLS.
Exact Dirichlet moments (Lemma D11.1 ) and the pair-fiber decomposition (Lemma D11.2 ). On each pair fiber, δ / s \delta/s δ / s is uniform on [ − 1 , 1 ] [-1,1] [ − 1 , 1 ] , which gives the pair-energy formula (D11.17) ; hence K K K is finite and positive semidefinite on V m , 2 V_{m,2} V m , 2 .
Symmetry: Lemma D11.3 and Lemma D11.4 show V m , 2 ≅ t r i v ⊕ s t d ⊗ R 2 ⊕ X V_{m,2}\cong\mathrm{triv}\oplus\mathrm{std}\otimes\R^2\oplus\mathrm X V m , 2 ≅ triv ⊕ std ⊗ R 2 ⊕ X , with explicit generators f 0 f_0 f 0 , ( L , Q ) (L,Q) ( L , Q ) and F F F .
Lemma D11.5 shows that invariant forms do not couple different sectors. Positivity on each sector therefore reduces to a Gram matrix of seed vectors.
Sector computations from steps 1–2: in the trivial sector the ratio is exactly λ ∗ \lambda^* λ ∗ (Lemma D11.6 ); the standard sector reduces to a 2 × 2 2\times2 2 × 2 Gram matrix (Lemma D11.7 ); the two-row sector reduces to a scalar (Lemma D11.8 ).
Assembly: K − λ ∗ G K-\lambda^*G K − λ ∗ G vanishes on the trivial sector. It is positive definite on the standard sector ((D11.41) ) and on X \mathrm X X . This proves (D11.5) together with its equality case.
Corollary Corollary D11.1 , under its stated hypothesis: averaging a certificate over the root-frame atoms and applying the theorem gives ε ≥ λ ∗ > 1 5 \eps\ge\lambda^*>\tfrac15 ε ≥ λ ∗ > 5 1 , and also gives Λ m , 2 ≥ λ ∗ \Lambda_{m,2}\ge\lambda^* Λ m , 2 ≥ λ ∗ .
Scope. This dossier proves an exact finite-dimensional spectral identity for the A m − 1 A_{m-1} A m − 1 root-frame conditional-fiber form of Route F (Conditional fibers: inverse-variance frames of line resamplings ) restricted to polynomial test functions of degree at most two, for every m ≥ 3 m\ge3 m ≥ 3 simultaneously. The statement was suggested by exact rational computations at m = 3 , … , 15 m=3,\dots,15 m = 3 , … , 15 recorded in provenance-stamped run artifacts (see Remark D11.1 ); no step of any proof below uses those computations. The main theorem is unconditional and self-contained. The corollary is stated only as a conditional, refutation-channel statement inside the candidate degree-k k k dual-certificate framework for Conjecture 22.1 ; it makes no claim about the all-frame gate itself, about degrees k ≥ 3 k\ge3 k ≥ 3 , about non-polynomial tests, or about KLS.
Setting. Let m ≥ 3 m\ge3 m ≥ 3 , let Δ m − 1 = { p ∈ R + m : ∑ i p i = 1 } \Delta_{m-1}=\{p\in\R_+^m:\sum_ip_i=1\} Δ m − 1 = { p ∈ R + m : ∑ i p i = 1 } , and let P = ( P 1 , … , P m ) P=(P_1,\dots,P_m) P = ( P 1 , … , P m ) be uniform on Δ m − 1 \Delta_{m-1} Δ m − 1 , i.e. P ∼ Dir ( 1 , … , 1 ) P\sim\Dir(1,\dots,1) P ∼ Dir ( 1 , … , 1 ) ; write μ \mu μ for its law. Put H 0 = 1 ⊥ H_0=\one^\perp H 0 = 1 ⊥ , d = m − 1 d=m-1 d = m − 1 , R m = m ( m + 1 ) R_m=\sqrt{m(m+1)} R m = m ( m + 1 ) , and
X = R m ( P − 1 m 1 ) ∈ H 0 , X=R_m\Bigl(P-\frac1m\one\Bigr)\in H_0, X = R m ( P − m 1 1 ) ∈ H 0 , which is isotropic on H 0 H_0 H 0 (uniform-simplex root proposition of the certified dossier solutions/conditional-fiber-frame-structure.md; this normalization is not used before the corollary). The symmetric group S m S_m S m acts on functions by permuting the coordinates of p p p , and μ \mu μ is exchangeable, so S m S_m S m acts by isometries of L 2 ( μ ) L^2(\mu) L 2 ( μ ) .
For i < j i<j i < j let F i j = σ ( ( P ℓ ) ℓ ≠ i , j ) \mathcal F_{ij}=\sigma\bigl((P_\ell)_{\ell\ne i,j}\bigr) F ij = σ ( ( P ℓ ) ℓ = i , j ) , let s i j = P i + P j s_{ij}=P_i+P_j s ij = P i + P j (an F i j \mathcal F_{ij} F ij -measurable variable, since s i j = 1 − ∑ ℓ ≠ i , j P ℓ s_{ij}=1-\sum_{\ell\ne i,j}P_\ell s ij = 1 − ∑ ℓ = i , j P ℓ ), and write Var i j \Var_{ij} Var ij and Cov i j \Cov_{ij} Cov ij for conditional variance and covariance given F i j \mathcal F_{ij} F ij . Define, for f , g ∈ L 2 ( μ ) f,g\in L^2(\mu) f , g ∈ L 2 ( μ ) with all the conditional quantities finite,
The quadratic form K ( f , f ) K(f,f) K ( f , f ) is exactly the root-frame conditional-fiber form D r o o t ( f ) \mathcal D_{\rm root}(f) D root ( f ) of (22.9) , as proved in the certified dossier above (its equation defining the root form); for the main theorem, (D11.2) is simply taken as the definition, so the theorem does not depend on that identification. Both K K K and G G G depend only on the μ \mu μ -equivalence classes of f , g f,g f , g , vanish when one argument is a.e. constant, and are S m S_m S m -invariant (exchangeability of μ \mu μ and invariance of the family of pairs).
Let W p o l y W_{\rm poly} W poly be the linear span of the monomials p i p_i p i (1 ≤ i ≤ m 1\le i\le m 1 ≤ i ≤ m ) and p i p j p_ip_j p i p j (1 ≤ i ≤ j ≤ m 1\le i\le j\le m 1 ≤ i ≤ j ≤ m ), i.e. all polynomials of degree at most 2 with zero constant term, and define the degree-two quotient
V m , 2 = { [ f ] : f ∈ W p o l y } ⊂ L 2 ( μ ) / R 1 , V_{m,2}
=\bigl\{[f]:f\in W_{\rm poly}\bigr\}
\subset L^2(\mu)\big/\R\one, V m , 2 = { [ f ] : f ∈ W poly } ⊂ L 2 ( μ ) / R 1 , where [ f ] [f] [ f ] denotes the class of f f f modulo additive constants. On V m , 2 V_{m,2} V m , 2 the form G = Var G=\Var G = Var is positive definite by construction, K K K is positive semidefinite and finite (Lemma D11.2 ), and both are S m S_m S m -invariant. The generalized minimum eigenvalue of the pencil is
λ min ( K , G ) ∣ V m , 2 = min 0 ≠ v ∈ V m , 2 K ( v , v ) G ( v , v ) . \lmin(K,G)\big|_{V_{m,2}}
=\min_{0\ne v\in V_{m,2}}\frac{K(v,v)}{G(v,v)}. λ m i n ( K , G ) ∣ ∣ V m , 2 = 0 = v ∈ V m , 2 min G ( v , v ) K ( v , v ) . Statements ¶ For every m ≥ 3 m\ge3 m ≥ 3 ,
λ min ( K , G ) ∣ V m , 2 = ( m + 2 ) ( m + 3 ) 5 m 2 , \lmin(K,G)\big|_{V_{m,2}}
=\frac{(m+2)(m+3)}{5m^2}, λ m i n ( K , G ) ∣ ∣ V m , 2 = 5 m 2 ( m + 2 ) ( m + 3 ) , and the minimum is attained exactly on the one-dimensional line R ⋅ [ ∑ i p i 2 ] = R ⋅ [ ∣ X ∣ 2 − ( m − 1 ) ] \R\cdot\bigl[\textstyle\sum_i p_i^2\bigr] =\R\cdot\bigl[\abs{X}^2-(m-1)\bigr] R ⋅ [ ∑ i p i 2 ] = R ⋅ [ ∣ X ∣ 2 − ( m − 1 ) ] spanned by the radial quadratic. In particular λ min ( K , G ) ∣ V m , 2 > 1 5 \lmin(K,G)|_{V_{m,2}}>\tfrac15 λ m i n ( K , G ) ∣ V m , 2 > 5 1 for every m ≥ 3 m\ge3 m ≥ 3 , and λ min ( K , G ) ∣ V m , 2 → 1 5 \lmin(K,G)|_{V_{m,2}}\to\tfrac15 λ m i n ( K , G ) ∣ V m , 2 → 5 1 as m → ∞ m\to\infty m → ∞ .
The corollary below lives inside the candidate degree-k k k dual-certificate framework for the simplex falsification channel of Conjecture 22.1 (the all-frame min–max Λ m , k \Lambda_{m,k} Λ m , k and its exact dual certificates; an exploratory framework, not a statement of the manuscript). We restate the needed objects to be self-contained. Write S ( H 0 ) S(H_0) S ( H 0 ) for the unit sphere of H 0 H_0 H 0 . For θ ∈ S ( H 0 ) \theta\in S(H_0) θ ∈ S ( H 0 ) and f f f a polynomial, let
q θ [ f ] = ∫ θ ⊥ Var μ θ , z ( f ( z + T θ ) ) Var μ θ , z ( T ) d μ ˉ θ ( z ) \qJac_\theta[f]
=\int_{\theta^\perp}
\frac{\Var_{\mu_{\theta,z}}\bigl(f(z+T\theta)\bigr)}
{\Var_{\mu_{\theta,z}}(T)}
\dd\bar\mu_\theta(z) q θ [ f ] = ∫ θ ⊥ Var μ θ , z ( T ) Var μ θ , z ( f ( z + Tθ ) ) d μ ˉ θ ( z ) be the single-direction normalized fiber energy of the certified structural dossier (with its null- and zero-variance-fiber conventions), a finite quantity for polynomial f f f by the certified factor-4 bound. An admissible frame is an even Borel probability ρ \rho ρ on S ( H 0 ) S(H_0) S ( H 0 ) with ( m − 1 ) ∫ θ θ T d ρ = I H 0 (m-1)\int\theta\theta^T\dd\rho=I_{H_0} ( m − 1 ) ∫ θ θ T d ρ = I H 0 . A degree-2 dual certificate with objective ε \eps ε is a finite family c 1 , … , c R ∈ V m , 2 c_1,\dots,c_R\in V_{m,2} c 1 , … , c R ∈ V m , 2 , weights w 1 , … , w R ≥ 0 w_1,\dots,w_R\ge0 w 1 , … , w R ≥ 0 , and a symmetric matrix M M M on H 0 H_0 H 0 such that
∑ r = 1 R w r G ( c r , c r ) = 1 , ∑ r = 1 R w r q θ [ c r ] ≤ θ T M θ for all θ ∈ S ( H 0 ) , Tr M ≤ ε . \sum_{r=1}^R w_r\,G(c_r,c_r)=1,
\qquad
\sum_{r=1}^R w_r\,\qJac_\theta[c_r]\le\theta^TM\theta
\quad\text{for all }\theta\in S(H_0),
\qquad
\Tr M\le\eps. r = 1 ∑ R w r G ( c r , c r ) = 1 , r = 1 ∑ R w r q θ [ c r ] ≤ θ T Mθ for all θ ∈ S ( H 0 ) , Tr M ≤ ε . By the weak-duality computation reproduced in the proof below, such a certificate forces every admissible frame ρ \rho ρ (for which the averaged form is defined) to have degree-two pencil gap at most ε \eps ε ; a sequence of such certificates with ε m → 0 \eps_m\to0 ε m → 0 at the fixed degree k = 2 k=2 k = 2 would therefore be the decisive fixed-degree refuter of the route on the simplex.
Assume the identification, certified in solutions/conditional-fiber-frame-structure.md (nodes lem:conditional-fiber-form and prop:conditional-fiber-root-obstruction ), of the pair-redistribution formula (D11.2) with the conditional-fiber form of the admissible A m − 1 A_{m-1} A m − 1 root frame, i.e.
K ( f , f ) = ( m − 1 ) ∫ S ( H 0 ) q θ [ f ] d ρ r o o t ( θ ) , ρ r o o t = 1 m ( m − 1 ) ∑ i ≠ j δ ( e i − e j ) / 2 . K(f,f)=(m-1)\int_{S(H_0)}\qJac_\theta[f]\dd\rho_{\rm root}(\theta),
\qquad
\rho_{\rm root}=\frac1{m(m-1)}\sum_{i\ne j}\delta_{(e_i-e_j)/\sqrt2}. K ( f , f ) = ( m − 1 ) ∫ S ( H 0 ) q θ [ f ] d ρ root ( θ ) , ρ root = m ( m − 1 ) 1 i = j ∑ δ ( e i − e j ) / 2 . Then for every m ≥ 3 m\ge3 m ≥ 3 :
every degree-2 dual certificate (D11.7) has
ε ≥ ( m + 2 ) ( m + 3 ) 5 m 2 > 1 5 ; \eps\;\ge\;\frac{(m+2)(m+3)}{5m^2}\;>\;\frac15; ε ≥ 5 m 2 ( m + 2 ) ( m + 3 ) > 5 1 ; consequently no sequence of degree-2 dual certificates with ε m → 0 \eps_m\to0 ε m → 0 exists, and within this framework any fixed-degree polynomial dual refutation of the conditional-fiber-frame route on the uniform simplex requires test degree k ≥ 3 k\ge3 k ≥ 3 ;
for every admissible frame ρ \rho ρ whose averaged degree-two form A ρ ( f , f ) = ( m − 1 ) ∫ q θ [ f ] d ρ ( θ ) A_\rho(f,f)=(m-1)\int\qJac_\theta[f]\dd\rho(\theta) A ρ ( f , f ) = ( m − 1 ) ∫ q θ [ f ] d ρ ( θ ) is defined on V m , 2 V_{m,2} V m , 2 , the all-frame degree-two min–max satisfies
Λ m , 2 : = sup ρ admissible min 0 ≠ v ∈ V m , 2 A ρ ( v , v ) G ( v , v ) ≥ ( m + 2 ) ( m + 3 ) 5 m 2 > 1 5 . \Lambda_{m,2}
:=\sup_{\rho\ \text{admissible}}
\ \min_{0\ne v\in V_{m,2}}\frac{A_\rho(v,v)}{G(v,v)}
\;\ge\;\frac{(m+2)(m+3)}{5m^2}\;>\;\frac15 . Λ m , 2 := ρ admissible sup 0 = v ∈ V m , 2 min G ( v , v ) A ρ ( v , v ) ≥ 5 m 2 ( m + 2 ) ( m + 3 ) > 5 1 . This corollary asserts nothing about upper bounds on Λ m , 2 \Lambda_{m,2} Λ m , 2 , about Λ m , k \Lambda_{m,k} Λ m , k for k ≥ 3 k\ge3 k ≥ 3 , about non-polynomial test functions, about the truth value of Conjecture 22.1 , or about KLS.
Preliminaries: moments and pair fibers ¶ For a ∈ N m a\in\mathbb N^m a ∈ N m with ∣ a ∣ = ∑ i a i \abs a=\sum_ia_i ∣ a ∣ = ∑ i a i ,
In particular, with D r = m ( m + 1 ) ⋯ ( m + r − 1 ) D_r=m(m+1)\cdots(m+r-1) D r = m ( m + 1 ) ⋯ ( m + r − 1 ) and distinct indices i , j , k , l i,j,k,l i , j , k , l :
E P i = 1 m , E P i 2 = 2 D 2 , E P i P j = 1 D 2 , E P i 3 = 6 D 3 , E P i 2 P j = 2 D 3 , E P i 4 = 24 D 4 , E P i 3 P j = 6 D 4 , E P i 2 P j 2 = 4 D 4 , E P i 2 P j P k = 2 D 4 , E P i P j P k P l = 1 D 4 . \begin{gathered}
\E P_i=\frac1m,\qquad
\E P_i^2=\frac2{D_2},\qquad
\E P_iP_j=\frac1{D_2},\\
\E P_i^3=\frac6{D_3},\qquad
\E P_i^2P_j=\frac2{D_3},\qquad
\E P_i^4=\frac{24}{D_4},\qquad
\E P_i^3P_j=\frac6{D_4},\\
\E P_i^2P_j^2=\frac4{D_4},\qquad
\E P_i^2P_jP_k=\frac2{D_4},\qquad
\E P_iP_jP_kP_l=\frac1{D_4}.
\end{gathered} E P i = m 1 , E P i 2 = D 2 2 , E P i P j = D 2 1 , E P i 3 = D 3 6 , E P i 2 P j = D 3 2 , E P i 4 = D 4 24 , E P i 3 P j = D 4 6 , E P i 2 P j 2 = D 4 4 , E P i 2 P j P k = D 4 2 , E P i P j P k P l = D 4 1 . Let E 1 , … , E m E_1,\dots,E_m E 1 , … , E m be i.i.d. standard exponentials and S = ∑ i E i S=\sum_iE_i S = ∑ i E i . By the classical Gamma–Dirichlet factorization, ( E 1 / S , … , E m / S ) ∼ Dir ( 1 , … , 1 ) (E_1/S,\dots,E_m/S)\sim\Dir(1,\dots,1) ( E 1 / S , … , E m / S ) ∼ Dir ( 1 , … , 1 ) and is independent of S ∼ Gamma ( m , 1 ) S\sim\GammaLaw(m,1) S ∼ Gamma ( m , 1 ) . Hence
∏ i a i ! = E ∏ i E i a i = E [ S ∣ a ∣ ∏ i P i a i ] = E S ∣ a ∣ ⋅ E ∏ i P i a i = ( m − 1 + ∣ a ∣ ) ! ( m − 1 ) ! E ∏ i P i a i , \prod_ia_i!
=\E\prod_iE_i^{a_i}
=\E\Bigl[S^{\abs a}\prod_iP_i^{a_i}\Bigr]
=\E S^{\abs a}\cdot\E\prod_iP_i^{a_i}
=\frac{(m-1+\abs a)!}{(m-1)!}\,\E\prod_iP_i^{a_i}, i ∏ a i ! = E i ∏ E i a i = E [ S ∣ a ∣ i ∏ P i a i ] = E S ∣ a ∣ ⋅ E i ∏ P i a i = ( m − 1 )! ( m − 1 + ∣ a ∣ )! E i ∏ P i a i , using E S r = Γ ( m + r ) / Γ ( m ) \E S^{r}=\Gamma(m+r)/\Gamma(m) E S r = Γ ( m + r ) /Γ ( m ) . Rearranging gives (D11.11) ; the table is immediate.
The following consequences are used repeatedly (i , j , a , b i,j,a,b i , j , a , b distinct):
E s i j = 2 m , E s i j 2 = 2 ⋅ 2 + 2 ⋅ 1 D 2 = 6 D 2 , E ( P a − P b ) 2 = 2 ⋅ 2 − 2 ⋅ 1 D 2 = 2 D 2 . \E s_{ij}=\frac2m,\qquad
\E s_{ij}^2=\frac{2\cdot2+2\cdot1}{D_2}=\frac6{D_2},\qquad
\E(P_a-P_b)^2=\frac{2\cdot2-2\cdot1}{D_2}=\frac2{D_2}. E s ij = m 2 , E s ij 2 = D 2 2 ⋅ 2 + 2 ⋅ 1 = D 2 6 , E ( P a − P b ) 2 = D 2 2 ⋅ 2 − 2 ⋅ 1 = D 2 2 . Fix i < j i<j i < j and abbreviate s = s i j s=s_{ij} s = s ij , δ = P i − P j \delta=P_i-P_j δ = P i − P j . Then, conditionally on F i j \mathcal F_{ij} F ij and on the event { s > 0 } \{s>0\} { s > 0 } (whose complement is μ \mu μ -null), the ratio δ / s \delta/s δ / s is uniform on [ − 1 , 1 ] [-1,1] [ − 1 , 1 ] and independent of F i j \mathcal F_{ij} F ij ; consequently
Var i j ( δ ) = s 2 3 , Var i j ( δ 2 ) = 4 s 4 45 , Cov i j ( δ , δ 2 ) = 0. \Var_{ij}(\delta)=\frac{s^2}3,\qquad
\Var_{ij}(\delta^2)=\frac{4s^4}{45},\qquad
\Cov_{ij}(\delta,\delta^2)=0. Var ij ( δ ) = 3 s 2 , Var ij ( δ 2 ) = 45 4 s 4 , Cov ij ( δ , δ 2 ) = 0. Every polynomial f f f of degree at most 2 can be written on the pair fiber, via the substitution p i = s + δ 2 p_i=\tfrac{s+\delta}2 p i = 2 s + δ , p j = s − δ 2 p_j=\tfrac{s-\delta}2 p j = 2 s − δ , uniquely as
f = α f + β f δ + γ f δ 2 , f=\alpha_f+\beta_f\,\delta+\gamma_f\,\delta^2, f = α f + β f δ + γ f δ 2 , where α f , β f , γ f \alpha_f,\beta_f,\gamma_f α f , β f , γ f are polynomials in s s s and ( p ℓ ) ℓ ≠ i , j (p_\ell)_{\ell\ne i,j} ( p ℓ ) ℓ = i , j (hence F i j \mathcal F_{ij} F ij -measurable), with deg β f ≤ 1 \deg\beta_f\le1 deg β f ≤ 1 and γ f \gamma_f γ f constant. For two such polynomials f , g f,g f , g ,
E Cov i j ( f , g ) s 2 = 1 3 E [ β f β g ] + 4 45 E [ γ f γ g s 2 ] , \E\,\frac{\Cov_{ij}(f,g)}{s^2}
=\frac13\,\E\bigl[\beta_f\beta_g\bigr]
+\frac4{45}\,\E\bigl[\gamma_f\gamma_g\,s^2\bigr], E s 2 Cov ij ( f , g ) = 3 1 E [ β f β g ] + 45 4 E [ γ f γ g s 2 ] , a finite quantity. In particular K K K is finite, symmetric, bilinear, positive semidefinite, and well defined on V m , 2 V_{m,2} V m , 2 .
The law μ \mu μ has constant density with respect to ( m − 1 ) (m-1) ( m − 1 ) -dimensional Hausdorff measure on Δ m − 1 \Delta_{m-1} Δ m − 1 . Conditioning on ( P ℓ ) ℓ ≠ i , j (P_\ell)_{\ell\ne i,j} ( P ℓ ) ℓ = i , j fixes s = 1 − ∑ ℓ ≠ i , j P ℓ s=1-\sum_{\ell\ne i,j}P_\ell s = 1 − ∑ ℓ = i , j P ℓ and leaves ( P i , P j ) (P_i,P_j) ( P i , P j ) with a constant conditional density on the segment { ( x , y ) : x , y ≥ 0 , x + y = s } \{(x,y):x,y\ge0,\ x+y=s\} {( x , y ) : x , y ≥ 0 , x + y = s } ; parametrized by P i ∈ [ 0 , s ] P_i\in[0,s] P i ∈ [ 0 , s ] this is the uniform law, so δ / s = 2 P i / s − 1 \delta/s=2P_i/s-1 δ / s = 2 P i / s − 1 is uniform on [ − 1 , 1 ] [-1,1] [ − 1 , 1 ] , with conditional law not depending on F i j \mathcal F_{ij} F ij . The event { s = 0 } \{s=0\} { s = 0 } is the face { P i = P j = 0 } \{P_i=P_j=0\} { P i = P j = 0 } , which is μ \mu μ -null. With V = δ / s V=\delta/s V = δ / s uniform on [ − 1 , 1 ] [-1,1] [ − 1 , 1 ] : E V = E V 3 = 0 \E V=\E V^3=0 E V = E V 3 = 0 , E V 2 = 1 3 \E V^2=\tfrac13 E V 2 = 3 1 , E V 4 = 1 5 \E V^4=\tfrac15 E V 4 = 5 1 , whence Var ( δ ∣ F i j ) = s 2 / 3 \Var(\delta\mid\mathcal F_{ij})=s^2/3 Var ( δ ∣ F ij ) = s 2 /3 , Var ( δ 2 ∣ F i j ) = s 4 ( 1 5 − 1 9 ) = 4 s 4 45 \Var(\delta^2\mid\mathcal F_{ij})=s^4(\tfrac15-\tfrac19)=\tfrac{4s^4}{45} Var ( δ 2 ∣ F ij ) = s 4 ( 5 1 − 9 1 ) = 45 4 s 4 , and Cov ( δ , δ 2 ∣ F i j ) = s 3 E V 3 = 0 \Cov(\delta,\delta^2\mid\mathcal F_{ij})=s^3\,\E V^3=0 Cov ( δ , δ 2 ∣ F ij ) = s 3 E V 3 = 0 , proving (D11.15) .
For (D11.16) , substitute p i = s + δ 2 p_i=\tfrac{s+\delta}2 p i = 2 s + δ , p j = s − δ 2 p_j=\tfrac{s-\delta}2 p j = 2 s − δ into each monomial of f f f :
p i = s 2 + δ 2 , p j = s 2 − δ 2 , p i 2 = s 2 4 + s 2 δ + 1 4 δ 2 , p j 2 = s 2 4 − s 2 δ + 1 4 δ 2 , p i p j = s 2 4 − 1 4 δ 2 , p i p ℓ = p ℓ 2 s + p ℓ 2 δ , p j p ℓ = p ℓ 2 s − p ℓ 2 δ ( ℓ ≠ i , j ) , \begin{gathered}
p_i=\tfrac s2+\tfrac\delta2,\qquad
p_j=\tfrac s2-\tfrac\delta2,\qquad
p_i^2=\tfrac{s^2}4+\tfrac s2\,\delta+\tfrac14\,\delta^2,\qquad
p_j^2=\tfrac{s^2}4-\tfrac s2\,\delta+\tfrac14\,\delta^2,\\
p_ip_j=\tfrac{s^2}4-\tfrac14\,\delta^2,\qquad
p_ip_\ell=\tfrac{p_\ell}2\,s+\tfrac{p_\ell}2\,\delta,\qquad
p_jp_\ell=\tfrac{p_\ell}2\,s-\tfrac{p_\ell}2\,\delta
\quad(\ell\ne i,j),
\end{gathered} p i = 2 s + 2 δ , p j = 2 s − 2 δ , p i 2 = 4 s 2 + 2 s δ + 4 1 δ 2 , p j 2 = 4 s 2 − 2 s δ + 4 1 δ 2 , p i p j = 4 s 2 − 4 1 δ 2 , p i p ℓ = 2 p ℓ s + 2 p ℓ δ , p j p ℓ = 2 p ℓ s − 2 p ℓ δ ( ℓ = i , j ) , while monomials not involving p i , p j p_i,p_j p i , p j contribute to α f \alpha_f α f only. Collecting powers of δ \delta δ gives (D11.16) with the stated degrees; uniqueness holds because ( 1 , δ , δ 2 ) (1,\delta,\delta^2) ( 1 , δ , δ 2 ) are linearly independent functions of δ \delta δ on any fiber with s > 0 s>0 s > 0 . Since α f \alpha_f α f is F i j \mathcal F_{ij} F ij -measurable, bilinearity of conditional covariance and (D11.15) give
Cov i j ( f , g ) = β f β g s 2 3 + γ f γ g 4 s 4 45 , \Cov_{ij}(f,g)
=\beta_f\beta_g\,\frac{s^2}3+\gamma_f\gamma_g\,\frac{4s^4}{45}, Cov ij ( f , g ) = β f β g 3 s 2 + γ f γ g 45 4 s 4 , the two cross terms carrying the vanishing factor Cov i j ( δ , δ 2 ) = 0 \Cov_{ij}(\delta,\delta^2)=0 Cov ij ( δ , δ 2 ) = 0 . Dividing by s 2 s^2 s 2 on { s > 0 } \{s>0\} { s > 0 } and taking expectations proves (D11.17) ; the integrands are polynomials, hence bounded on the simplex, so the expectation is finite. Positive semidefiniteness of K K K is clear from Var i j ≥ 0 \Var_{ij}\ge0 Var ij ≥ 0 . Conditional covariances depend only on the a.e. classes of f , g f,g f , g and vanish when one argument is a.e. constant, so K K K descends to V m , 2 V_{m,2} V m , 2 .
Symmetry structure of the degree-two quotient ¶ Throughout, “module” means a finite-dimensional real representation of S m S_m S m ; all maps are S m S_m S m -equivariant unless stated otherwise. We use the following standard facts about a finite group Γ \Gamma Γ acting on real vector spaces; each has a one-paragraph classical proof, recalled for self-containment.
(Complete reducibility.) Averaging any inner product over Γ \Gamma Γ produces an invariant inner product; the orthogonal complement of a submodule is a submodule; hence every module is a direct sum of irreducibles, every submodule has an invariant complement, and every quotient of a module is isomorphic to a submodule. Consequently, in a short exact sequence of modules the multiplicity of each irreducible is additive.
(Schur.) A nonzero map between irreducibles is an isomorphism; the image of an irreducible submodule under any equivariant map is 0 or isomorphic to it. The E E E -isotypic component W E ( V ) W_E(V) W E ( V ) of a module V V V is the sum of all submodules isomorphic to the irreducible E E E ; equivariant maps send E E E -isotypic parts into E E E -isotypic parts, and V V V is the direct sum of its isotypic components.
(Orbit counting for permutation modules.) If Γ \Gamma Γ acts on finite sets S , T S,T S , T , the space of equivariant linear maps R S → R T \R^S\to\R^T R S → R T has dimension equal to the number of Γ \Gamma Γ -orbits on T × S T\times S T × S : an equivariant matrix is exactly a matrix constant on orbits.
(Multiplicity via Hom.) If E E E is irreducible with End Γ ( E ) = R i d \operatorname{End}_\Gamma(E)=\R\,\mathrm{id} End Γ ( E ) = R id , then for every module V V V the multiplicity of E E E in V V V equals dim Hom Γ ( E , V ) \dim\operatorname{Hom}_\Gamma(E,V) dim Hom Γ ( E , V ) , and W E ( V ) ≅ E ⊗ R k W_E(V)\cong E\otimes\R^{k} W E ( V ) ≅ E ⊗ R k with k k k that multiplicity. (Decompose V V V into irreducibles by (F1); by (F2) and Schur, Hom Γ ( E , ⋅ ) \operatorname{Hom}_\Gamma(E,\cdot) Hom Γ ( E , ⋅ ) of each summand is R \R R for summands ≅ E \cong E ≅ E and 0 otherwise.) In particular the multiplicity of E E E is monotone under submodules and quotients.
(Invariant bilinear forms on an irreducible.) If E E E is irreducible with End Γ ( E ) = R i d \operatorname{End}_\Gamma(E)=\R\,\mathrm{id} End Γ ( E ) = R id , the space of invariant bilinear forms on E E E is one-dimensional, spanned by any fixed invariant inner product J E J_E J E : a form corresponds to an equivariant map E → E ∗ ≅ E E\to E^*\cong E E → E ∗ ≅ E , i.e. to an element of End Γ ( E ) = R \operatorname{End}_\Gamma(E)=\R End Γ ( E ) = R .
Let M = R m M=\R^m M = R m with permuted coordinates and, for m ≥ 3 m\ge3 m ≥ 3 , let N = R ( [ m ] 2 ) N=\R^{\binom{[m]}2} N = R ( 2 [ m ] ) be the permutation module on unordered pairs { i , j } \{i,j\} { i , j } , with basis ( x i j ) i < j (x_{ij})_{i<j} ( x ij ) i < j . Then:
M = t r i v ⊕ s t d M=\mathrm{triv}\oplus\mathrm{std} M = triv ⊕ std , where t r i v = R 1 \mathrm{triv}=\R\one triv = R 1 and s t d = { a : ∑ i a i = 0 } \mathrm{std}=\{a:\sum_ia_i=0\} std = { a : ∑ i a i = 0 } is irreducible of dimension m − 1 m-1 m − 1 with End S m ( s t d ) = R i d \operatorname{End}_{S_m}(\mathrm{std})=\R\,\mathrm{id} End S m ( std ) = R id , and s t d ≇ t r i v \mathrm{std}\not\cong\mathrm{triv} std ≅ triv .
For m ≥ 4 m\ge4 m ≥ 4 , N = t r i v ⊕ s t d ⊕ X N=\mathrm{triv}\oplus\mathrm{std}\oplus\mathrm X N = triv ⊕ std ⊕ X with each summand of multiplicity one, where X \mathrm X X is irreducible of dimension m ( m − 3 ) / 2 m(m-3)/2 m ( m − 3 ) /2 , satisfies End S m ( X ) = R i d \operatorname{End}_{S_m}(\mathrm X)=\R\,\mathrm{id} End S m ( X ) = R id , and X ≇ t r i v , s t d \mathrm X\not\cong\mathrm{triv},\mathrm{std} X ≅ triv , std . For m = 3 m=3 m = 3 , N = t r i v ⊕ s t d N=\mathrm{triv}\oplus\mathrm{std} N = triv ⊕ std and the summand X \mathrm X X is absent.
(1) S m S_m S m has two orbits on [ m ] 2 [m]^2 [ m ] 2 (diagonal, off-diagonal), so dim End ( M ) = 2 \dim\operatorname{End}(M)=2 dim End ( M ) = 2 by (F3). Also M S m = R 1 M^{S_m}=\R\one M S m = R 1 is one-dimensional, so t r i v \mathrm{triv} triv has multiplicity one; let C = 1 ⊥ C=\one^\perp C = 1 ⊥ be its invariant complement. Then C S m = 0 C^{S_m}=0 C S m = 0 , so Hom ( t r i v , C ) = 0 \operatorname{Hom}(\mathrm{triv},C)=0 Hom ( triv , C ) = 0 and 2 = dim End ( M ) = dim End ( t r i v ) + dim End ( C ) = 1 + dim End ( C ) 2=\dim\operatorname{End}(M) =\dim\operatorname{End}(\mathrm{triv})+\dim\operatorname{End}(C) =1+\dim\operatorname{End}(C) 2 = dim End ( M ) = dim End ( triv ) + dim End ( C ) = 1 + dim End ( C ) . A decomposable module has endomorphism algebra of dimension at least 2 (the two projections), so End ( C ) = R i d \operatorname{End}(C)=\R\,\mathrm{id} End ( C ) = R id forces C C C irreducible. Finally C ≇ t r i v C\not\cong\mathrm{triv} C ≅ triv because C S m = 0 C^{S_m}=0 C S m = 0 . Set s t d = C \mathrm{std}=C std = C .
(2) Let m ≥ 4 m\ge4 m ≥ 4 . The orbits of S m S_m S m on (ordered) pairs of 2-subsets are classified by ∣ A ∩ B ∣ ∈ { 2 , 1 , 0 } \abs{A\cap B}\in\{2,1,0\} ∣ A ∩ B ∣ ∈ { 2 , 1 , 0 } , all realized, so dim End ( N ) = 3 \dim\operatorname{End}(N)=3 dim End ( N ) = 3 . The orbits on [ m ] × ( [ m ] 2 ) [m]\times\binom{[m]}2 [ m ] × ( 2 [ m ] ) are classified by i ∈ A i\in A i ∈ A versus i ∉ A i\notin A i ∈ / A , so dim Hom ( M , N ) = 2 \dim\operatorname{Hom}(M,N)=2 dim Hom ( M , N ) = 2 . As N S m N^{S_m} N S m is one-dimensional (one orbit of 2-subsets), t r i v \mathrm{triv} triv has multiplicity one in N N N and dim Hom ( s t d , N ) = dim Hom ( M , N ) − dim Hom ( t r i v , N ) = 2 − 1 = 1 \dim\operatorname{Hom}(\mathrm{std},N) =\dim\operatorname{Hom}(M,N)-\dim\operatorname{Hom}(\mathrm{triv},N)=2-1=1 dim Hom ( std , N ) = dim Hom ( M , N ) − dim Hom ( triv , N ) = 2 − 1 = 1 , so by (F4) s t d \mathrm{std} std has multiplicity exactly one. Decompose N = t r i v ⊕ S ′ ⊕ X N=\mathrm{triv}\oplus S'\oplus \mathrm X N = triv ⊕ S ′ ⊕ X with S ′ ≅ s t d S'\cong\mathrm{std} S ′ ≅ std and X \mathrm X X the sum of the remaining irreducible summands, which contains no copy of t r i v \mathrm{triv} triv or s t d \mathrm{std} std . Then cross-Homs between the three summands vanish and 3 = dim End ( N ) = 1 + 1 + dim End ( X ) 3=\dim\operatorname{End}(N)=1+1+\dim\operatorname{End}(\mathrm X) 3 = dim End ( N ) = 1 + 1 + dim End ( X ) , so as in (1) X \mathrm X X is irreducible with End ( X ) = R i d \operatorname{End}(\mathrm X)=\R\,\mathrm{id} End ( X ) = R id , and X ≇ t r i v , s t d \mathrm X\not\cong\mathrm{triv},\mathrm{std} X ≅ triv , std (otherwise those multiplicities would exceed one). Its dimension is ( m 2 ) − 1 − ( m − 1 ) = m ( m − 3 ) / 2 \binom m2-1-(m-1)=m(m-3)/2 ( 2 m ) − 1 − ( m − 1 ) = m ( m − 3 ) /2 . For m = 3 m=3 m = 3 there is no orbit with ∣ A ∩ B ∣ = 0 \abs{A\cap B}=0 ∣ A ∩ B ∣ = 0 , so dim End ( N ) = 2 \dim\operatorname{End}(N)=2 dim End ( N ) = 2 and the same argument yields N = t r i v ⊕ s t d N=\mathrm{triv}\oplus\mathrm{std} N = triv ⊕ std (dimensions: 3 = 1 + 2 3=1+2 3 = 1 + 2 ).
For m ≥ 3 m\ge3 m ≥ 3 , as S m S_m S m -modules,
V m , 2 ≅ t r i v ⊕ s t d ⊗ R 2 ⊕ X , dim V m , 2 = ( m − 1 ) ( m + 2 ) 2 , V_{m,2}\;\cong\;
\mathrm{triv}\ \oplus\ \mathrm{std}\otimes\R^2\ \oplus\ \mathrm X,
\qquad
\dim V_{m,2}=\frac{(m-1)(m+2)}2, V m , 2 ≅ triv ⊕ std ⊗ R 2 ⊕ X , dim V m , 2 = 2 ( m − 1 ) ( m + 2 ) , where the X \mathrm X X -summand is absent when m = 3 m=3 m = 3 . Moreover:
the t r i v \mathrm{triv} triv -isotypic component is W t r i v = R [ f 0 ] W_{\rm triv}=\R\,[f_0] W triv = R [ f 0 ] with f 0 = ∑ k p k 2 f_0=\sum_kp_k^2 f 0 = ∑ k p k 2 , and [ f 0 ] ≠ 0 [f_0]\ne0 [ f 0 ] = 0 ;
the classes L = [ p 1 − p 2 ] L=[p_1-p_2] L = [ p 1 − p 2 ] and Q = [ p 1 2 − p 2 2 ] Q=[p_1^2-p_2^2] Q = [ p 1 2 − p 2 2 ] are nonzero, linearly independent, and lie in the s t d \mathrm{std} std -isotypic component W s t d W_{\rm std} W std ; they are the images of the common seed vector v 0 = e 1 − e 2 ∈ s t d v_0=e_1-e_2\in\mathrm{std} v 0 = e 1 − e 2 ∈ std under the two equivariant maps T 1 : a ↦ [ ∑ i a i p i ] T_1:a\mapsto[\textstyle\sum_ia_ip_i] T 1 : a ↦ [ ∑ i a i p i ] and T 2 : a ↦ [ ∑ i a i p i 2 ] T_2:a\mapsto[\textstyle\sum_ia_ip_i^2] T 2 : a ↦ [ ∑ i a i p i 2 ] , whose images span W s t d W_{\rm std} W std ;
for m ≥ 4 m\ge4 m ≥ 4 , the class F = [ ( p 1 − p 3 ) ( p 2 − p 4 ) ] F=[(p_1-p_3)(p_2-p_4)] F = [( p 1 − p 3 ) ( p 2 − p 4 )] is nonzero and lies in the X \mathrm X X -isotypic component W X W_{\mathrm X} W X , which it generates.
Kernel of the quotient map. Define the equivariant surjection Ψ : W p o l y → V m , 2 \Psi:W_{\rm poly}\to V_{m,2} Ψ : W poly → V m , 2 , f ↦ [ f ] f\mapsto[f] f ↦ [ f ] . We claim
ker Ψ = { b 0 ∑ i p i + ( ∑ i p i − 1 ) ∑ i b i p i : b 0 ∈ R , b ∈ R m } ≅ t r i v ⊕ M ≅ 2 t r i v ⊕ s t d . \ker\Psi
=\Bigl\{\,b_0\textstyle\sum_ip_i
+\bigl(\textstyle\sum_ip_i-1\bigr)\textstyle\sum_ib_ip_i
\;:\;b_0\in\R,\ b\in\R^m\Bigr\}
\;\cong\;\mathrm{triv}\oplus M
\;\cong\;2\,\mathrm{triv}\oplus\mathrm{std}. ker Ψ = { b 0 ∑ i p i + ( ∑ i p i − 1 ) ∑ i b i p i : b 0 ∈ R , b ∈ R m } ≅ triv ⊕ M ≅ 2 triv ⊕ std . Indeed f ∈ ker Ψ f\in\ker\Psi f ∈ ker Ψ means f = c f=c f = c μ \mu μ -a.e. for some c ∈ R c\in\R c ∈ R . The support Δ m − 1 \Delta_{m-1} Δ m − 1 has nonempty relative interior in the hyperplane H = { ∑ i p i = 1 } H=\{\sum_ip_i=1\} H = { ∑ i p i = 1 } , and a polynomial vanishing on a relatively open subset of an affine subspace vanishes on the whole subspace; hence f − c f-c f − c vanishes on H H H . Choosing affine coordinates in which t = ∑ i p i − 1 t=\sum_ip_i-1 t = ∑ i p i − 1 is one coordinate and dividing by t t t (polynomial division in t t t , degree bookkeeping: deg ≤ 2 \deg\le2 deg ≤ 2 ), we get f = c + ( ∑ i p i − 1 ) ℓ f=c+(\sum_ip_i-1)\ell f = c + ( ∑ i p i − 1 ) ℓ with ℓ \ell ℓ affine, say ℓ = b 0 + ∑ i b i p i \ell=b_0+\sum_ib_ip_i ℓ = b 0 + ∑ i b i p i . Since f f f has zero constant term, c = b 0 c=b_0 c = b 0 , which yields exactly the displayed set; conversely every element of that set is μ \mu μ -a.e. constant (equal to b 0 b_0 b 0 ). The parametrization ( b 0 , b ) ↦ f (b_0,b)\mapsto f ( b 0 , b ) ↦ f is linear, injective (compare first the quadratic homogeneous part ( ∑ i p i ) ( ∑ i b i p i ) (\sum_ip_i)(\sum_ib_ip_i) ( ∑ i p i ) ( ∑ i b i p i ) , which vanishes only if b = 0 b=0 b = 0 since the polynomial ring is a domain; then b 0 ∑ p i = 0 b_0\sum p_i=0 b 0 ∑ p i = 0 forces b 0 = 0 b_0=0 b 0 = 0 ), and equivariant for the action fixing b 0 b_0 b 0 and permuting b b b . This proves (D11.21) .
Multiplicities. The monomial families ( p i ) (p_i) ( p i ) , ( p i 2 ) (p_i^2) ( p i 2 ) , ( p i p j ) i < j (p_ip_j)_{i<j} ( p i p j ) i < j are linearly independent in the polynomial ring and are permuted by S m S_m S m exactly as the bases of M M M , M M M , N N N ; hence W p o l y ≅ M ⊕ M ⊕ N W_{\rm poly}\cong M\oplus M\oplus N W poly ≅ M ⊕ M ⊕ N , whose isotypic multiplicities are (by Lemma D11.3 ): t r i v \mathrm{triv} triv : 3, s t d \mathrm{std} std : 3, X \mathrm X X : 1 (for m ≥ 4 m\ge4 m ≥ 4 ; X \mathrm X X absent at m = 3 m=3 m = 3 ). By (F1) applied to 0 → ker Ψ → W p o l y → V m , 2 → 0 0\to\ker\Psi\to W_{\rm poly}\to V_{m,2}\to0 0 → ker Ψ → W poly → V m , 2 → 0 and (D11.21) , the multiplicities in V m , 2 V_{m,2} V m , 2 are t r i v \mathrm{triv} triv : 3 − 2 = 1 3-2=1 3 − 2 = 1 , s t d \mathrm{std} std : 3 − 1 = 2 3-1=2 3 − 1 = 2 , X \mathrm X X : 1 − 0 = 1 1-0=1 1 − 0 = 1 , and no other irreducible occurs. This is (D11.20) ; the dimension is 1 + 2 ( m − 1 ) + m ( m − 3 ) / 2 = ( m − 1 ) ( m + 2 ) / 2 1+2(m-1)+m(m-3)/2=(m-1)(m+2)/2 1 + 2 ( m − 1 ) + m ( m − 3 ) /2 = ( m − 1 ) ( m + 2 ) /2 (also valid at m = 3 m=3 m = 3 ).
(1). [ f 0 ] [f_0] [ f 0 ] is S m S_m S m -fixed. It is nonzero: if f 0 ∈ ker Ψ f_0\in\ker\Psi f 0 ∈ ker Ψ , comparing quadratic homogeneous parts in (D11.21) gives ∑ i p i 2 = ( ∑ i p i ) ( ∑ i b i p i ) \sum_ip_i^2=(\sum_ip_i)(\sum_ib_ip_i) ∑ i p i 2 = ( ∑ i p i ) ( ∑ i b i p i ) ; the coefficient of p i 2 p_i^2 p i 2 forces b i = 1 b_i=1 b i = 1 for all i i i , but then the coefficient of p 1 p 2 p_1p_2 p 1 p 2 on the right is 2 ≠ 0 2\ne0 2 = 0 , a contradiction. Since the t r i v \mathrm{triv} triv -multiplicity is one, W t r i v = R [ f 0 ] W_{\rm triv}=\R[f_0] W triv = R [ f 0 ] .
(2). T 1 , T 2 T_1,T_2 T 1 , T 2 are restrictions to s t d ⊂ M \mathrm{std}\subset M std ⊂ M of the equivariant maps a ↦ [ ∑ a i p i ] a\mapsto[\sum a_ip_i] a ↦ [ ∑ a i p i ] , a ↦ [ ∑ a i p i 2 ] a\mapsto[\sum a_ip_i^2] a ↦ [ ∑ a i p i 2 ] , so their images lie in W s t d W_{\rm std} W std by (F2), and L = T 1 v 0 L=T_1v_0 L = T 1 v 0 , Q = T 2 v 0 Q=T_2v_0 Q = T 2 v 0 . Linear independence of L , Q L,Q L , Q in V m , 2 V_{m,2} V m , 2 : suppose a L + b Q ∈ ker Ψ aL+bQ\in\ker\Psi a L + b Q ∈ ker Ψ , i.e. a ( p 1 − p 2 ) + b ( p 1 2 − p 2 2 ) = b 0 ∑ i p i + ( ∑ i p i − 1 ) ∑ i b i p i a(p_1-p_2)+b(p_1^2-p_2^2) =b_0\sum_ip_i+(\sum_ip_i-1)\sum_ib_ip_i a ( p 1 − p 2 ) + b ( p 1 2 − p 2 2 ) = b 0 ∑ i p i + ( ∑ i p i − 1 ) ∑ i b i p i . Quadratic parts: b ( p 1 2 − p 2 2 ) = ( ∑ i p i ) ( ∑ i b i p i ) b(p_1^2-p_2^2)=(\sum_ip_i)(\sum_ib_ip_i) b ( p 1 2 − p 2 2 ) = ( ∑ i p i ) ( ∑ i b i p i ) ; the p i 2 p_i^2 p i 2 coefficients give b 1 = b b_1=b b 1 = b , b 2 = − b b_2=-b b 2 = − b , b ℓ = 0 b_\ell=0 b ℓ = 0 (ℓ ≥ 3 \ell\ge3 ℓ ≥ 3 ), and then the p 1 p 3 p_1p_3 p 1 p 3 coefficient (using m ≥ 3 m\ge3 m ≥ 3 ) gives 0 = b 1 + b 3 = b 0=b_1+b_3=b 0 = b 1 + b 3 = b , so b = 0 b=0 b = 0 and b ≡ 0 b\equiv0 b ≡ 0 . The linear part then reads a ( p 1 − p 2 ) = b 0 ∑ i p i a(p_1-p_2)=b_0\sum_ip_i a ( p 1 − p 2 ) = b 0 ∑ i p i , forcing a = b 0 = − a a=b_0=-a a = b 0 = − a , i.e.\ a = 0 a=0 a = 0 . In particular L , Q ≠ 0 L,Q\ne0 L , Q = 0 , so T 1 , T 2 ≠ 0 T_1,T_2\ne0 T 1 , T 2 = 0 and, s t d \mathrm{std} std being irreducible, T 1 ( s t d ) ≅ T 2 ( s t d ) ≅ s t d T_1(\mathrm{std})\cong T_2(\mathrm{std})\cong\mathrm{std} T 1 ( std ) ≅ T 2 ( std ) ≅ std . The two image submodules are distinct: if T 1 ( s t d ) = T 2 ( s t d ) = : U T_1(\mathrm{std})=T_2(\mathrm{std})=:U T 1 ( std ) = T 2 ( std ) =: U , then T 1 , T 2 ∈ Hom ( s t d , U ) T_1,T_2\in\operatorname{Hom}(\mathrm{std},U) T 1 , T 2 ∈ Hom ( std , U ) , a one-dimensional space by (F4)–(F5) (as U ≅ s t d U\cong\mathrm{std} U ≅ std ), so T 2 = c T 1 T_2=cT_1 T 2 = c T 1 and Q = c L Q=cL Q = c L , contradicting independence. Distinct irreducible submodules intersect in 0, so T 1 ( s t d ) ⊕ T 2 ( s t d ) ⊆ W s t d T_1(\mathrm{std})\oplus T_2(\mathrm{std})\subseteq W_{\rm std} T 1 ( std ) ⊕ T 2 ( std ) ⊆ W std has dimension 2 ( m − 1 ) = dim W s t d 2(m-1)=\dim W_{\rm std} 2 ( m − 1 ) = dim W std ; hence the images span W s t d W_{\rm std} W std .
(3). Let m ≥ 4 m\ge4 m ≥ 4 and let ψ : N → V m , 2 \psi:N\to V_{m,2} ψ : N → V m , 2 be the equivariant map x i j ↦ [ p i p j ] x_{ij}\mapsto[p_ip_j] x ij ↦ [ p i p j ] . Consider
v = x 12 − x 23 − x 14 + x 34 ∈ N , ψ ( v ) = [ p 1 p 2 − p 2 p 3 − p 1 p 4 + p 3 p 4 ] = [ ( p 1 − p 3 ) ( p 2 − p 4 ) ] = F . v=x_{12}-x_{23}-x_{14}+x_{34}\in N,
\qquad
\psi(v)=[p_1p_2-p_2p_3-p_1p_4+p_3p_4]=[(p_1-p_3)(p_2-p_4)]=F. v = x 12 − x 23 − x 14 + x 34 ∈ N , ψ ( v ) = [ p 1 p 2 − p 2 p 3 − p 1 p 4 + p 3 p 4 ] = [( p 1 − p 3 ) ( p 2 − p 4 )] = F . We check v ∈ W X ( N ) v\in W_{\mathrm X}(N) v ∈ W X ( N ) . With the standard (invariant) inner product on N N N , the isotypic components of N N N are mutually orthogonal. The t r i v \mathrm{triv} triv -component is spanned by ∑ i < j x i j \sum_{i<j}x_{ij} ∑ i < j x ij , and the s t d \mathrm{std} std -component lies in the image of the equivariant map A : M → N A:M\to N A : M → N , e k ↦ u k : = ∑ ℓ ≠ k x k ℓ e_k\mapsto u_k:=\sum_{\ell\ne k}x_{k\ell} e k ↦ u k := ∑ ℓ = k x k ℓ (indeed A ( s t d ) ≠ 0 A(\mathrm{std})\ne0 A ( std ) = 0 because u 1 − u 2 u_1-u_2 u 1 − u 2 has coefficient 1 on x 13 x_{13} x 13 , and the s t d \mathrm{std} std -multiplicity of N N N is one, so W s t d ( N ) = A ( s t d ) W_{\rm std}(N)=A(\mathrm{std}) W std ( N ) = A ( std ) ). Now ⟨ v , ∑ i < j x i j ⟩ = 1 − 1 − 1 + 1 = 0 \langle v,\sum_{i<j}x_{ij}\rangle=1-1-1+1=0 ⟨ v , ∑ i < j x ij ⟩ = 1 − 1 − 1 + 1 = 0 and, for every k k k , ⟨ v , u k ⟩ = 0 \langle v,u_k\rangle=0 ⟨ v , u k ⟩ = 0 : for k = 1 k=1 k = 1 the pairs of v v v containing 1 are x 12 x_{12} x 12 (+ + + ) and x 14 x_{14} x 14 (− - − ); for k = 2 k=2 k = 2 : x 12 x_{12} x 12 (+ + + ), x 23 x_{23} x 23 (− - − ); for k = 3 k=3 k = 3 : x 23 x_{23} x 23 (− - − ), x 34 x_{34} x 34 (+ + + ); for k = 4 k=4 k = 4 : x 14 x_{14} x 14 (− - − ), x 34 x_{34} x 34 (+ + + ); for k ≥ 5 k\ge5 k ≥ 5 : none. Hence v ⊥ W t r i v ( N ) ⊕ W s t d ( N ) v\perp W_{\rm triv}(N)\oplus W_{\rm std}(N) v ⊥ W triv ( N ) ⊕ W std ( N ) , i.e.\ v ∈ W X ( N ) v\in W_{\mathrm X}(N) v ∈ W X ( N ) . By (F2), F = ψ ( v ) ∈ W X ( V m , 2 ) F=\psi(v)\in W_{\mathrm X}(V_{m,2}) F = ψ ( v ) ∈ W X ( V m , 2 ) . Finally F ≠ 0 F\ne0 F = 0 : if ( p 1 − p 3 ) ( p 2 − p 4 ) ∈ ker Ψ (p_1-p_3)(p_2-p_4)\in\ker\Psi ( p 1 − p 3 ) ( p 2 − p 4 ) ∈ ker Ψ , comparing quadratic parts with (D11.21) gives ( p 1 − p 3 ) ( p 2 − p 4 ) = ( ∑ i p i ) ( ∑ i b i p i ) (p_1-p_3)(p_2-p_4)=(\sum_ip_i)(\sum_ib_ip_i) ( p 1 − p 3 ) ( p 2 − p 4 ) = ( ∑ i p i ) ( ∑ i b i p i ) ; the left side has no p i 2 p_i^2 p i 2 terms, so all b i = 0 b_i=0 b i = 0 , but the left side has p 1 p 2 p_1p_2 p 1 p 2 -coefficient 1, a contradiction. Since W X W_{\mathrm X} W X has multiplicity one and ψ ∣ W X ( N ) \psi|_{W_{\mathrm X}(N)} ψ ∣ W X ( N ) is injective (its restriction to the irreducible W X ( N ) W_{\mathrm X}(N) W X ( N ) is nonzero), F F F generates W X W_{\mathrm X} W X as a module.
Let V V V be a module with invariant symmetric bilinear forms B B B (arbitrary) and G G G (positive definite), and let V = ⨁ E W E V=\bigoplus_EW_E V = ⨁ E W E be its isotypic decomposition over pairwise non-isomorphic irreducibles E E E with End ( E ) = R i d \operatorname{End}(E)=\R\,\mathrm{id} End ( E ) = R id . Then:
B ( W E , W E ′ ) = 0 B(W_E,W_{E'})=0 B ( W E , W E ′ ) = 0 for E ≇ E ′ E\not\cong E' E ≅ E ′ ; hence B B B is positive semidefinite (resp. definite) on V V V if and only if it is so on each W E W_E W E .
Suppose W E W_E W E is spanned by the images of equivariant maps T 1 , … , T k : E → V T_1,\dots,T_k:E\to V T 1 , … , T k : E → V that are linearly independent in Hom S m ( E , V ) \operatorname{Hom}_{S_m}(E,V) Hom S m ( E , V ) , and fix 0 ≠ v 0 ∈ E 0\ne v_0\in E 0 = v 0 ∈ E . Then the map Φ : E ⊗ R k → W E \Phi:E\otimes\R^k\to W_E Φ : E ⊗ R k → W E , u ⊗ ε a ↦ T a u u\otimes\varepsilon_a\mapsto T_au u ⊗ ε a ↦ T a u , is an isomorphism, and there is a symmetric k × k k\times k k × k matrix B ^ \widehat B B with
where J E J_E J E is a fixed invariant inner product on E E E . Consequently B B B is positive semidefinite (resp. definite) on W E W_E W E if and only if the k × k k\times k k × k Gram matrix ( B ( T a v 0 , T b v 0 ) ) a , b = J E ( v 0 , v 0 ) B ^ \bigl(B(T_av_0,T_bv_0)\bigr)_{a,b}=J_E(v_0,v_0)\,\widehat B ( B ( T a v 0 , T b v 0 ) ) a , b = J E ( v 0 , v 0 ) B is positive semidefinite (resp. definite).
(1) The invariant form B B B and an invariant inner product on W E ′ W_{E'} W E ′ induce an equivariant map W E → W E ′ ∗ ≅ W E ′ W_E\to W_{E'}^*\cong W_{E'} W E → W E ′ ∗ ≅ W E ′ . By (F2) and Schur, every equivariant map from an E E E -isotypic to an E ′ E' E ′ -isotypic module is zero when E ≇ E ′ E\not\cong E' E ≅ E ′ . Hence B ( W E , W E ′ ) = 0 B(W_E,W_{E'})=0 B ( W E , W E ′ ) = 0 , and B B B decomposes as the orthogonal (with respect to the decomposition) sum of its restrictions.
(2) Φ \Phi Φ is equivariant and surjective (images span), and dim ( E ⊗ R k ) = k dim E = dim W E \dim(E\otimes\R^k)=k\dim E=\dim W_E dim ( E ⊗ R k ) = k dim E = dim W E because the multiplicity of E E E in W E W_E W E equals dim Hom ( E , W E ) ≥ k \dim\operatorname{Hom}(E,W_E)\ge k dim Hom ( E , W E ) ≥ k by linear independence, while surjectivity gives ≤ k \le k ≤ k ; so Φ \Phi Φ is an isomorphism. For fixed a , b a,b a , b , the bilinear form ( u , u ′ ) ↦ B ( T a u , T b u ′ ) (u,u')\mapsto B(T_au,T_bu') ( u , u ′ ) ↦ B ( T a u , T b u ′ ) on E E E is invariant, hence by (F5) equals B ^ a b J E ( u , u ′ ) \widehat B_{ab}J_E(u,u') B ab J E ( u , u ′ ) for a unique scalar B ^ a b \widehat B_{ab} B ab ; symmetry of B B B and of J E J_E J E gives B ^ a b = B ^ b a \widehat B_{ab}=\widehat B_{ba} B ab = B ba . Now for f = Φ ( ∑ α u α ⊗ s α ) f=\Phi\bigl(\sum_\alpha u^\alpha\otimes s_\alpha\bigr) f = Φ ( ∑ α u α ⊗ s α ) with ( u α ) α (u^\alpha)_\alpha ( u α ) α a J E J_E J E -orthonormal basis of E E E and s α ∈ R k s_\alpha\in\R^k s α ∈ R k ,
B ( f , f ) = ∑ α , γ ∑ a , b s α a s γ b B ( T a u α , T b u γ ) = ∑ α , γ J E ( u α , u γ ) s α T B ^ s γ = ∑ α s α T B ^ s α . B(f,f)
=\sum_{\alpha,\gamma}\sum_{a,b}
s_\alpha^a s_\gamma^b\,B(T_au^\alpha,T_bu^\gamma)
=\sum_{\alpha,\gamma}J_E(u^\alpha,u^\gamma)\,s_\alpha^T\widehat B\,s_\gamma
=\sum_\alpha s_\alpha^T\widehat B\,s_\alpha. B ( f , f ) = α , γ ∑ a , b ∑ s α a s γ b B ( T a u α , T b u γ ) = α , γ ∑ J E ( u α , u γ ) s α T B s γ = α ∑ s α T B s α . Since every element of W E W_E W E is such an f f f and the vectors ( s α ) α (s_\alpha)_\alpha ( s α ) α are arbitrary, B ≥ 0 B\ge0 B ≥ 0 (resp. > 0 >0 > 0 ) on W E W_E W E iff B ^ ⪰ 0 \widehat B\succeq0 B ⪰ 0 (resp. ≻ 0 \succ0 ≻ 0 ), iff the Gram matrix J E ( v 0 , v 0 ) B ^ J_E(v_0,v_0)\widehat B J E ( v 0 , v 0 ) B is so (J E ( v 0 , v 0 ) > 0 J_E(v_0,v_0)>0 J E ( v 0 , v 0 ) > 0 ).
Sector computations ¶ Throughout this subsection E i j ( f , g ) E_{ij}(f,g) E ij ( f , g ) denotes the pair energy (D11.17) and we tabulate the coefficients ( β , γ ) (\beta,\gamma) ( β , γ ) of Lemma D11.2 for each seed and each pair type; pairs not listed have β = γ = 0 \beta=\gamma=0 β = γ = 0 . Recall (D11.14) and D 2 = m ( m + 1 ) D_2=m(m+1) D 2 = m ( m + 1 ) , D 3 = D 2 ( m + 2 ) D_3=D_2(m+2) D 3 = D 2 ( m + 2 ) , D 4 = D 3 ( m + 3 ) D_4=D_3(m+3) D 4 = D 3 ( m + 3 ) .
With f 0 = ∑ k p k 2 f_0=\sum_kp_k^2 f 0 = ∑ k p k 2 ,
K ( f 0 , f 0 ) = 4 ( m − 1 ) 5 m 2 ( m + 1 ) 2 , G ( f 0 , f 0 ) = 4 ( m − 1 ) ( m + 1 ) 2 ( m + 2 ) ( m + 3 ) , K ( f 0 , f 0 ) G ( f 0 , f 0 ) = ( m + 2 ) ( m + 3 ) 5 m 2 . K(f_0,f_0)=\frac{4(m-1)}{5m^2(m+1)^2},
\qquad
G(f_0,f_0)=\frac{4(m-1)}{(m+1)^2(m+2)(m+3)},
\qquad
\frac{K(f_0,f_0)}{G(f_0,f_0)}=\frac{(m+2)(m+3)}{5m^2}. K ( f 0 , f 0 ) = 5 m 2 ( m + 1 ) 2 4 ( m − 1 ) , G ( f 0 , f 0 ) = ( m + 1 ) 2 ( m + 2 ) ( m + 3 ) 4 ( m − 1 ) , G ( f 0 , f 0 ) K ( f 0 , f 0 ) = 5 m 2 ( m + 2 ) ( m + 3 ) . Moreover [ f 0 ] = 1 m ( m + 1 ) [ ∣ X ∣ 2 − ( m − 1 ) ] [f_0]=\tfrac1{m(m+1)}\,[\abs X^2-(m-1)] [ f 0 ] = m ( m + 1 ) 1 [ ∣ X ∣ 2 − ( m − 1 )] in V m , 2 V_{m,2} V m , 2 .
For every pair ( i , j ) (i,j) ( i , j ) , by (D11.18) , p i 2 + p j 2 = s 2 2 + δ 2 2 p_i^2+p_j^2=\tfrac{s^2}2+\tfrac{\delta^2}2 p i 2 + p j 2 = 2 s 2 + 2 δ 2 , so ( β , γ ) = ( 0 , 1 2 ) (\beta,\gamma)=(0,\tfrac12) ( β , γ ) = ( 0 , 2 1 ) and, by (D11.17) and (D11.14) , E i j ( f 0 , f 0 ) = 4 45 ⋅ 1 4 E s 2 = 1 45 ⋅ 6 D 2 = 2 15 D 2 E_{ij}(f_0,f_0)=\tfrac4{45}\cdot\tfrac14\,\E s^2=\tfrac1{45}\cdot\tfrac6{D_2} =\tfrac2{15D_2} E ij ( f 0 , f 0 ) = 45 4 ⋅ 4 1 E s 2 = 45 1 ⋅ D 2 6 = 15 D 2 2 . Summing over the ( m 2 ) \binom m2 ( 2 m ) pairs and inserting the prefactor of (D11.2) ,
K ( f 0 , f 0 ) = 12 m 2 ( m + 1 ) ⋅ m ( m − 1 ) 2 ⋅ 2 15 m ( m + 1 ) = 4 ( m − 1 ) 5 m 2 ( m + 1 ) 2 . K(f_0,f_0)
=\frac{12}{m^2(m+1)}\cdot\frac{m(m-1)}2\cdot\frac2{15\,m(m+1)}
=\frac{4(m-1)}{5m^2(m+1)^2}. K ( f 0 , f 0 ) = m 2 ( m + 1 ) 12 ⋅ 2 m ( m − 1 ) ⋅ 15 m ( m + 1 ) 2 = 5 m 2 ( m + 1 ) 2 4 ( m − 1 ) . For the variance, Lemma D11.1 gives E f 0 = m ⋅ 2 D 2 = 2 m + 1 \E f_0=m\cdot\tfrac2{D_2}=\tfrac2{m+1} E f 0 = m ⋅ D 2 2 = m + 1 2 and E f 0 2 = m E P 1 4 + m ( m − 1 ) E P 1 2 P 2 2 = 24 m + 4 m ( m − 1 ) D 4 = 4 m ( m + 5 ) D 4 \E f_0^2=m\,\E P_1^4+m(m-1)\,\E P_1^2P_2^2 =\tfrac{24m+4m(m-1)}{D_4}=\tfrac{4m(m+5)}{D_4} E f 0 2 = m E P 1 4 + m ( m − 1 ) E P 1 2 P 2 2 = D 4 24 m + 4 m ( m − 1 ) = D 4 4 m ( m + 5 ) , so
G ( f 0 , f 0 ) = 4 ( m + 5 ) ( m + 1 ) ( m + 2 ) ( m + 3 ) − 4 ( m + 1 ) 2 = 4 [ ( m + 5 ) ( m + 1 ) − ( m + 2 ) ( m + 3 ) ] ( m + 1 ) 2 ( m + 2 ) ( m + 3 ) = 4 ( m − 1 ) ( m + 1 ) 2 ( m + 2 ) ( m + 3 ) , G(f_0,f_0)
=\frac{4(m+5)}{(m+1)(m+2)(m+3)}-\frac4{(m+1)^2}
=\frac{4\bigl[(m+5)(m+1)-(m+2)(m+3)\bigr]}{(m+1)^2(m+2)(m+3)}
=\frac{4(m-1)}{(m+1)^2(m+2)(m+3)}, G ( f 0 , f 0 ) = ( m + 1 ) ( m + 2 ) ( m + 3 ) 4 ( m + 5 ) − ( m + 1 ) 2 4 = ( m + 1 ) 2 ( m + 2 ) ( m + 3 ) 4 [ ( m + 5 ) ( m + 1 ) − ( m + 2 ) ( m + 3 ) ] = ( m + 1 ) 2 ( m + 2 ) ( m + 3 ) 4 ( m − 1 ) , using ( m + 5 ) ( m + 1 ) − ( m + 2 ) ( m + 3 ) = m − 1 (m+5)(m+1)-(m+2)(m+3)=m-1 ( m + 5 ) ( m + 1 ) − ( m + 2 ) ( m + 3 ) = m − 1 . The quotient is ( m + 2 ) ( m + 3 ) / ( 5 m 2 ) (m+2)(m+3)/(5m^2) ( m + 2 ) ( m + 3 ) / ( 5 m 2 ) . Finally ∣ X ∣ 2 = m ( m + 1 ) ∑ i ( p i − 1 m ) 2 = m ( m + 1 ) ( f 0 − 1 m ) \abs X^2=m(m+1)\sum_i(p_i-\tfrac1m)^2=m(m+1)\bigl(f_0-\tfrac1m\bigr) ∣ X ∣ 2 = m ( m + 1 ) ∑ i ( p i − m 1 ) 2 = m ( m + 1 ) ( f 0 − m 1 ) , so [ ∣ X ∣ 2 − ( m − 1 ) ] = m ( m + 1 ) [ f 0 ] [\abs X^2-(m-1)]=m(m+1)[f_0] [ ∣ X ∣ 2 − ( m − 1 )] = m ( m + 1 ) [ f 0 ] .
Energies. The ( β , γ ) (\beta,\gamma) ( β , γ ) tables from (D11.18) , with j j j always denoting an index ≥ 3 \ge3 ≥ 3 distinct from 1 , 2 1,2 1 , 2 :
pair β L γ L β Q γ Q ( 1 , 2 ) 1 0 s 0 ( 1 , j ) 1 2 0 s 2 1 4 ( 2 , j ) − 1 2 0 − s 2 − 1 4 \begin{array}{l|cc|cc}
\text{pair} & \beta_L & \gamma_L & \beta_Q & \gamma_Q\\\hline
(1,2) & 1 & 0 & s & 0\\
(1,j) & \tfrac12 & 0 & \tfrac s2 & \tfrac14\\
(2,j) & -\tfrac12 & 0 & -\tfrac s2 & -\tfrac14
\end{array} pair ( 1 , 2 ) ( 1 , j ) ( 2 , j ) β L 1 2 1 − 2 1 γ L 0 0 0 β Q s 2 s − 2 s γ Q 0 4 1 − 4 1 (For ( 1 , j ) (1,j) ( 1 , j ) : L = s + δ 2 − p 2 L=\tfrac{s+\delta}2-p_2 L = 2 s + δ − p 2 and Q = s 2 4 + s 2 δ + δ 2 4 − p 2 2 Q=\tfrac{s^2}4+\tfrac s2\delta+\tfrac{\delta^2}4-p_2^2 Q = 4 s 2 + 2 s δ + 4 δ 2 − p 2 2 ; for ( 2 , j ) (2,j) ( 2 , j ) , with δ = p 2 − p j \delta=p_2-p_j δ = p 2 − p j : L = p 1 − s + δ 2 L=p_1-\tfrac{s+\delta}2 L = p 1 − 2 s + δ , Q = p 1 2 − s 2 4 − s 2 δ − δ 2 4 Q=p_1^2-\tfrac{s^2}4-\tfrac s2\delta-\tfrac{\delta^2}4 Q = p 1 2 − 4 s 2 − 2 s δ − 4 δ 2 ; for ( 1 , 2 ) (1,2) ( 1 , 2 ) : L = δ L=\delta L = δ , Q = s δ Q=s\delta Q = sδ .) By (D11.17) –(D11.14) :
E 12 ( L , L ) = 1 3 , E 1 j ( L , L ) = E 2 j ( L , L ) = 1 12 , E 12 ( L , Q ) = 1 3 E s = 2 3 m , E 1 j ( L , Q ) = E 2 j ( L , Q ) = 1 3 ⋅ E s 4 = 1 6 m , E 12 ( Q , Q ) = 1 3 E s 2 = 2 D 2 , E 1 j ( Q , Q ) = E 2 j ( Q , Q ) = 1 3 ⋅ E s 2 4 + 4 45 ⋅ E s 2 16 = 16 180 E s 2 = 8 15 D 2 . \begin{aligned}
E_{12}(L,L)&=\tfrac13, &
E_{1j}(L,L)=E_{2j}(L,L)&=\tfrac1{12},\\
E_{12}(L,Q)&=\tfrac13\E s=\tfrac2{3m}, &
E_{1j}(L,Q)=E_{2j}(L,Q)&=\tfrac13\cdot\tfrac{\E s}4=\tfrac1{6m},\\
E_{12}(Q,Q)&=\tfrac13\E s^2=\tfrac2{D_2}, &
E_{1j}(Q,Q)=E_{2j}(Q,Q)
&=\tfrac13\cdot\tfrac{\E s^2}4+\tfrac4{45}\cdot\tfrac{\E s^2}{16}
=\tfrac{16}{180}\,\E s^2=\tfrac8{15D_2}.
\end{aligned} E 12 ( L , L ) E 12 ( L , Q ) E 12 ( Q , Q ) = 3 1 , = 3 1 E s = 3 m 2 , = 3 1 E s 2 = D 2 2 , E 1 j ( L , L ) = E 2 j ( L , L ) E 1 j ( L , Q ) = E 2 j ( L , Q ) E 1 j ( Q , Q ) = E 2 j ( Q , Q ) = 12 1 , = 3 1 ⋅ 4 E s = 6 m 1 , = 3 1 ⋅ 4 E s 2 + 45 4 ⋅ 16 E s 2 = 180 16 E s 2 = 15 D 2 8 . There are 2 ( m − 2 ) 2(m-2) 2 ( m − 2 ) pairs of the types ( 1 , j ) , ( 2 , j ) (1,j),(2,j) ( 1 , j ) , ( 2 , j ) , so
∑ i < j E i j ( L , L ) = 1 3 + 2 ( m − 2 ) 12 = m 6 , ∑ i < j E i j ( L , Q ) = 2 3 m + 2 ( m − 2 ) 6 m = 2 + ( m − 2 ) 3 m = 1 3 , ∑ i < j E i j ( Q , Q ) = 2 D 2 + 16 ( m − 2 ) 15 D 2 = 2 ( 8 m − 1 ) 15 D 2 . \begin{aligned}
\sum_{i<j}E_{ij}(L,L)&=\tfrac13+\tfrac{2(m-2)}{12}=\tfrac m6,\\
\sum_{i<j}E_{ij}(L,Q)&=\tfrac2{3m}+\tfrac{2(m-2)}{6m}=\tfrac{2+(m-2)}{3m}
=\tfrac13,\\
\sum_{i<j}E_{ij}(Q,Q)&=\tfrac2{D_2}+\tfrac{16(m-2)}{15D_2}
=\tfrac{2(8m-1)}{15D_2}.
\end{aligned} i < j ∑ E ij ( L , L ) i < j ∑ E ij ( L , Q ) i < j ∑ E ij ( Q , Q ) = 3 1 + 12 2 ( m − 2 ) = 6 m , = 3 m 2 + 6 m 2 ( m − 2 ) = 3 m 2 + ( m − 2 ) = 3 1 , = D 2 2 + 15 D 2 16 ( m − 2 ) = 15 D 2 2 ( 8 m − 1 ) . Multiplying by 12 / ( m 2 ( m + 1 ) ) 12/(m^2(m+1)) 12/ ( m 2 ( m + 1 )) gives the three K K K -entries in (D11.28) .
Variances. By symmetry E L = E Q = 0 \E L=\E Q=0 E L = E Q = 0 , so, by Lemma D11.1 ,
G ( L , L ) = E ( P 1 − P 2 ) 2 = 2 D 2 , G ( L , Q ) = E [ ( P 1 − P 2 ) ( P 1 2 − P 2 2 ) ] = E [ P 1 3 + P 2 3 − P 1 P 2 ( P 1 + P 2 ) ] = 12 − 4 D 3 = 8 D 3 , G ( Q , Q ) = E ( P 1 2 − P 2 2 ) 2 = 2 E P 1 4 − 2 E P 1 2 P 2 2 = 48 − 8 D 4 = 40 D 4 . \begin{aligned}
G(L,L)&=\E(P_1-P_2)^2=\tfrac2{D_2},\\
G(L,Q)&=\E\bigl[(P_1-P_2)(P_1^2-P_2^2)\bigr]
=\E\bigl[P_1^3+P_2^3-P_1P_2(P_1+P_2)\bigr]
=\tfrac{12-4}{D_3}=\tfrac8{D_3},\\
G(Q,Q)&=\E(P_1^2-P_2^2)^2
=2\,\E P_1^4-2\,\E P_1^2P_2^2=\tfrac{48-8}{D_4}=\tfrac{40}{D_4}.
\end{aligned} G ( L , L ) G ( L , Q ) G ( Q , Q ) = E ( P 1 − P 2 ) 2 = D 2 2 , = E [ ( P 1 − P 2 ) ( P 1 2 − P 2 2 ) ] = E [ P 1 3 + P 2 3 − P 1 P 2 ( P 1 + P 2 ) ] = D 3 12 − 4 = D 3 8 , = E ( P 1 2 − P 2 2 ) 2 = 2 E P 1 4 − 2 E P 1 2 P 2 2 = D 4 48 − 8 = D 4 40 . Energy. The ( β , γ ) (\beta,\gamma) ( β , γ ) table, computed from (D11.18) (here j ≥ 5 j\ge5 j ≥ 5 ; in each row δ = p i − p j \delta=p_i-p_j δ = p i − p j for the listed pair ( i , j ) (i,j) ( i , j ) , i < j i<j i < j ):
pair β F γ F derivation ( 1 , 3 ) p 2 − p 4 0 F = δ ( p 2 − p 4 ) ( 2 , 4 ) p 1 − p 3 0 F = ( p 1 − p 3 ) δ ( 1 , 2 ) p 3 − p 4 2 − 1 4 F = ( s + δ 2 − p 3 ) ( s − δ 2 − p 4 ) ( 3 , 4 ) p 1 − p 2 2 − 1 4 F = ( p 1 − s + δ 2 ) ( p 2 − s − δ 2 ) ( 1 , 4 ) p 2 − p 3 2 1 4 F = ( s + δ 2 − p 3 ) ( p 2 − s − δ 2 ) ( 2 , 3 ) p 1 − p 4 2 1 4 F = ( p 1 − s − δ 2 ) ( s + δ 2 − p 4 ) ( 1 , j ) p 2 − p 4 2 0 F = ( s + δ 2 − p 3 ) ( p 2 − p 4 ) ( 2 , j ) p 1 − p 3 2 0 ( 3 , j ) − p 2 − p 4 2 0 ( 4 , j ) − p 1 − p 3 2 0 \begin{array}{l|cc|l}
\text{pair} & \beta_F & \gamma_F & \text{derivation}\\\hline
(1,3) & p_2-p_4 & 0 & F=\delta\,(p_2-p_4)\\
(2,4) & p_1-p_3 & 0 & F=(p_1-p_3)\,\delta\\
(1,2) & \tfrac{p_3-p_4}2 & -\tfrac14 &
F=\bigl(\tfrac{s+\delta}2-p_3\bigr)\bigl(\tfrac{s-\delta}2-p_4\bigr)\\
(3,4) & \tfrac{p_1-p_2}2 & -\tfrac14 &
F=\bigl(p_1-\tfrac{s+\delta}2\bigr)\bigl(p_2-\tfrac{s-\delta}2\bigr)\\
(1,4) & \tfrac{p_2-p_3}2 & \tfrac14 &
F=\bigl(\tfrac{s+\delta}2-p_3\bigr)\bigl(p_2-\tfrac{s-\delta}2\bigr)\\
(2,3) & \tfrac{p_1-p_4}2 & \tfrac14 &
F=\bigl(p_1-\tfrac{s-\delta}2\bigr)\bigl(\tfrac{s+\delta}2-p_4\bigr)\\
(1,j) & \tfrac{p_2-p_4}2 & 0 & F=\bigl(\tfrac{s+\delta}2-p_3\bigr)(p_2-p_4)\\
(2,j) & \tfrac{p_1-p_3}2 & 0 & \\
(3,j) & -\tfrac{p_2-p_4}2 & 0 & \\
(4,j) & -\tfrac{p_1-p_3}2 & 0 &
\end{array} pair ( 1 , 3 ) ( 2 , 4 ) ( 1 , 2 ) ( 3 , 4 ) ( 1 , 4 ) ( 2 , 3 ) ( 1 , j ) ( 2 , j ) ( 3 , j ) ( 4 , j ) β F p 2 − p 4 p 1 − p 3 2 p 3 − p 4 2 p 1 − p 2 2 p 2 − p 3 2 p 1 − p 4 2 p 2 − p 4 2 p 1 − p 3 − 2 p 2 − p 4 − 2 p 1 − p 3 γ F 0 0 − 4 1 − 4 1 4 1 4 1 0 0 0 0 derivation F = δ ( p 2 − p 4 ) F = ( p 1 − p 3 ) δ F = ( 2 s + δ − p 3 ) ( 2 s − δ − p 4 ) F = ( p 1 − 2 s + δ ) ( p 2 − 2 s − δ ) F = ( 2 s + δ − p 3 ) ( p 2 − 2 s − δ ) F = ( p 1 − 2 s − δ ) ( 2 s + δ − p 4 ) F = ( 2 s + δ − p 3 ) ( p 2 − p 4 ) For instance, for the pair ( 1 , 2 ) (1,2) ( 1 , 2 ) : F = [ ( s 2 − p 3 ) + δ 2 ] [ ( s 2 − p 4 ) − δ 2 ] = α + p 3 − p 4 2 δ − 1 4 δ 2 F=\bigl[(\tfrac s2-p_3)+\tfrac\delta2\bigr] \bigl[(\tfrac s2-p_4)-\tfrac\delta2\bigr] =\alpha+\tfrac{p_3-p_4}2\,\delta-\tfrac14\,\delta^2 F = [ ( 2 s − p 3 ) + 2 δ ] [ ( 2 s − p 4 ) − 2 δ ] = α + 2 p 3 − p 4 δ − 4 1 δ 2 with α \alpha α F 12 \mathcal F_{12} F 12 -measurable; the rows ( 3 , 4 ) (3,4) ( 3 , 4 ) , ( 1 , 4 ) (1,4) ( 1 , 4 ) , ( 2 , 3 ) (2,3) ( 2 , 3 ) are identical expansions. By (D11.17) –(D11.14) ,
E 13 ( F , F ) = E 24 ( F , F ) = 1 3 E ( P 2 − P 4 ) 2 = 2 3 D 2 , E 12 ( F , F ) = E 34 ( F , F ) = E 14 ( F , F ) = E 23 ( F , F ) = 1 3 ⋅ E ( P 3 − P 4 ) 2 4 + 4 45 ⋅ E s 2 16 = 1 6 D 2 + 1 30 D 2 = 1 5 D 2 , E i j ( F , F ) ( i ∈ { 1 , 2 , 3 , 4 } , j ≥ 5 ) = 1 3 ⋅ E ( P a − P b ) 2 4 = 1 6 D 2 ( 4 ( m − 4 ) pairs ) . \begin{aligned}
E_{13}(F,F)=E_{24}(F,F)
&=\tfrac13\,\E(P_2-P_4)^2=\tfrac2{3D_2},\\
E_{12}(F,F)=E_{34}(F,F)=E_{14}(F,F)=E_{23}(F,F)
&=\tfrac13\cdot\tfrac{\E(P_3-P_4)^2}4+\tfrac4{45}\cdot\tfrac{\E s^2}{16}
=\tfrac1{6D_2}+\tfrac1{30D_2}=\tfrac1{5D_2},\\
E_{ij}(F,F)\ \ (i\in\{1,2,3,4\},\ j\ge5)
&=\tfrac13\cdot\tfrac{\E(P_a-P_b)^2}4=\tfrac1{6D_2}
\qquad(4(m-4)\text{ pairs}).
\end{aligned} E 13 ( F , F ) = E 24 ( F , F ) E 12 ( F , F ) = E 34 ( F , F ) = E 14 ( F , F ) = E 23 ( F , F ) E ij ( F , F ) ( i ∈ { 1 , 2 , 3 , 4 } , j ≥ 5 ) = 3 1 E ( P 2 − P 4 ) 2 = 3 D 2 2 , = 3 1 ⋅ 4 E ( P 3 − P 4 ) 2 + 45 4 ⋅ 16 E s 2 = 6 D 2 1 + 30 D 2 1 = 5 D 2 1 , = 3 1 ⋅ 4 E ( P a − P b ) 2 = 6 D 2 1 ( 4 ( m − 4 ) pairs ) . Hence
∑ i < j E i j ( F , F ) = 1 D 2 [ 4 3 + 4 5 + 4 ( m − 4 ) 6 ] = 1 D 2 ⋅ 20 + 12 + 10 ( m − 4 ) 15 = 2 ( 5 m − 4 ) 15 D 2 , \sum_{i<j}E_{ij}(F,F)
=\frac1{D_2}\Bigl[\frac43+\frac45+\frac{4(m-4)}6\Bigr]
=\frac1{D_2}\cdot\frac{20+12+10(m-4)}{15}
=\frac{2(5m-4)}{15\,D_2}, i < j ∑ E ij ( F , F ) = D 2 1 [ 3 4 + 5 4 + 6 4 ( m − 4 ) ] = D 2 1 ⋅ 15 20 + 12 + 10 ( m − 4 ) = 15 D 2 2 ( 5 m − 4 ) , and K ( F , F ) = 12 m 2 ( m + 1 ) ⋅ 2 ( 5 m − 4 ) 15 m ( m + 1 ) = 8 ( 5 m − 4 ) 5 m 3 ( m + 1 ) 2 K(F,F)=\tfrac{12}{m^2(m+1)}\cdot\tfrac{2(5m-4)}{15m(m+1)} =\tfrac{8(5m-4)}{5m^3(m+1)^2} K ( F , F ) = m 2 ( m + 1 ) 12 ⋅ 15 m ( m + 1 ) 2 ( 5 m − 4 ) = 5 m 3 ( m + 1 ) 2 8 ( 5 m − 4 ) .
Variance. E F = E P 1 P 2 − E P 1 P 4 − E P 2 P 3 + E P 3 P 4 = 0 \E F=\E P_1P_2-\E P_1P_4-\E P_2P_3+\E P_3P_4=0 E F = E P 1 P 2 − E P 1 P 4 − E P 2 P 3 + E P 3 P 4 = 0 , and expanding F 2 = ( p 1 2 − 2 p 1 p 3 + p 3 2 ) ( p 2 2 − 2 p 2 p 4 + p 4 2 ) F^2=(p_1^2-2p_1p_3+p_3^2)(p_2^2-2p_2p_4+p_4^2) F 2 = ( p 1 2 − 2 p 1 p 3 + p 3 2 ) ( p 2 2 − 2 p 2 p 4 + p 4 2 ) termwise with Lemma D11.1 (all four indices distinct),
E F 2 = 4 ⋅ 4 − 8 ⋅ 2 + 4 ⋅ 1 D 4 = 4 D 4 , \E F^2
=\frac{4\cdot4-8\cdot2+4\cdot1}{D_4}
=\frac4{D_4}, E F 2 = D 4 4 ⋅ 4 − 8 ⋅ 2 + 4 ⋅ 1 = D 4 4 , the three groups being: the four square–square products, each with E P a 2 P b 2 = 4 / D 4 \E P_a^2P_b^2=4/D_4 E P a 2 P b 2 = 4/ D 4 , totalling 16 / D 4 16/D_4 16/ D 4 ; the four products of a square with a − 2 p b p c -2p_bp_c − 2 p b p c factor, each contributing − 2 E P a 2 P b P c = − 4 / D 4 -2\,\E P_a^2P_bP_c=-4/D_4 − 2 E P a 2 P b P c = − 4/ D 4 , totalling − 16 / D 4 -16/D_4 − 16/ D 4 ; and the single product ( − 2 p 1 p 3 ) ( − 2 p 2 p 4 ) (-2p_1p_3)(-2p_2p_4) ( − 2 p 1 p 3 ) ( − 2 p 2 p 4 ) , contributing 4 E P 1 P 2 P 3 P 4 = 4 / D 4 4\,\E P_1P_2P_3P_4=4/D_4 4 E P 1 P 2 P 3 P 4 = 4/ D 4 . The quotient follows by G ( F , F ) = E F 2 G(F,F)=\E F^2 G ( F , F ) = E F 2 and D 4 = m ( m + 1 ) ( m + 2 ) ( m + 3 ) D_4=m(m+1)(m+2)(m+3) D 4 = m ( m + 1 ) ( m + 2 ) ( m + 3 ) .
Write λ ∗ = ( m + 2 ) ( m + 3 ) / ( 5 m 2 ) \lambda^*=(m+2)(m+3)/(5m^2) λ ∗ = ( m + 2 ) ( m + 3 ) / ( 5 m 2 ) and let Φ = K − λ ∗ G \Phi=K-\lambda^*G Φ = K − λ ∗ G , an S m S_m S m -invariant symmetric bilinear form on V m , 2 V_{m,2} V m , 2 (Lemma D11.2 ). By Lemma D11.4 and Lemma D11.5 (1),
Φ ( f , f ) = Φ ( f t r i v , f t r i v ) + Φ ( f s t d , f s t d ) + Φ ( f X , f X ) \Phi(f,f)=\Phi(f_{\rm triv},f_{\rm triv})
+\Phi(f_{\rm std},f_{\rm std})+\Phi(f_{\mathrm X},f_{\mathrm X}) Φ ( f , f ) = Φ ( f triv , f triv ) + Φ ( f std , f std ) + Φ ( f X , f X ) for the isotypic components of any f ∈ V m , 2 f\in V_{m,2} f ∈ V m , 2 (the X \mathrm X X -term absent at m = 3 m=3 m = 3 ). We treat the three sectors.
Trivial sector. W t r i v = R [ f 0 ] W_{\rm triv}=\R[f_0] W triv = R [ f 0 ] and, by Lemma D11.6 , K ( f 0 , f 0 ) = λ ∗ G ( f 0 , f 0 ) K(f_0,f_0)=\lambda^*G(f_0,f_0) K ( f 0 , f 0 ) = λ ∗ G ( f 0 , f 0 ) , i.e. Φ ≡ 0 \Phi\equiv0 Φ ≡ 0 on W t r i v W_{\rm triv} W triv , with G ( f 0 , f 0 ) > 0 G(f_0,f_0)>0 G ( f 0 , f 0 ) > 0 .
Standard sector. Apply Lemma D11.5 (2) with E = s t d E=\mathrm{std} E = std , k = 2 k=2 k = 2 , the maps T 1 , T 2 T_1,T_2 T 1 , T 2 and seed v 0 = e 1 − e 2 v_0=e_1-e_2 v 0 = e 1 − e 2 of Lemma D11.4 (2) (linearly independent in Hom \operatorname{Hom} Hom , since c 1 T 1 + c 2 T 2 = 0 c_1T_1+c_2T_2=0 c 1 T 1 + c 2 T 2 = 0 evaluated at v 0 v_0 v 0 gives c 1 L + c 2 Q = 0 c_1L+c_2Q=0 c 1 L + c 2 Q = 0 , hence c 1 = c 2 = 0 c_1=c_2=0 c 1 = c 2 = 0 ). Positive definiteness of Φ \Phi Φ on W s t d W_{\rm std} W std is therefore equivalent to positive definiteness of the 2 × 2 2\times2 2 × 2 Gram matrix of ( L , Q ) (L,Q) ( L , Q ) under Φ \Phi Φ . Multiplying the entries of (D11.28) by the common positive factor m ( m + 1 ) / 2 m(m+1)/2 m ( m + 1 ) /2 yields the normalized matrices
K ~ = ( 1 2 m 2 m 4 ( 8 m − 1 ) 5 m 2 ( m + 1 ) ) , G ~ = ( 1 4 m + 2 4 m + 2 20 ( m + 2 ) ( m + 3 ) ) , \widetilde K=
\begin{pmatrix}
1 & \tfrac2m\\
\tfrac2m & \tfrac{4(8m-1)}{5m^2(m+1)}
\end{pmatrix},
\qquad
\widetilde G=
\begin{pmatrix}
1 & \tfrac4{m+2}\\
\tfrac4{m+2} & \tfrac{20}{(m+2)(m+3)}
\end{pmatrix}, K = ( 1 m 2 m 2 5 m 2 ( m + 1 ) 4 ( 8 m − 1 ) ) , G = ( 1 m + 2 4 m + 2 4 ( m + 2 ) ( m + 3 ) 20 ) , and a direct computation gives
( K ~ − λ ∗ G ~ ) 11 = 1 − ( m + 2 ) ( m + 3 ) 5 m 2 = 4 m 2 − 5 m − 6 5 m 2 = ( 4 m + 3 ) ( m − 2 ) 5 m 2 , ( K ~ − λ ∗ G ~ ) 12 = 2 m − 4 ( m + 3 ) 5 m 2 = 10 m − 4 m − 12 5 m 2 = 6 ( m − 2 ) 5 m 2 , ( K ~ − λ ∗ G ~ ) 22 = 4 ( 8 m − 1 ) 5 m 2 ( m + 1 ) − 4 m 2 = 4 ( 8 m − 1 ) − 20 ( m + 1 ) 5 m 2 ( m + 1 ) = 12 ( m − 2 ) 5 m 2 ( m + 1 ) , \begin{aligned}
(\widetilde K-\lambda^*\widetilde G)_{11}
&=1-\frac{(m+2)(m+3)}{5m^2}
=\frac{4m^2-5m-6}{5m^2}=\frac{(4m+3)(m-2)}{5m^2},\\
(\widetilde K-\lambda^*\widetilde G)_{12}
&=\frac2m-\frac{4(m+3)}{5m^2}
=\frac{10m-4m-12}{5m^2}=\frac{6(m-2)}{5m^2},\\
(\widetilde K-\lambda^*\widetilde G)_{22}
&=\frac{4(8m-1)}{5m^2(m+1)}-\frac4{m^2}
=\frac{4(8m-1)-20(m+1)}{5m^2(m+1)}=\frac{12(m-2)}{5m^2(m+1)},
\end{aligned} ( K − λ ∗ G ) 11 ( K − λ ∗ G ) 12 ( K − λ ∗ G ) 22 = 1 − 5 m 2 ( m + 2 ) ( m + 3 ) = 5 m 2 4 m 2 − 5 m − 6 = 5 m 2 ( 4 m + 3 ) ( m − 2 ) , = m 2 − 5 m 2 4 ( m + 3 ) = 5 m 2 10 m − 4 m − 12 = 5 m 2 6 ( m − 2 ) , = 5 m 2 ( m + 1 ) 4 ( 8 m − 1 ) − m 2 4 = 5 m 2 ( m + 1 ) 4 ( 8 m − 1 ) − 20 ( m + 1 ) = 5 m 2 ( m + 1 ) 12 ( m − 2 ) , that is,
5 m 2 ( K ~ − λ ∗ G ~ ) = ( m − 2 ) ( 4 m + 3 6 6 12 m + 1 ) . 5m^2\,(\widetilde K-\lambda^*\widetilde G)
=(m-2)
\begin{pmatrix}
4m+3 & 6\\
6 & \tfrac{12}{m+1}
\end{pmatrix}. 5 m 2 ( K − λ ∗ G ) = ( m − 2 ) ( 4 m + 3 6 6 m + 1 12 ) . For m ≥ 3 m\ge3 m ≥ 3 the factor m − 2 m-2 m − 2 is positive, the diagonal entries are positive, and the determinant of the bracketed matrix is 12 ( 4 m + 3 ) m + 1 − 36 = 12 ( 4 m + 3 ) − 36 ( m + 1 ) m + 1 = 12 m m + 1 > 0 \tfrac{12(4m+3)}{m+1}-36=\tfrac{12(4m+3)-36(m+1)}{m+1}=\tfrac{12m}{m+1}>0 m + 1 12 ( 4 m + 3 ) − 36 = m + 1 12 ( 4 m + 3 ) − 36 ( m + 1 ) = m + 1 12 m > 0 . Hence Φ \Phi Φ is positive definite on W s t d W_{\rm std} W std : Φ ( f s t d , f s t d ) > 0 \Phi(f_{\rm std},f_{\rm std})>0 Φ ( f std , f std ) > 0 whenever f s t d ≠ 0 f_{\rm std}\ne0 f std = 0 .
Two-row sector (m ≥ 4 m\ge4 m ≥ 4 ). W X W_{\mathrm X} W X has multiplicity one and is generated by F F F (Lemma D11.4 (3)), so Lemma D11.5 (2) with k = 1 k=1 k = 1 reduces positivity on W X W_{\mathrm X} W X to the sign of the scalar Φ ( F , F ) \Phi(F,F) Φ ( F , F ) . By Lemma D11.8 ,
K ( F , F ) G ( F , F ) = 2 ( 5 m − 4 ) m + 1 λ ∗ = λ ∗ + 9 ( m − 1 ) m + 1 λ ∗ > λ ∗ , \frac{K(F,F)}{G(F,F)}
=\frac{2(5m-4)}{m+1}\,\lambda^*
=\lambda^*+\frac{9(m-1)}{m+1}\,\lambda^*
>\lambda^*, G ( F , F ) K ( F , F ) = m + 1 2 ( 5 m − 4 ) λ ∗ = λ ∗ + m + 1 9 ( m − 1 ) λ ∗ > λ ∗ , since 2 ( 5 m − 4 ) − ( m + 1 ) = 9 ( m − 1 ) > 0 2(5m-4)-(m+1)=9(m-1)>0 2 ( 5 m − 4 ) − ( m + 1 ) = 9 ( m − 1 ) > 0 . Hence Φ ( F , F ) = G ( F , F ) ( K ( F , F ) G ( F , F ) − λ ∗ ) > 0 \Phi(F,F)=G(F,F)\bigl(\tfrac{K(F,F)}{G(F,F)}-\lambda^*\bigr)>0 Φ ( F , F ) = G ( F , F ) ( G ( F , F ) K ( F , F ) − λ ∗ ) > 0 and Φ \Phi Φ is positive definite on W X W_{\mathrm X} W X .
Assembly. For every f ∈ V m , 2 f\in V_{m,2} f ∈ V m , 2 , Φ ( f , f ) ≥ 0 \Phi(f,f)\ge0 Φ ( f , f ) ≥ 0 , i.e. K ( f , f ) ≥ λ ∗ G ( f , f ) K(f,f)\ge\lambda^*G(f,f) K ( f , f ) ≥ λ ∗ G ( f , f ) , with equality if and only if f s t d = 0 f_{\rm std}=0 f std = 0 and f X = 0 f_{\mathrm X}=0 f X = 0 , i.e. f ∈ W t r i v = R [ f 0 ] f\in W_{\rm triv}=\R[f_0] f ∈ W triv = R [ f 0 ] . Since K ( f 0 , f 0 ) = λ ∗ G ( f 0 , f 0 ) K(f_0,f_0)=\lambda^*G(f_0,f_0) K ( f 0 , f 0 ) = λ ∗ G ( f 0 , f 0 ) with G ( f 0 , f 0 ) > 0 G(f_0,f_0)>0 G ( f 0 , f 0 ) > 0 , the minimum (D11.4) equals λ ∗ \lambda^* λ ∗ and is attained exactly on R [ f 0 ] = R [ ∣ X ∣ 2 − ( m − 1 ) ] \R[f_0]=\R[\abs X^2-(m-1)] R [ f 0 ] = R [ ∣ X ∣ 2 − ( m − 1 )] (Lemma D11.6 ). Finally ( m + 2 ) ( m + 3 ) > m 2 (m+2)(m+3)>m^2 ( m + 2 ) ( m + 3 ) > m 2 gives λ ∗ > 1 5 \lambda^*>\tfrac15 λ ∗ > 5 1 for all m m m , and λ ∗ → 1 5 \lambda^*\to\tfrac15 λ ∗ → 5 1 .
All statements are conditional on the identification (D11.8) , certified in solutions/conditional-fiber-frame-structure.md: the root frame ρ r o o t \rho_{\rm root} ρ root is an admissible even frame, and for every f f f in the maximal form domain (in particular for every polynomial) the root conditional-fiber form equals the pair-redistribution expression (D11.2) .
(1). Let ( c r , w r , M , ε ) (c_r,w_r,M,\eps) ( c r , w r , M , ε ) be a degree-2 dual certificate (D11.7) . Apply the direction bound in (D11.7) at the m ( m − 1 ) m(m-1) m ( m − 1 ) atoms of ρ r o o t \rho_{\rm root} ρ root and average:
∑ r w r K ( c r , c r ) = ( m − 1 ) ∫ ∑ r w r q θ [ c r ] d ρ r o o t ( θ ) ≤ ( m − 1 ) ∫ θ T M θ d ρ r o o t ( θ ) = Tr ( M ( m − 1 ) ∫ θ θ T d ρ r o o t ) = Tr M ≤ ε , \sum_rw_r\,K(c_r,c_r)
=(m-1)\int\sum_rw_r\,\qJac_\theta[c_r]\dd\rho_{\rm root}(\theta)
\le(m-1)\int\theta^TM\theta\dd\rho_{\rm root}(\theta)
=\Tr\Bigl(M\,(m-1)\!\int\theta\theta^T\dd\rho_{\rm root}\Bigr)
=\Tr M\le\eps, r ∑ w r K ( c r , c r ) = ( m − 1 ) ∫ r ∑ w r q θ [ c r ] d ρ root ( θ ) ≤ ( m − 1 ) ∫ θ T Mθ d ρ root ( θ ) = Tr ( M ( m − 1 ) ∫ θ θ T d ρ root ) = Tr M ≤ ε , using the frame identity ( m − 1 ) ∫ θ θ T d ρ r o o t = I H 0 (m-1)\int\theta\theta^T\dd\rho_{\rm root}=I_{H_0} ( m − 1 ) ∫ θ θ T d ρ root = I H 0 and M M M symmetric on H 0 H_0 H 0 . On the other hand, by Theorem D11.1 , K ( c r , c r ) ≥ λ ∗ G ( c r , c r ) K(c_r,c_r)\ge\lambda^*G(c_r,c_r) K ( c r , c r ) ≥ λ ∗ G ( c r , c r ) for every r r r , so
ε ≥ ∑ r w r K ( c r , c r ) ≥ λ ∗ ∑ r w r G ( c r , c r ) = λ ∗ = ( m + 2 ) ( m + 3 ) 5 m 2 > 1 5 . \eps\ \ge\ \sum_rw_r\,K(c_r,c_r)
\ \ge\ \lambda^*\sum_rw_r\,G(c_r,c_r)=\lambda^*
=\frac{(m+2)(m+3)}{5m^2}>\frac15 . ε ≥ r ∑ w r K ( c r , c r ) ≥ λ ∗ r ∑ w r G ( c r , c r ) = λ ∗ = 5 m 2 ( m + 2 ) ( m + 3 ) > 5 1 . (2). Immediate from (1): every degree-2 certificate objective exceeds 1 5 \tfrac15 5 1 uniformly in m ≥ 3 m\ge3 m ≥ 3 , so no sequence ε m → 0 \eps_m\to0 ε m → 0 exists at k = 2 k=2 k = 2 . Within the candidate framework, in which a fixed-degree dual refuter is exactly such a certificate sequence, any polynomial dual refutation must therefore use degree k ≥ 3 k\ge3 k ≥ 3 .
(3). For any admissible ρ \rho ρ whose averaged form A ρ A_\rho A ρ is defined on V m , 2 V_{m,2} V m , 2 , the supremum defining Λ m , 2 \Lambda_{m,2} Λ m , 2 dominates the value at ρ = ρ r o o t \rho=\rho_{\rm root} ρ = ρ root , and by (D11.8) and Theorem D11.1 that value is λ min ( K , G ) ∣ V m , 2 = λ ∗ \lmin(K,G)|_{V_{m,2}}=\lambda^* λ m i n ( K , G ) ∣ V m , 2 = λ ∗ .
Remarks, non-claims, and audit ¶ Two exact computations in rational arithmetic, kept in the project’s run records, give the degree-two root-frame pencil minimum at m = 3 , 4 , 5 m=3,4,5 m = 3 , 4 , 5 as 2 / 3 2/3 2/3 , 21 / 40 21/40 21/40 , 56 / 125 56/125 56/125 respectively, and record the radial quotient anchor ( m + 2 ) ( m + 3 ) / ( 5 m 2 ) (m+2)(m+3)/(5m^2) ( m + 2 ) ( m + 3 ) / ( 5 m 2 ) exactly for every computed m ≤ 15 m\le15 m ≤ 15 . These values agree with the closed form (D11.5) : ( 5 ⋅ 6 ) / 45 = 2 / 3 (5\cdot6)/45=2/3 ( 5 ⋅ 6 ) /45 = 2/3 , ( 6 ⋅ 7 ) / 80 = 21 / 40 (6\cdot7)/80=21/40 ( 6 ⋅ 7 ) /80 = 21/40 , ( 7 ⋅ 8 ) / 125 = 56 / 125 (7\cdot8)/125=56/125 ( 7 ⋅ 8 ) /125 = 56/125 . Per repository constraint, these artifacts are directional research evidence only; no step of the proofs above uses them, and this agreement certifies nothing.
None. Theorem D11.1 is unconditional; every step is finite-dimensional linear algebra, elementary representation theory of S m S_m S m (proved from facts (F1)–(F5), themselves proved or classical with one-line arguments), and exact Dirichlet moments (Lemma D11.1 , whose proof invokes the classical Gamma–Dirichlet factorization: the normalized vector of i.i.d. standard exponentials is Dir ( 1 , … , 1 ) \Dir(1,\dots,1) Dir ( 1 , … , 1 ) and independent of their sum). Corollary D11.1 is conditional exactly on the hypothesis stated in its preamble, namely the certified identification (D11.8) (nodes lem:conditional-fiber-form and prop:conditional-fiber-root-obstruction , both checked_by: agent with a persisted review), together with the candidate status of the Λ m , k \Lambda_{m,k} Λ m , k /dual-certificate framework itself.
This dossier does not claim: any upper bound on Λ m , 2 \Lambda_{m,2} Λ m , 2 or on any all-frame quantity; anything about Λ m , k \Lambda_{m,k} Λ m , k or root-frame pencils for k ≥ 3 k\ge3 k ≥ 3 ; anything about non-polynomial tests — indeed the certified vertex-cap obstruction (Proposition 22.1 ) shows the full L 2 L^2 L 2 root-frame gap is O ( m − 2 ) O(m^{-2}) O ( m − 2 ) , so the degree-two floor (D11.5) genuinely does not extend beyond the polynomial quotient; any optimality of the root orbit among admissible frames; any answer to Conjecture 22.1 ; and nothing about KLS.
Obstructions respected. The candidate node carries no bounded_by edge. Consistency checks against the neighboring certified and imported obstructions: (i) prop:conditional-fiber-root-obstruction (root-frame L 2 L^2 L 2 gap O ( m − 2 ) O(m^{-2}) O ( m − 2 ) via a vertex-cap indicator) is compatible with (D11.5) because the cap indicator is not a polynomial of degree two; the two statements jointly prove that any test exhibiting the root-frame collapse must leave V m , 2 V_{m,2} V m , 2 , which is precisely the content of Corollary D11.1 (2) for the dual channel. (ii) prop:sasada-negative-exchange (imported negative-rate exchange upper bound 48 / [ m ( m + 1 ) ] 48/[m(m+1)] 48/ [ m ( m + 1 )] for the L 2 L^2 L 2 gap) is compatible for the same reason. (iii) The six route-level obstruction nodes (rem:two-tail-slice-bounds , rem:projection-ceiling , rem:crude-insufficient , rem:relative-ceiling , rem:profile-circularity , rem:single-coordinate-cuts ) fence Eldan-localization proof shapes; no stochastic localization, projection summation, bootstrap, isoperimetric localization, or rank-one inference occurs here. No numerical output justifies any step.