Throughout, a real-valued function on a subinterval I I I of the real numbers R \mathbb{R} R is called continuous on I I I when it is continuous relative to I I I , both I I I and the codomain R \mathbb{R} R carrying the metric of the real line . Expectations are unchanged when integrands are modified off events of probability 1 1 1 , and all uses of the Tonelli and Fubini theorems are on the product of [ 0 , T ] [0,T] [ 0 , T ] (trace Borel Ο \sigma Ο -algebra, restricted Lebesgue measure) with ( Ξ© , F , P ) (\Omega,\mathcal{F},\mathbb{P}) ( Ξ© , F , P ) , both finite measures. By conclusions 1 and 2 of the policy lemma all entries of E \mathcal{E} E , B \mathcal{B} B , E ~ \tilde{\mathcal{E}} E ~ , G \mathcal{G} G , K ~ \tilde{\mathcal{K}} K ~ , Ξ \Pi Ξ , ( Ξ ~ β ) β 1 (\tilde{\Theta}^\star)^{-1} ( Ξ ~ β ) β 1 , and of the closed-loop matrix M t = E t β B t G t β K ~ t E ~ t \mathcal{M}_t=\mathcal{E}_t-\mathcal{B}_t\mathcal{G}_t-\tilde{\mathcal{K}}_t\tilde{\mathcal{E}}_t M t β = E t β β B t β G t β β K ~ t β E ~ t β (written M t M_t M t β in the policy lemma ; renamed M t \mathcal{M}_t M t β here to avoid collision with the state martingale vector M t M_t M t β of the statement) are continuous, hence bounded in absolute value, each entry attaining a maximum and a minimum by the extreme value theorem : fix entry bounds c E c_{\mathcal{E}} c E β , c B c_{\mathcal{B}} c B β , c E ~ c_{\tilde{\mathcal{E}}} c E ~ β , C G C_{\mathcal{G}} C G β , C K ~ C_{\tilde{K}} C K ~ β , c Ξ c_\Pi c Ξ β , c Ξ ~ c_{\tilde\Theta} c Ξ ~ β , c M c_{\mathcal{M}} c M β respectively. For a matrix H H H with p p p rows, q q q columns, and entries bounded by c c c , the row-wise Cauchy-Schwarz estimate gives β£ H x β£ β€ p q β c β β£ x β£ |Hx|\le\sqrt{pq}\,c\,|x| β£ H x β£ β€ pq β c β£ x β£ for x β R q x\in\mathbb{R}^q x β R q (as in the proof of the completion-of-squares theorem ); write g β = m l β C G g^*=\sqrt{ml}\,C_{\mathcal{G}} g β = m l β C G β , k β = l l ~ β C K ~ k^*=\sqrt{l\tilde{l}}\,C_{\tilde{K}} k β = l l ~ β C K ~ β , b β = l m β c B b^*=\sqrt{lm}\,c_{\mathcal{B}} b β = l m β c B β , c β = l β l β ( c E + l ~ C K ~ c E ~ ) c^*=\sqrt{l\,l}\,(c_{\mathcal{E}}+\tilde{l}C_{\tilde{K}}c_{\tilde{\mathcal{E}}}) c β = l l β ( c E β + l ~ C K ~ β c E ~ β ) , c M β = l β c M c_{\mathcal{M}}^*=l\,c_{\mathcal{M}} c M β β = l c M β for the resulting operator bounds of G t \mathcal{G}_t G t β , K ~ t \tilde{\mathcal{K}}_t K ~ t β , B t \mathcal{B}_t B t β , E t β K ~ t E ~ t \mathcal{E}_t-\tilde{\mathcal{K}}_t\tilde{\mathcal{E}}_t E t β β K ~ t β E ~ t β , M t \mathcal{M}_t M t β (the entries of E t β K ~ t E ~ t \mathcal{E}_t-\tilde{\mathcal{K}}_t\tilde{\mathcal{E}}_t E t β β K ~ t β E ~ t β being bounded by c 1 = c E + l ~ C K ~ c E ~ c_1=c_{\mathcal{E}}+\tilde{l}C_{\tilde{K}}c_{\tilde{\mathcal{E}}} c 1 β = c E β + l ~ C K ~ β c E ~ β ). The control set A \mathcal{A} A is convex by hypothesis; this is a standing assumption of the second-moment , fourth-moment , state residual , and covariance deviation lemmas invoked below. Recall the residual bounds: with z s = ( s s , a s ) z_s=(\mathfrak{s}_s,\mathfrak{a}_s) z s β = ( s s β , a s β ) , Ξ = l ( B + K ) l ( l + m ) \Lambda=l(B+K)\sqrt{l(l+m)} Ξ = l ( B + K ) l ( l + m ) β , Ξ ~ = l l ~ ( B ~ + K ~ ) \tilde{\Lambda}=\sqrt{l\tilde{l}}(\tilde{B}+\tilde{K}) Ξ ~ = l l ~ β ( B ~ + K ~ ) , c e = 3 2 l l K ( l + m ) c_e=\tfrac{3}{2}l\sqrt{l}K(l+m) c e β = 2 3 β l l β K ( l + m ) , and c ~ e = 3 2 l l ~ K ~ \tilde{c}_e=\tfrac{3}{2}l\sqrt{\tilde{l}}\tilde{K} c ~ e β = 2 3 β l l ~ β K ~ , part (a) of the state residual lemma gives β£ e s β£ β€ min β‘ ( c e N β 1 / 2 β£ z s β£ 2 , β 2 Ξ β£ z s β£ ) |e_s|\le\min(c_e N^{-1/2}|z_s|^2,\,2\Lambda|z_s|) β£ e s β β£ β€ min ( c e β N β 1/2 β£ z s β β£ 2 , 2Ξβ£ z s β β£ ) and part (a) of the observation residual lemma gives β£ e ~ s β£ β€ min β‘ ( c ~ e N β 1 / 2 β£ s s β£ 2 , β 2 Ξ ~ β£ s s β£ ) |\tilde{e}_s|\le\min(\tilde{c}_e N^{-1/2}|\mathfrak{s}_s|^2,\,2\tilde{\Lambda}|\mathfrak{s}_s|) β£ e ~ s β β£ β€ min ( c ~ e β N β 1/2 β£ s s β β£ 2 , 2 Ξ ~ β£ s s β β£ ) , at every point of [ 0 , T ] Γ Ξ© [0,T]\times\Omega [ 0 , T ] Γ Ξ© . Finally let Ξ t \Xi_t Ξ t β be the sum of all counters, with c ~ t β€ Ξ t \tilde{c}_t\le\Xi_t c ~ t β β€ Ξ t β and E [ Ξ T p ] < β \mathbb{E}[\Xi_T^p]<\infty E [ Ξ T p β ] < β for every natural p p p , by part (c) of the multiplier lemma .
Step 1: part (a). By conclusion 4(c) of the policy lemma , β£ s ^ t N β£ β€ C β ( N 1 / 2 + N β 1 / 2 c ~ T ) |\hat{\mathfrak{s}}^N_t|\le C^\circ(N^{1/2}+N^{-1/2}\tilde{c}_T) β£ s ^ t N β β£ β€ C β ( N 1/2 + N β 1/2 c ~ T β ) at every point of Ξ© 0 Γ [ 0 , T ] \Omega_0\times[0,T] Ξ© 0 β Γ [ 0 , T ] , so β£ a t β£ = Ο t β£ G t s ^ t N β£ β€ β£ G t s ^ t N β£ β€ g β C β ( N 1 / 2 + N β 1 / 2 Ξ T ) |\mathfrak{a}_t|=\chi_t|\mathcal{G}_t\hat{\mathfrak{s}}^N_t|\le|\mathcal{G}_t\hat{\mathfrak{s}}^N_t|\le g^*C^\circ(N^{1/2}+N^{-1/2}\Xi_T) β£ a t β β£ = Ο t β β£ G t β s ^ t N β β£ β€ β£ G t β s ^ t N β β£ β€ g β C β ( N 1/2 + N β 1/2 Ξ T β ) there, the clamp indicator taking the values 0 0 0 and 1 1 1 only. Hence, for p β { 2 , 4 } p\in\{2,4\} p β { 2 , 4 } , E [ β£ a t β£ p ] β€ ( g β C β ) p β 2 p β E [ N p / 2 + N β p / 2 Ξ T β p ] < β \mathbb{E}[|\mathfrak{a}_t|^p]\le(g^*C^\circ)^p\,2^p\,\mathbb{E}[N^{p/2}+N^{-p/2}\Xi_T^{\,p}]<\infty E [ β£ a t β β£ p ] β€ ( g β C β ) p 2 p E [ N p /2 + N β p /2 Ξ T p β ] < β uniformly in t t t , and A 2 \mathcal{A}_2 A 2 β and A 4 \mathcal{A}_4 A 4 β are finite, their integrands being measurable by clause (a) of the a priori second-moment bound and of the fourth-moment bound . So the state residual lemma applies. Adaptedness. Ξ£ t \Sigma_t Ξ£ t β , hence s t \mathfrak{s}_t s t β , is F t s y s \mathcal{F}^{\mathrm{sys}}_t F t sys β -measurable by part (iv) of the existence theorem (S t S_t S t β being constant). For the filter: by conclusion 4(a) of the policy lemma, s ^ t N = f c ~ t N ( t , ( Ο 1 , β¦ , Ο c ~ t ) , ( Ο
1 , β¦ , Ο
c ~ t ) ) \hat{\mathfrak{s}}^N_t=f^N_{\tilde{c}_t}(t,(\tau_1,\dots,\tau_{\tilde{c}_t}),(\upsilon_1,\dots,\upsilon_{\tilde{c}_t})) s ^ t N β = f c ~ t β N β ( t , ( Ο 1 β , β¦ , Ο c ~ t β β ) , ( Ο
1 β , β¦ , Ο
c ~ t β β )) on Ξ© 0 \Omega_0 Ξ© 0 β ; by part (iv) of the existence theorem the observation-event count, event times, and channels up to t t t are measurable for the observation filtration, contained in F t s y s \mathcal{F}^{\mathrm{sys}}_t F t sys β ; on each event { c ~ t = k } β F t s y s \{\tilde{c}_t=k\}\in\mathcal{F}^{\mathrm{sys}}_t { c ~ t β = k } β F t sys β the value f k N ( t , Ο , Ο
) f^N_k(t,\tau,\upsilon) f k N β ( t , Ο , Ο
) is, for each of the finitely many channel words Ο
β { 1 , β¦ , l ~ } k \upsilon\in\{1,\dots,\tilde{l}\}^k Ο
β { 1 , β¦ , l ~ } k , a sequentially continuous function of ( Ο 1 , β¦ , Ο k ) (\tau_1,\dots,\tau_k) ( Ο 1 β , β¦ , Ο k β ) (its defining formula in conclusion 3 of the policy lemma involving the continuous Ξ¦ \Phi Ξ¦ , Ξ¨ \Psi Ξ¨ , K ~ \tilde{\mathcal{K}} K ~ and, on { c ~ t = k } \{\tilde{c}_t=k\} { c ~ t β = k } , indicators 1 { Ο j β€ t } \mathbf{1}_{\{\tau_j\le t\}} 1 { Ο j β β€ t } β identically 1 1 1 ), hence composes measurably by the composition lemma ; the countable sum over k k k of the indicator-multiplied values is then F t s y s \mathcal{F}^{\mathrm{sys}}_t F t sys β -measurable, and off Ξ© 0 \Omega_0 Ξ© 0 β the modification is absorbed because F t s y s \mathcal{F}^{\mathrm{sys}}_t F t sys β contains all null events (solution definition ). So Ξ΅ t = s t β s ^ t N \varepsilon_t=\mathfrak{s}_t-\hat{\mathfrak{s}}^N_t Ξ΅ t β = s t β β s ^ t N β is F t s y s \mathcal{F}^{\mathrm{sys}}_t F t sys β -measurable. Product-measurability of 1 Ξ© 0 Ξ΅ Ξ³ \mathbf{1}_{\Omega_0}\varepsilon^\gamma 1 Ξ© 0 β β Ξ΅ Ξ³ holds because 1 Ξ© 0 s Ξ³ \mathbf{1}_{\Omega_0}\mathfrak{s}^\gamma 1 Ξ© 0 β β s Ξ³ is product-measurable (joint measurability lemma , as in Step 0 of the published proof of the weighted second-moment lemma ) and 1 Ξ© 0 s ^ N , Ξ³ \mathbf{1}_{\Omega_0}\hat{\mathfrak{s}}^{N,\gamma} 1 Ξ© 0 β β s ^ N , Ξ³ is product-measurable by conclusion 4(c) of the policy lemma. Moments: β£ Ξ΅ t β£ β€ 2 N + C β ( N 1 / 2 + N β 1 / 2 Ξ T ) |\varepsilon_t|\le2\sqrt{N}+C^\circ(N^{1/2}+N^{-1/2}\Xi_T) β£ Ξ΅ t β β£ β€ 2 N β + C β ( N 1/2 + N β 1/2 Ξ T β ) almost surely, so E [ β£ Ξ΅ t β£ p ] < β \mathbb{E}[|\varepsilon_t|^p]<\infty E [ β£ Ξ΅ t β β£ p ] < β for all p p p , uniformly in t t t ; Ξ t N , Ξ³ Ξ΄ \Pi^{N,\gamma\delta}_t Ξ t N , Ξ³ Ξ΄ β is then finite, symmetric by commutativity, measurable in t t t by the Fubini theorem (bounded-by-integrable product-measurable integrand 1 Ξ© 0 Ξ΅ Ξ³ Ξ΅ Ξ΄ \mathbf{1}_{\Omega_0}\varepsilon^\gamma\varepsilon^\delta 1 Ξ© 0 β β Ξ΅ Ξ³ Ξ΅ Ξ΄ ), and bounded in t t t by the uniform moment bound; s ^ 0 N = 0 \hat{\mathfrak{s}}^N_0=0 s ^ 0 N β = 0 (conclusion 4(a)) gives Ξ΅ 0 = s 0 \varepsilon_0=\mathfrak{s}_0 Ξ΅ 0 β = s 0 β on Ξ© 0 \Omega_0 Ξ© 0 β , hence Ξ 0 N , Ξ³ Ξ΄ = E [ s 0 Ξ³ s 0 Ξ΄ ] \Pi^{N,\gamma\delta}_0=\mathbb{E}[\mathfrak{s}^\gamma_0\mathfrak{s}^\delta_0] Ξ 0 N , Ξ³ Ξ΄ β = E [ s 0 Ξ³ β s 0 Ξ΄ β ] .
Step 2: part (b). Let Ξ© 1 \Omega_1 Ξ© 1 β be the intersection of Ξ© 0 \Omega_0 Ξ© 0 β , the event Ξ© a \Omega_{\mathfrak{a}} Ξ© a β of clause (b) of the state residual lemma , and the almost-sure event of clause (a) of the martingale decomposition ; P ( Ξ© 1 ) = 1 \mathbb{P}(\Omega_1)=1 P ( Ξ© 1 β ) = 1 . Fix Ο β Ξ© 1 \omega\in\Omega_1 Ο β Ξ© 1 β and t β [ 0 , T ] t\in[0,T] t β [ 0 , T ] . Clause (c) of the state residual lemma (with E s = E s E_s=\mathcal{E}_s E s β = E s β , B s = B s \mathsf{B}_s=\mathcal{B}_s B s β = B s β as noted in the statement) gives
s t = s 0 + β« [ 0 , t ] ( E r s r + B r a r + e r ) β d r + N β M t , \mathfrak{s}_t=\mathfrak{s}_0+\int_{[0,t]}\big(\mathcal{E}_r\mathfrak{s}_r+\mathcal{B}_r\mathfrak{a}_r+e_r\big)\,dr+\sqrt{N}\,M_t, s t β = s 0 β + β« [ 0 , t ] β ( E r β s r β + B r β a r β + e r β ) d r + N β M t β ,
all integrals existing componentwise at Ο \omega Ο (the e e e -integral by clause (b) of that lemma, the others having bounded integrands on Ξ© 0 \Omega_0 Ξ© 0 β ). Conclusion 4(b) of the policy lemma gives
s ^ t N = β« [ 0 , t ] ( E r s ^ r N β B r G r s ^ r N β K ~ r ( N 1 / 2 b ~ ( S r ) + E ~ r s ^ r N ) ) β d r + J t K ~ , \hat{\mathfrak{s}}^N_t=\int_{[0,t]}\Big(\mathcal{E}_r\hat{\mathfrak{s}}^N_r-\mathcal{B}_r\mathcal{G}_r\hat{\mathfrak{s}}^N_r-\tilde{\mathcal{K}}_r\big(N^{1/2}\tilde{b}(S_r)+\tilde{\mathcal{E}}_r\hat{\mathfrak{s}}^N_r\big)\Big)\,dr+J^{\tilde{\mathcal{K}}}_t, s ^ t N β = β« [ 0 , t ] β ( E r β s ^ r N β β B r β G r β s ^ r N β β K ~ r β ( N 1/2 b ~ ( S r β ) + E ~ r β s ^ r N β ) ) d r + J t K ~ β ,
where the jump sum of that conclusion is exactly the weighted observation sum J t K ~ J^{\tilde{\mathcal{K}}}_t J t K ~ β with weight K ~ \tilde{\mathcal{K}} K ~ . By the definition of the weighted compensated sum, J t K ~ = J ~ t + N 1 / 2 β« [ 0 , t ] K ~ r b ~ ( Ξ£ r ) β d r J^{\tilde{\mathcal{K}}}_t=\tilde{J}_t+N^{1/2}\int_{[0,t]}\tilde{\mathcal{K}}_r\tilde{b}(\Sigma_r)\,dr J t K ~ β = J ~ t β + N 1/2 β« [ 0 , t ] β K ~ r β b ~ ( Ξ£ r β ) d r . Subtracting the two displays, the two control terms no longer cancel but combine into the clamp remainder: by conclusion 4(a) of the policy lemma, a r = β Ο r β G r s ^ r N \mathfrak{a}_r=-\chi_r\,\mathcal{G}_r\hat{\mathfrak{s}}^N_r a r β = β Ο r β G r β s ^ r N β at every point of Ξ© 0 Γ [ 0 , T ] \Omega_0\times[0,T] Ξ© 0 β Γ [ 0 , T ] , so
B r a r β ( β B r G r s ^ r N ) = ( 1 β Ο r ) β B r G r s ^ r N = w r , \mathcal{B}_r\mathfrak{a}_r-\big(-\mathcal{B}_r\mathcal{G}_r\hat{\mathfrak{s}}^N_r\big)=(1-\chi_r)\,\mathcal{B}_r\mathcal{G}_r\hat{\mathfrak{s}}^N_r=w_r , B r β a r β β ( β B r β G r β s ^ r N β ) = ( 1 β Ο r β ) B r β G r β s ^ r N β = w r β ,
which vanishes at every point at which the clamp is inactive. Hence, with g ~ r = N ( b ~ ( Ξ£ r ) β b ~ ( S r ) ) \tilde{g}_r=\sqrt{N}(\tilde{b}(\Sigma_r)-\tilde{b}(S_r)) g ~ β r β = N β ( b ~ ( Ξ£ r β ) β b ~ ( S r β )) ,
Ξ΅ t = s 0 + β« [ 0 , t ] ( E r Ξ΅ r + e r + w r + K ~ r E ~ r s ^ r N β K ~ r g ~ r ) β d r + N β M t β J ~ t , \varepsilon_t=\mathfrak{s}_0+\int_{[0,t]}\Big(\mathcal{E}_r\varepsilon_r+e_r+w_r+\tilde{\mathcal{K}}_r\tilde{\mathcal{E}}_r\hat{\mathfrak{s}}^N_r-\tilde{\mathcal{K}}_r\tilde{g}_r\Big)\,dr+\sqrt{N}\,M_t-\tilde{J}_t, Ξ΅ t β = s 0 β + β« [ 0 , t ] β ( E r β Ξ΅ r β + e r β + w r β + K ~ r β E ~ r β s ^ r N β β K ~ r β g ~ β r β ) d r + N β M t β β J ~ t β ,
using the linearity of the Lebesgue integral (each summand separately integrable at Ο \omega Ο ). By the definition of the observation linearization residual , g ~ r = E ~ r s r + e ~ r \tilde{g}_r=\tilde{\mathcal{E}}_r\mathfrak{s}_r+\tilde{e}_r g ~ β r β = E ~ r β s r β + e ~ r β pointwise, so K ~ r E ~ r s ^ r N β K ~ r g ~ r = β K ~ r E ~ r Ξ΅ r β K ~ r e ~ r \tilde{\mathcal{K}}_r\tilde{\mathcal{E}}_r\hat{\mathfrak{s}}^N_r-\tilde{\mathcal{K}}_r\tilde{g}_r=-\tilde{\mathcal{K}}_r\tilde{\mathcal{E}}_r\varepsilon_r-\tilde{\mathcal{K}}_r\tilde{e}_r K ~ r β E ~ r β s ^ r N β β K ~ r β g ~ β r β = β K ~ r β E ~ r β Ξ΅ r β β K ~ r β e ~ r β , which yields the display of (b) on Ξ© 1 \Omega_1 Ξ© 1 β .
Step 3: part (c). Write v r = ( E r β K ~ r E ~ r ) Ξ΅ r + e r β K ~ r e ~ r + w r v_r=(\mathcal{E}_r-\tilde{\mathcal{K}}_r\tilde{\mathcal{E}}_r)\varepsilon_r+e_r-\tilde{\mathcal{K}}_r\tilde{e}_r+w_r v r β = ( E r β β K ~ r β E ~ r β ) Ξ΅ r β + e r β β K ~ r β e ~ r β + w r β and m t = N M t m_t=\sqrt{N}M_t m t β = N β M t β , and define V t = β« [ 0 , t ] v r β d r V_t=\int_{[0,t]}v_r\,dr V t β = β« [ 0 , t ] β v r β d r componentwise at each Ο β Ξ© 1 \omega\in\Omega_1 Ο β Ξ© 1 β and V t = 0 V_t=0 V t β = 0 off Ξ© 1 \Omega_1 Ξ© 1 β ; each V t Ξ³ V^\gamma_t V t Ξ³ β is a random variable by the Tonelli theorem applied to the positive and negative parts of 1 Ξ© 1 v Ξ³ \mathbf{1}_{\Omega_1}v^\gamma 1 Ξ© 1 β β v Ξ³ , which is product-measurable: 1 Ξ© 0 e Ξ³ \mathbf{1}_{\Omega_0}e^\gamma 1 Ξ© 0 β β e Ξ³ and 1 Ξ© 0 e ~ Ο
\mathbf{1}_{\Omega_0}\tilde{e}^\upsilon 1 Ξ© 0 β β e ~ Ο
are product-measurable by clause (b) of the state and observation residual lemmas, 1 Ξ© 0 Ξ΅ Ξ³ \mathbf{1}_{\Omega_0}\varepsilon^\gamma 1 Ξ© 0 β β Ξ΅ Ξ³ by Step 1, and 1 Ξ© 0 w Ξ³ \mathbf{1}_{\Omega_0}w^\gamma 1 Ξ© 0 β β w Ξ³ because w r = B r a r + B r G r s ^ r N w_r=\mathcal{B}_r\mathfrak{a}_r+\mathcal{B}_r\mathcal{G}_r\hat{\mathfrak{s}}^N_r w r β = B r β a r β + B r β G r β s ^ r N β on Ξ© 0 \Omega_0 Ξ© 0 β by Step 2, where 1 Ξ© 0 a j = N β 1 Ξ© 0 ( Ξ± j β A j ) \mathbf{1}_{\Omega_0}\mathfrak{a}^j=\sqrt{N}\,\mathbf{1}_{\Omega_0}(\alpha^j-A^j) 1 Ξ© 0 β β a j = N β 1 Ξ© 0 β β ( Ξ± j β A j ) is product-measurable by part (c) of the joint measurability lemma (the components of A A A being continuous) and 1 Ξ© 0 s ^ N , Ξ³ \mathbf{1}_{\Omega_0}\hat{\mathfrak{s}}^{N,\gamma} 1 Ξ© 0 β β s ^ N , Ξ³ by conclusion 4(c) of the policy lemma; the coefficients are continuous in r r r , and products with the measurable 1 Ξ© 1 \mathbf{1}_{\Omega_1} 1 Ξ© 1 β β preserve product-measurability (composition lemma ). By Step 2, almost surely Ξ΅ t = Ξ΅ 0 + V t + m t β J ~ t \varepsilon_t=\varepsilon_0+V_t+m_t-\tilde{J}_t Ξ΅ t β = Ξ΅ 0 β + V t β + m t β β J ~ t β for all t t t , with Ξ΅ 0 = s 0 \varepsilon_0=\mathfrak{s}_0 Ξ΅ 0 β = s 0 β . Moreover v r v_r v r β is F r s y s \mathcal{F}^{\mathrm{sys}}_r F r sys β -measurable up to modification on a null event (Step 1 for Ξ΅ r \varepsilon_r Ξ΅ r β ; e r = g r β E r s r β B r a r e_r=g_r-\mathcal{E}_r\mathfrak{s}_r-\mathcal{B}_r\mathfrak{a}_r e r β = g r β β E r β s r β β B r β a r β , with g r = N ( b ( Ξ£ r , Ξ± r ) β b ( S r , A r ) ) g_r=\sqrt{N}(b(\Sigma_r,\alpha_r)-b(S_r,A_r)) g r β = N β ( b ( Ξ£ r β , Ξ± r β ) β b ( S r β , A r β )) for the aggregate state drift b b b of Ξ² \beta Ξ² (unrelated to the operator bound b β b^* b β above), as in the state residual lemma , and e ~ r = g ~ r β E ~ r s r \tilde{e}_r=\tilde{g}_r-\tilde{\mathcal{E}}_r\mathfrak{s}_r e ~ r β = g ~ β r β β E ~ r β s r β are compositions of continuous maps with the adapted Ξ£ r \Sigma_r Ξ£ r β , Ξ± r \alpha_r Ξ± r β from part (iv) of the existence theorem ), and sup β‘ r E [ ( v r Ξ³ ) 2 ] < β \sup_r\mathbb{E}[(v^\gamma_r)^2]<\infty sup r β E [( v r Ξ³ β ) 2 ] < β by Step 1 and the linear residual bounds (β£ v r β£ β€ c β β£ Ξ΅ r β£ + 2 Ξ β£ z r β£ + 2 k β Ξ ~ β£ s r β£ + b β g β β£ s ^ r N β£ |v_r|\le c^*|\varepsilon_r|+2\Lambda|z_r|+2k^*\tilde{\Lambda}|\mathfrak{s}_r|+b^*g^*|\hat{\mathfrak{s}}^N_r| β£ v r β β£ β€ c β β£ Ξ΅ r β β£ + 2Ξβ£ z r β β£ + 2 k β Ξ ~ β£ s r β β£ + b β g β β£ s ^ r N β β£ , using β£ w r β£ β€ b β g β β£ s ^ r N β£ |w_r|\le b^*g^*|\hat{\mathfrak{s}}^N_r| β£ w r β β£ β€ b β g β β£ s ^ r N β β£ since 1 β Ο r β { 0 , 1 } 1-\chi_r\in\{0,1\} 1 β Ο r β β { 0 , 1 } , and β£ z r β£ β€ β£ s r β£ + β£ a r β£ |z_r|\le|\mathfrak{s}_r|+|\mathfrak{a}_r| β£ z r β β£ β€ β£ s r β β£ + β£ a r β β£ has uniformly bounded second moments for the fixed N N N ).
We record four facts, for 0 β€ s β€ t β€ T 0\le s\le t\le T 0 β€ s β€ t β€ T and all indices. (3a) If X X X is square-integrable and F s s y s \mathcal{F}^{\mathrm{sys}}_s F s sys β -measurable then E [ X ( m t Ξ΄ β m s Ξ΄ ) ] = 0 \mathbb{E}[X(m^\delta_t-m^\delta_s)]=0 E [ X ( m t Ξ΄ β β m s Ξ΄ β )] = 0 and E [ X ( J ~ t Ξ΄ β J ~ s Ξ΄ ) ] = 0 \mathbb{E}[X(\tilde{J}^\delta_t-\tilde{J}^\delta_s)]=0 E [ X ( J ~ t Ξ΄ β β J ~ s Ξ΄ β )] = 0 : the second is part (b) of the weighted-sums lemma ; for the first, part (c) of the counter moment lemma gives, almost surely, N M u Ξ΄ = β Ο β Ξ΄ ( M u Ο Ξ΄ β M u Ξ΄ Ο ) N M^\delta_u=\sum_{\sigma\neq\delta}(\mathfrak{M}^{\sigma\delta}_u-\mathfrak{M}^{\delta\sigma}_u) N M u Ξ΄ β = β Ο ξ = Ξ΄ β ( M u Ο Ξ΄ β β M u Ξ΄ Ο β ) for all u u u , with M Ο Ξ΄ = β i M i , Ο Ξ΄ \mathfrak{M}^{\sigma\delta}=\sum_iM^{i,\sigma\delta} M Ο Ξ΄ = β i β M i , Ο Ξ΄ the aggregate compensated counters, so the claim follows from part (a) of the multiplier lemma applied per clock label and linearity. (3b) E [ m t Ξ³ m t Ξ΄ ] = β« [ 0 , t ] E [ Ξ Ξ³ Ξ΄ ( Ξ£ s , Ξ± s ) ] β d s \mathbb{E}[m^\gamma_tm^\delta_t]=\int_{[0,t]}\mathbb{E}[\Theta^{\gamma\delta}(\Sigma_s,\alpha_s)]\,ds E [ m t Ξ³ β m t Ξ΄ β ] = β« [ 0 , t ] β E [ Ξ Ξ³ Ξ΄ ( Ξ£ s β , Ξ± s β )] d s : part (c) of the martingale decomposition with r = 0 r=0 r = 0 , D = Ξ© D=\Omega D = Ξ© , multiplied by N N N , followed by the Fubini theorem for the bounded product-measurable integrand (as in fact (1d) of the published proof of the weighted second-moment lemma ). (3c) E [ J ~ t Ξ³ J ~ t Ξ΄ ] = β« [ 0 , t ] β Ο
K ~ s Ξ³ Ο
K ~ s Ξ΄ Ο
β E [ b ~ Ο
( Ξ£ s ) ] β d s \mathbb{E}[\tilde{J}^\gamma_t\tilde{J}^\delta_t]=\int_{[0,t]}\sum_\upsilon\tilde{\mathcal{K}}^{\gamma\upsilon}_s\tilde{\mathcal{K}}^{\delta\upsilon}_s\,\mathbb{E}[\tilde{b}^\upsilon(\Sigma_s)]\,ds E [ J ~ t Ξ³ β J ~ t Ξ΄ β ] = β« [ 0 , t ] β β Ο
β K ~ s Ξ³ Ο
β K ~ s Ξ΄ Ο
β E [ b ~ Ο
( Ξ£ s β )] d s : part (c) of the weighted-sums lemma with Z = 1 Z=1 Z = 1 , r = 0 r=0 r = 0 , F = G = K ~ F=G=\tilde{\mathcal{K}} F = G = K ~ , followed by Fubini (the integrand bounded and product-measurable by its part (a)); the expectations E [ b ~ Ο
( Ξ£ s ) ] \mathbb{E}[\tilde{b}^\upsilon(\Sigma_s)] E [ b ~ Ο
( Ξ£ s β )] are bounded and measurable in s s s by part (a) of the decomposition theorem and Fubini. (3d) E [ m t Ξ³ J ~ t Ξ΄ ] = 0 \mathbb{E}[m^\gamma_t\tilde{J}^\delta_t]=0 E [ m t Ξ³ β J ~ t Ξ΄ β ] = 0 : part (d) of the weighted-sums lemma with Z = 1 Z=1 Z = 1 , r = 0 r=0 r = 0 (m 0 = J ~ 0 = 0 m_0=\tilde{J}_0=0 m 0 β = J ~ 0 β = 0 almost surely).
Now expand E [ Ξ΅ t Ξ³ Ξ΅ t Ξ΄ ] \mathbb{E}[\varepsilon^\gamma_t\varepsilon^\delta_t] E [ Ξ΅ t Ξ³ β Ξ΅ t Ξ΄ β ] using the four-term representation; all sixteen products are integrable (every factor lies in every mean-square space by Step 1, part (a) of the weighted-sums lemma, the boundedness of M Ξ³ M^\gamma M Ξ³ on Ξ© 0 \Omega_0 Ξ© 0 β , and β£ V t β£ β€ β« [ 0 , T ] β£ v r β£ d r |V_t|\le\int_{[0,T]}|v_r|dr β£ V t β β£ β€ β« [ 0 , T ] β β£ v r β β£ d r with E [ ( β« β£ v β£ ) 2 ] β€ T β« E β£ v r β£ 2 d r < β \mathbb{E}[(\int|v|)^2]\le T\int\mathbb{E}|v_r|^2dr<\infty E [( β« β£ v β£ ) 2 ] β€ T β« E β£ v r β β£ 2 d r < β by the Cauchy-Schwarz inequality and Tonelli ). The terms E [ Ξ΅ 0 Ξ³ m t Ξ΄ ] \mathbb{E}[\varepsilon^\gamma_0m^\delta_t] E [ Ξ΅ 0 Ξ³ β m t Ξ΄ β ] , E [ Ξ΅ 0 Ξ³ J ~ t Ξ΄ ] \mathbb{E}[\varepsilon^\gamma_0\tilde{J}^\delta_t] E [ Ξ΅ 0 Ξ³ β J ~ t Ξ΄ β ] and their mirrors vanish by (3a) with s = 0 s=0 s = 0 (Ξ΅ 0 = s 0 \varepsilon_0=\mathfrak{s}_0 Ξ΅ 0 β = s 0 β bounded and F 0 s y s \mathcal{F}^{\mathrm{sys}}_0 F 0 sys β -measurable). Next: E [ Ξ΅ 0 Ξ³ V t Ξ΄ ] = β« [ 0 , t ] E [ Ξ΅ 0 Ξ³ v s Ξ΄ ] d s \mathbb{E}[\varepsilon^\gamma_0V^\delta_t]=\int_{[0,t]}\mathbb{E}[\varepsilon^\gamma_0v^\delta_s]ds E [ Ξ΅ 0 Ξ³ β V t Ξ΄ β ] = β« [ 0 , t ] β E [ Ξ΅ 0 Ξ³ β v s Ξ΄ β ] d s by Fubini (dominated by 2 N β 1 Ξ© 1 β£ v s Ξ΄ β£ 2\sqrt{N}\,\mathbf{1}_{\Omega_1}|v^\delta_s| 2 N β 1 Ξ© 1 β β β£ v s Ξ΄ β β£ ). Pathwise on Ξ© 1 \Omega_1 Ξ© 1 β , the integration by parts lemma with u 0 = v 0 = 0 u_0=v_0=0 u 0 β = v 0 β = 0 gives V t Ξ³ V t Ξ΄ = β« [ 0 , t ] ( v s Ξ³ V s Ξ΄ + V s Ξ³ v s Ξ΄ ) d s V^\gamma_tV^\delta_t=\int_{[0,t]}(v^\gamma_sV^\delta_s+V^\gamma_sv^\delta_s)ds V t Ξ³ β V t Ξ΄ β = β« [ 0 , t ] β ( v s Ξ³ β V s Ξ΄ β + V s Ξ³ β v s Ξ΄ β ) d s , so E [ V t Ξ³ V t Ξ΄ ] = β« [ 0 , t ] E [ v s Ξ³ V s Ξ΄ + V s Ξ³ v s Ξ΄ ] d s \mathbb{E}[V^\gamma_tV^\delta_t]=\int_{[0,t]}\mathbb{E}[v^\gamma_sV^\delta_s+V^\gamma_sv^\delta_s]ds E [ V t Ξ³ β V t Ξ΄ β ] = β« [ 0 , t ] β E [ v s Ξ³ β V s Ξ΄ β + V s Ξ³ β v s Ξ΄ β ] d s by Fubini (dominated by β£ v s β£ β
β« [ 0 , T ] β£ v r β£ d r |v_s|\cdot\int_{[0,T]}|v_r|dr β£ v s β β£ β
β« [ 0 , T ] β β£ v r β β£ d r , integrable on the product as just noted). Pathwise V t Ξ³ m t Ξ΄ = β« [ 0 , t ] v s Ξ³ β m t Ξ΄ β d s V^\gamma_tm^\delta_t=\int_{[0,t]}v^\gamma_s\,m^\delta_t\,ds V t Ξ³ β m t Ξ΄ β = β« [ 0 , t ] β v s Ξ³ β m t Ξ΄ β d s , so by Fubini (domination by 1 Ξ© 1 β£ v s Ξ³ β£ β£ m t Ξ΄ β£ \mathbf{1}_{\Omega_1}|v^\gamma_s||m^\delta_t| 1 Ξ© 1 β β β£ v s Ξ³ β β£β£ m t Ξ΄ β β£ , integrable on the product by Cauchy-Schwarz) and (3a) with X = v s Ξ³ X=v^\gamma_s X = v s Ξ³ β ,
E [ V t Ξ³ m t Ξ΄ ] = β« [ 0 , t ] E [ v s Ξ³ β m t Ξ΄ ] β d s = β« [ 0 , t ] E [ v s Ξ³ β m s Ξ΄ ] β d s , \mathbb{E}[V^\gamma_tm^\delta_t]=\int_{[0,t]}\mathbb{E}[v^\gamma_s\,m^\delta_t]\,ds=\int_{[0,t]}\mathbb{E}[v^\gamma_s\,m^\delta_s]\,ds, E [ V t Ξ³ β m t Ξ΄ β ] = β« [ 0 , t ] β E [ v s Ξ³ β m t Ξ΄ β ] d s = β« [ 0 , t ] β E [ v s Ξ³ β m s Ξ΄ β ] d s ,
and identically E [ V t Ξ³ J ~ t Ξ΄ ] = β« [ 0 , t ] E [ v s Ξ³ J ~ s Ξ΄ ] d s \mathbb{E}[V^\gamma_t\tilde{J}^\delta_t]=\int_{[0,t]}\mathbb{E}[v^\gamma_s\tilde{J}^\delta_s]ds E [ V t Ξ³ β J ~ t Ξ΄ β ] = β« [ 0 , t ] β E [ v s Ξ³ β J ~ s Ξ΄ β ] d s (using the second identity of (3a)), with the mirrored versions for the ( Ξ΄ , Ξ³ ) (\delta,\gamma) ( Ξ΄ , Ξ³ ) pairs. Combining all terms with (3b), (3c), (3d), and re-assembling Ξ΅ s Ξ΄ = Ξ΅ 0 Ξ΄ + V s Ξ΄ + m s Ξ΄ β J ~ s Ξ΄ \varepsilon^\delta_s=\varepsilon^\delta_0+V^\delta_s+m^\delta_s-\tilde{J}^\delta_s Ξ΅ s Ξ΄ β = Ξ΅ 0 Ξ΄ β + V s Ξ΄ β + m s Ξ΄ β β J ~ s Ξ΄ β (almost surely) inside the integrands:
Ξ t N , Ξ³ Ξ΄ = Ξ 0 N , Ξ³ Ξ΄ + β« [ 0 , t ] ( E [ v s Ξ³ Ξ΅ s Ξ΄ ] + E [ Ξ΅ s Ξ³ v s Ξ΄ ] + E [ Ξ Ξ³ Ξ΄ ( Ξ£ s , Ξ± s ) ] + β Ο
K ~ s Ξ³ Ο
K ~ s Ξ΄ Ο
E [ b ~ Ο
( Ξ£ s ) ] ) d s . \Pi^{N,\gamma\delta}_t=\Pi^{N,\gamma\delta}_0+\int_{[0,t]}\Big(\mathbb{E}[v^\gamma_s\varepsilon^\delta_s]+\mathbb{E}[\varepsilon^\gamma_sv^\delta_s]+\mathbb{E}[\Theta^{\gamma\delta}(\Sigma_s,\alpha_s)]+\sum_\upsilon\tilde{\mathcal{K}}^{\gamma\upsilon}_s\tilde{\mathcal{K}}^{\delta\upsilon}_s\mathbb{E}[\tilde{b}^\upsilon(\Sigma_s)]\Big)ds . Ξ t N , Ξ³ Ξ΄ β = Ξ 0 N , Ξ³ Ξ΄ β + β« [ 0 , t ] β ( E [ v s Ξ³ β Ξ΅ s Ξ΄ β ] + E [ Ξ΅ s Ξ³ β v s Ξ΄ β ] + E [ Ξ Ξ³ Ξ΄ ( Ξ£ s β , Ξ± s β )] + Ο
β β K ~ s Ξ³ Ο
β K ~ s Ξ΄ Ο
β E [ b ~ Ο
( Ξ£ s β )] ) d s .
Finally, E [ v s Ξ³ Ξ΅ s Ξ΄ ] = β Ο ( E s β K ~ s E ~ s ) Ξ³ Ο β Ξ s N , Ο Ξ΄ + E [ ( e s β K ~ s e ~ s + w s ) Ξ³ Ξ΅ s Ξ΄ ] \mathbb{E}[v^\gamma_s\varepsilon^\delta_s]=\sum_\rho(\mathcal{E}_s-\tilde{\mathcal{K}}_s\tilde{\mathcal{E}}_s)^{\gamma\rho}\,\Pi^{N,\rho\delta}_s+\mathbb{E}[(e_s-\tilde{\mathcal{K}}_s\tilde{e}_s+w_s)^\gamma\varepsilon^\delta_s] E [ v s Ξ³ β Ξ΅ s Ξ΄ β ] = β Ο β ( E s β β K ~ s β E ~ s β ) Ξ³ Ο Ξ s N , Ο Ξ΄ β + E [( e s β β K ~ s β e ~ s β + w s β ) Ξ³ Ξ΅ s Ξ΄ β ] by linearity, and the pair of such terms produces ( ( E β K ~ E ~ ) Ξ N + Ξ N ( E β K ~ E ~ ) β€ ) Ξ³ Ξ΄ + X s Ξ³ Ξ΄ ((\mathcal{E}-\tilde{\mathcal{K}}\tilde{\mathcal{E}})\Pi^N+\Pi^N(\mathcal{E}-\tilde{\mathcal{K}}\tilde{\mathcal{E}})^{\top})^{\gamma\delta}+X^{\gamma\delta}_s (( E β K ~ E ~ ) Ξ N + Ξ N ( E β K ~ E ~ ) β€ ) Ξ³ Ξ΄ + X s Ξ³ Ξ΄ β , using the symmetry Ξ N , Ο Ξ΄ = Ξ N , Ξ΄ Ο \Pi^{N,\rho\delta}=\Pi^{N,\delta\rho} Ξ N , Ο Ξ΄ = Ξ N , Ξ΄ Ο and the transpose convention. All integrands are bounded in s s s (Step 1 moment bounds, fixed N N N ) and measurable (Fubini on the product-measurable, bounded-by-integrable modified integrands), so t β¦ Ξ t N , Ξ³ Ξ΄ t\mapsto\Pi^{N,\gamma\delta}_t t β¦ Ξ t N , Ξ³ Ξ΄ β is continuous by the absolute continuity of the Lebesgue integral . This proves (c).
Step 4: part (d). On Ξ© 0 \Omega_0 Ξ© 0 β , keeping the filter alone, conclusion 4(b) of the policy lemma β whose drift term is already β B r G r s ^ r N -\mathcal{B}_r\mathcal{G}_r\hat{\mathfrak{s}}^N_r β B r β G r β s ^ r N β , so that no appeal to the control identity is needed here and the clamp does not enter β together with J t K ~ = J ~ t + N 1 / 2 β« [ 0 , t ] K ~ r b ~ ( Ξ£ r ) d r J^{\tilde{\mathcal{K}}}_t=\tilde{J}_t+N^{1/2}\int_{[0,t]}\tilde{\mathcal{K}}_r\tilde{b}(\Sigma_r)dr J t K ~ β = J ~ t β + N 1/2 β« [ 0 , t ] β K ~ r β b ~ ( Ξ£ r β ) d r gives, pathwise on Ξ© 0 \Omega_0 Ξ© 0 β , for all t t t :
s ^ t N = β« [ 0 , t ] ( M r β s ^ r N + K ~ r β g ~ r ) β d r + J ~ t , g ~ r = N ( b ~ ( Ξ£ r ) β b ~ ( S r ) ) , \hat{\mathfrak{s}}^N_t=\int_{[0,t]}\big(\mathcal{M}_r\,\hat{\mathfrak{s}}^N_r+\tilde{\mathcal{K}}_r\,\tilde{g}_r\big)\,dr+\tilde{J}_t,\qquad \tilde{g}_r=\sqrt{N}\big(\tilde{b}(\Sigma_r)-\tilde{b}(S_r)\big), s ^ t N β = β« [ 0 , t ] β ( M r β s ^ r N β + K ~ r β g ~ β r β ) d r + J ~ t β , g ~ β r β = N β ( b ~ ( Ξ£ r β ) β b ~ ( S r β ) ) ,
with M r \mathcal{M}_r M r β the closed-loop matrix (as renamed above). By parts (i) and (ii) of the observation drift regularity lemma (restriction to the simplex and the Lipschitz bound, with d ( Ξ£ r , S r ) = N β 1 / 2 β£ s r β£ d(\Sigma_r,S_r)=N^{-1/2}|\mathfrak{s}_r| d ( Ξ£ r β , S r β ) = N β 1/2 β£ s r β β£ ), β£ g ~ r β£ β€ l ~ β l β ( B ~ + K ~ ) β β£ s r β£ = Ξ ~ β£ s r β£ |\tilde{g}_r|\le\sqrt{\tilde{l}}\,\sqrt{l}\,(\tilde{B}+\tilde{K})\,|\mathfrak{s}_r|=\tilde{\Lambda}|\mathfrak{s}_r| β£ g ~ β r β β£ β€ l ~ β l β ( B ~ + K ~ ) β£ s r β β£ = Ξ ~ β£ s r β β£ . For a componentwise integral: for t = 0 t=0 t = 0 the bound ( β« [ 0 , 0 ] f ) 4 β€ 0 = t 3 β« [ 0 , 0 ] f 4 (\int_{[0,0]}f)^4\le0=t^3\int_{[0,0]}f^4 ( β« [ 0 , 0 ] β f ) 4 β€ 0 = t 3 β« [ 0 , 0 ] β f 4 is trivial; for t β ( 0 , T ] t\in(0,T] t β ( 0 , T ] , claim 4 of the toolkit (with a = 0 < b = t a=0<b=t a = 0 < b = t and g = 1 g=1 g = 1 ) gives ( β« [ 0 , t ] f ) 2 β€ t β« [ 0 , t ] f 2 (\int_{[0,t]}f)^2\le t\int_{[0,t]}f^2 ( β« [ 0 , t ] β f ) 2 β€ t β« [ 0 , t ] β f 2 for measurable f β₯ 0 f\ge0 f β₯ 0 with β« [ 0 , t ] f 2 < β \int_{[0,t]}f^2<\infty β« [ 0 , t ] β f 2 < β ; applying this once to f f f and once to f 2 f^2 f 2 in place of f f f (valid for the bounded integrands used below, which have finite fourth moments) gives ( β« [ 0 , t ] f 2 ) 2 β€ t β« [ 0 , t ] f 4 (\int_{[0,t]}f^2)^2\le t\int_{[0,t]}f^4 ( β« [ 0 , t ] β f 2 ) 2 β€ t β« [ 0 , t ] β f 4 , so ( β« [ 0 , t ] f ) 4 = ( ( β« [ 0 , t ] f ) 2 ) 2 β€ ( t β« [ 0 , t ] f 2 ) 2 = t 2 ( β« [ 0 , t ] f 2 ) 2 β€ t 2 β
t β« [ 0 , t ] f 4 = t 3 β« [ 0 , t ] f 4 (\int_{[0,t]}f)^4=\big((\int_{[0,t]}f)^2\big)^2\le\big(t\int_{[0,t]}f^2\big)^2=t^2\big(\int_{[0,t]}f^2\big)^2\le t^2\cdot t\int_{[0,t]}f^4=t^3\int_{[0,t]}f^4 ( β« [ 0 , t ] β f ) 4 = ( ( β« [ 0 , t ] β f ) 2 ) 2 β€ ( t β« [ 0 , t ] β f 2 ) 2 = t 2 ( β« [ 0 , t ] β f 2 ) 2 β€ t 2 β
t β« [ 0 , t ] β f 4 = t 3 β« [ 0 , t ] β f 4 ; together with ( a + b + c ) 4 β€ 27 ( a 4 + b 4 + c 4 ) (a+b+c)^4\le27(a^4+b^4+c^4) ( a + b + c ) 4 β€ 27 ( a 4 + b 4 + c 4 ) ; hence, on Ξ© 0 \Omega_0 Ξ© 0 β ,
β£ s ^ t N β£ 4 Β β€ Β 27 β T 3 β ( c M β ) 4 β« [ 0 , t ] β£ s ^ r N β£ 4 d r + 27 β T 3 β ( k β Ξ ~ ) 4 β« [ 0 , t ] β£ s r β£ 4 d r + 27 β β£ J ~ t β£ 4 . |\hat{\mathfrak{s}}^N_t|^4\ \le\ 27\,T^3\,(c^*_{\mathcal{M}})^4\int_{[0,t]}|\hat{\mathfrak{s}}^N_r|^4dr+27\,T^3\,(k^*\tilde{\Lambda})^4\int_{[0,t]}|\mathfrak{s}_r|^4dr+27\,|\tilde{J}_t|^4 . β£ s ^ t N β β£ 4 Β β€ Β 27 T 3 ( c M β β ) 4 β« [ 0 , t ] β β£ s ^ r N β β£ 4 d r + 27 T 3 ( k β Ξ ~ ) 4 β« [ 0 , t ] β β£ s r β β£ 4 d r + 27 β£ J ~ t β β£ 4 .
Taking expectations (Tonelli, the integrands product-measurable as in Steps 1 and 3) and using E [ β£ J ~ t β£ 4 ] β€ l β Ξ³ E [ ( J ~ t Ξ³ ) 4 ] β€ 11 β l 2 ( 1 + C K ~ ) 4 ( 1 + l ~ B ~ T ) 2 = : c 7 \mathbb{E}[|\tilde{J}_t|^4]\le l\sum_\gamma\mathbb{E}[(\tilde{J}^\gamma_t)^4]\le11\,l^2(1+C_{\tilde{K}})^4(1+\tilde{l}\tilde{B}T)^2=:c_7 E [ β£ J ~ t β β£ 4 ] β€ l β Ξ³ β E [( J ~ t Ξ³ β ) 4 ] β€ 11 l 2 ( 1 + C K ~ β ) 4 ( 1 + l ~ B ~ T ) 2 =: c 7 β by part (e) of the weighted-sums lemma ,
E [ β£ s ^ t N β£ 4 ] β€ 27 T 3 ( c M β ) 4 β« [ 0 , t ] E [ β£ s ^ r N β£ 4 ] d r + 27 T 3 ( k β Ξ ~ ) 4 β« [ 0 , t ] E [ β£ s r β£ 4 ] d r + 27 c 7 . \mathbb{E}[|\hat{\mathfrak{s}}^N_t|^4]\le27T^3(c^*_{\mathcal{M}})^4\int_{[0,t]}\mathbb{E}[|\hat{\mathfrak{s}}^N_r|^4]dr+27T^3(k^*\tilde{\Lambda})^4\int_{[0,t]}\mathbb{E}[|\mathfrak{s}_r|^4]dr+27c_7 . E [ β£ s ^ t N β β£ 4 ] β€ 27 T 3 ( c M β β ) 4 β« [ 0 , t ] β E [ β£ s ^ r N β β£ 4 ] d r + 27 T 3 ( k β Ξ ~ ) 4 β« [ 0 , t ] β E [ β£ s r β β£ 4 ] d r + 27 c 7 β .
Part (b) of the fourth-moment bound , together with β£ a r β£ = Ο r β£ G r s ^ r N β£ β€ g β β£ s ^ r N β£ |\mathfrak{a}_r|=\chi_r|\mathcal{G}_r\hat{\mathfrak{s}}^N_r|\le g^*|\hat{\mathfrak{s}}^N_r| β£ a r β β£ = Ο r β β£ G r β s ^ r N β β£ β€ g β β£ s ^ r N β β£ (so E [ β£ a r β£ 4 ] β€ ( g β ) 4 E [ β£ s ^ r N β£ 4 ] \mathbb{E}[|\mathfrak{a}_r|^4]\le(g^*)^4\mathbb{E}[|\hat{\mathfrak{s}}^N_r|^4] E [ β£ a r β β£ 4 ] β€ ( g β ) 4 E [ β£ s ^ r N β β£ 4 ] ), gives, with c M β² = 6 l 2 ( 2 ( l β 1 ) ) 4 c_{M'}=6l^2(2(l-1))^4 c M β² β = 6 l 2 ( 2 ( l β 1 ) ) 4 ,
E [ β£ s t β£ 4 ] β€ 27 β E [ β£ s 0 β£ 4 ] + 27 c M β² ( B T + ( B T ) 2 ) + 54 T 3 Ξ 4 β« [ 0 , t ] ( E [ β£ s r β£ 4 ] + ( g β ) 4 E [ β£ s ^ r N β£ 4 ] ) d r . \mathbb{E}[|\mathfrak{s}_t|^4]\le27\,\mathbb{E}[|\mathfrak{s}_0|^4]+27c_{M'}(BT+(BT)^2)+54T^3\Lambda^4\int_{[0,t]}\Big(\mathbb{E}[|\mathfrak{s}_r|^4]+(g^*)^4\mathbb{E}[|\hat{\mathfrak{s}}^N_r|^4]\Big)dr . E [ β£ s t β β£ 4 ] β€ 27 E [ β£ s 0 β β£ 4 ] + 27 c M β² β ( BT + ( BT ) 2 ) + 54 T 3 Ξ 4 β« [ 0 , t ] β ( E [ β£ s r β β£ 4 ] + ( g β ) 4 E [ β£ s ^ r N β β£ 4 ] ) d r .
Set Ο ( t ) = E [ β£ s t β£ 4 ] + E [ β£ s ^ t N β£ 4 ] \psi(t)=\mathbb{E}[|\mathfrak{s}_t|^4]+\mathbb{E}[|\hat{\mathfrak{s}}^N_t|^4] Ο ( t ) = E [ β£ s t β β£ 4 ] + E [ β£ s ^ t N β β£ 4 ] . Adding the two displays, there are reals a β€ c 8 β ΞΊ 0 a\le c_8\,\kappa_0 a β€ c 8 β ΞΊ 0 β and b β₯ 0 b\ge0 b β₯ 0 , both determined by the data listed in (d) only (a = 27 E [ β£ s 0 β£ 4 ] + 27 c M β² ( B T + ( B T ) 2 ) + 27 c 7 β€ c 8 ΞΊ 0 a=27\mathbb{E}[|\mathfrak{s}_0|^4]+27c_{M'}(BT+(BT)^2)+27c_7\le c_8\kappa_0 a = 27 E [ β£ s 0 β β£ 4 ] + 27 c M β² β ( BT + ( BT ) 2 ) + 27 c 7 β β€ c 8 β ΞΊ 0 β ), with Ο ( t ) β€ a + b β« [ 0 , t ] Ο ( s ) d s \psi(t)\le a+b\int_{[0,t]}\psi(s)ds Ο ( t ) β€ a + b β« [ 0 , t ] β Ο ( s ) d s for all t t t . The function Ο \psi Ο is measurable (clause (a) of the fourth-moment lemma; conclusion 4(c) of the policy lemma with Tonelli) and bounded on [ 0 , T ] [0,T] [ 0 , T ] for the fixed N N N (Step 1). Let u ( t ) = β« [ 0 , t ] Ο ( s ) d s u(t)=\int_{[0,t]}\psi(s)ds u ( t ) = β« [ 0 , t ] β Ο ( s ) d s ; then u u u is continuous on [ 0 , T ] [0,T] [ 0 , T ] by the absolute continuity of the integral , and u ( t ) β€ a T + b β« [ 0 , t ] u ( s ) d s u(t)\le aT+b\int_{[0,t]}u(s)ds u ( t ) β€ a T + b β« [ 0 , t ] β u ( s ) d s by monotonicity of the integral ; since the Lebesgue and Riemann integrals of the continuous u u u agree, by claim 3 of the interval toolkit , Gronwall's lemma gives u ( t ) β€ a T exp β‘ ( b T ) u(t)\le aT\exp(bT) u ( t ) β€ a T exp ( b T ) , whence Ο ( t ) β€ a ( 1 + b T exp β‘ ( b T ) ) \psi(t)\le a(1+bT\exp(bT)) Ο ( t ) β€ a ( 1 + b T exp ( b T )) for every t t t . Since β£ Ξ΅ t β£ 4 β€ 8 ( β£ s t β£ 4 + β£ s ^ t N β£ 4 ) |\varepsilon_t|^4\le8(|\mathfrak{s}_t|^4+|\hat{\mathfrak{s}}^N_t|^4) β£ Ξ΅ t β β£ 4 β€ 8 ( β£ s t β β£ 4 + β£ s ^ t N β β£ 4 ) and β£ a t β£ 4 β€ ( g β ) 4 β£ s ^ t N β£ 4 |\mathfrak{a}_t|^4\le(g^*)^4|\hat{\mathfrak{s}}^N_t|^4 β£ a t β β£ 4 β€ ( g β ) 4 β£ s ^ t N β β£ 4 , part (d) follows with C 1 = ( 8 + ( g β ) 4 + 1 ) β c 8 β ( 1 + b T exp β‘ ( b T ) ) C_1=(8+(g^*)^4+1)\,c_8\,(1+bT\exp(bT)) C 1 β = ( 8 + ( g β ) 4 + 1 ) c 8 β ( 1 + b T exp ( b T )) ; the displayed consequences follow from E [ β£ β
β£ 2 ] β€ 1 + E [ β£ β
β£ 4 ] \mathbb{E}[|\cdot|^2]\le1+\mathbb{E}[|\cdot|^4] E [ β£ β
β£ 2 ] β€ 1 + E [ β£ β
β£ 4 ] , ΞΊ 0 β₯ 1 \kappa_0\ge1 ΞΊ 0 β β₯ 1 , and integration over [ 0 , T ] [0,T] [ 0 , T ] .
Step 5: part (e). By conclusion 2 of the policy lemma , Ξ t = Ξ 0 + β« 0 t ( E r Ξ r + Ξ r E r β€ β Ξ r D ~ r Ξ r + Ξ r β ) d r \Pi_t=\Pi_0+\int_0^t(\mathcal{E}_r\Pi_r+\Pi_r\mathcal{E}_r^{\top}-\Pi_r\tilde{D}_r\Pi_r+\Theta^\star_r)dr Ξ t β = Ξ 0 β + β« 0 t β ( E r β Ξ r β + Ξ r β E r β€ β β Ξ r β D ~ r β Ξ r β + Ξ r β β ) d r with every Ξ r \Pi_r Ξ r β symmetric. We first record the algebraic identity, for each r r r :
( E r β K ~ r E ~ r ) Ξ r + Ξ r ( E r β K ~ r E ~ r ) β€ + Ξ r β + K ~ r Ξ ~ r β K ~ r β€ = E r Ξ r + Ξ r E r β€ β Ξ r D ~ r Ξ r + Ξ r β . (\mathcal{E}_r-\tilde{\mathcal{K}}_r\tilde{\mathcal{E}}_r)\Pi_r+\Pi_r(\mathcal{E}_r-\tilde{\mathcal{K}}_r\tilde{\mathcal{E}}_r)^{\top}+\Theta^\star_r+\tilde{\mathcal{K}}_r\tilde{\Theta}^\star_r\tilde{\mathcal{K}}_r^{\top}=\mathcal{E}_r\Pi_r+\Pi_r\mathcal{E}_r^{\top}-\Pi_r\tilde{D}_r\Pi_r+\Theta^\star_r . ( E r β β K ~ r β E ~ r β ) Ξ r β + Ξ r β ( E r β β K ~ r β E ~ r β ) β€ + Ξ r β β + K ~ r β Ξ ~ r β β K ~ r β€ β = E r β Ξ r β + Ξ r β E r β€ β β Ξ r β D ~ r β Ξ r β + Ξ r β β .
Indeed, with K ~ r = Ξ r E ~ r β€ ( Ξ ~ r β ) β 1 \tilde{\mathcal{K}}_r=\Pi_r\tilde{\mathcal{E}}_r^{\top}(\tilde{\Theta}^\star_r)^{-1} K ~ r β = Ξ r β E ~ r β€ β ( Ξ ~ r β β ) β 1 , the reversal rule for the transpose , the symmetry of Ξ r \Pi_r Ξ r β and of ( Ξ ~ r β ) β 1 (\tilde{\Theta}^\star_r)^{-1} ( Ξ ~ r β β ) β 1 (a diagonal matrix, by conclusion 1 of the policy lemma): K ~ r E ~ r Ξ r = Ξ r D ~ r Ξ r \tilde{\mathcal{K}}_r\tilde{\mathcal{E}}_r\Pi_r=\Pi_r\tilde{D}_r\Pi_r K ~ r β E ~ r β Ξ r β = Ξ r β D ~ r β Ξ r β ; Ξ r ( K ~ r E ~ r ) β€ = Ξ r E ~ r β€ ( Ξ ~ r β ) β 1 E ~ r Ξ r = Ξ r D ~ r Ξ r \Pi_r(\tilde{\mathcal{K}}_r\tilde{\mathcal{E}}_r)^{\top}=\Pi_r\tilde{\mathcal{E}}_r^{\top}(\tilde{\Theta}^\star_r)^{-1}\tilde{\mathcal{E}}_r\Pi_r=\Pi_r\tilde{D}_r\Pi_r Ξ r β ( K ~ r β E ~ r β ) β€ = Ξ r β E ~ r β€ β ( Ξ ~ r β β ) β 1 E ~ r β Ξ r β = Ξ r β D ~ r β Ξ r β ; and K ~ r Ξ ~ r β K ~ r β€ = Ξ r E ~ r β€ ( Ξ ~ r β ) β 1 Ξ ~ r β ( Ξ ~ r β ) β 1 E ~ r Ξ r = Ξ r D ~ r Ξ r \tilde{\mathcal{K}}_r\tilde{\Theta}^\star_r\tilde{\mathcal{K}}_r^{\top}=\Pi_r\tilde{\mathcal{E}}_r^{\top}(\tilde{\Theta}^\star_r)^{-1}\tilde{\Theta}^\star_r(\tilde{\Theta}^\star_r)^{-1}\tilde{\mathcal{E}}_r\Pi_r=\Pi_r\tilde{D}_r\Pi_r K ~ r β Ξ ~ r β β K ~ r β€ β = Ξ r β E ~ r β€ β ( Ξ ~ r β β ) β 1 Ξ ~ r β β ( Ξ ~ r β β ) β 1 E ~ r β Ξ r β = Ξ r β D ~ r β Ξ r β , so the two sides agree, the three correction terms combining to β Ξ r D ~ r Ξ r -\Pi_r\tilde{D}_r\Pi_r β Ξ r β D ~ r β Ξ r β . By clauses 6 and 7 of the fluctuation LQG data , ( Ξ r β ) Ξ³ Ξ΄ = Ξ Ξ³ Ξ΄ ( S r , A r ) (\Theta^\star_r)^{\gamma\delta}=\Theta^{\gamma\delta}(S_r,A_r) ( Ξ r β β ) Ξ³ Ξ΄ = Ξ Ξ³ Ξ΄ ( S r β , A r β ) and ( K ~ r Ξ ~ r β K ~ r β€ ) Ξ³ Ξ΄ = β Ο
K ~ r Ξ³ Ο
K ~ r Ξ΄ Ο
β b ~ Ο
( S r ) (\tilde{\mathcal{K}}_r\tilde{\Theta}^\star_r\tilde{\mathcal{K}}_r^{\top})^{\gamma\delta}=\sum_\upsilon\tilde{\mathcal{K}}^{\gamma\upsilon}_r\tilde{\mathcal{K}}^{\delta\upsilon}_r\,\tilde{b}^\upsilon(S_r) ( K ~ r β Ξ ~ r β β K ~ r β€ β ) Ξ³ Ξ΄ = β Ο
β K ~ r Ξ³ Ο
β K ~ r Ξ΄ Ο
β b ~ Ο
( S r β ) . Subtracting the resulting integral equation for Ξ \Pi Ξ from the evolution identity of part (c) (the Riemann and Lebesgue integrals agreeing for the continuous integrand of the Riccati equation, by claim 3 of the interval toolkit ), the difference D t = Ξ t N β Ξ t D_t=\Pi^N_t-\Pi_t D t β = Ξ t N β β Ξ t β satisfies, entrywise,
D t Ξ³ Ξ΄ = D 0 Ξ³ Ξ΄ + β« [ 0 , t ] ( ( ( E β K ~ E ~ ) D + D ( E β K ~ E ~ ) β€ ) r Ξ³ Ξ΄ + X r Ξ³ Ξ΄ + Ξ r Ξ³ Ξ΄ + Ξ ~ r Ξ³ Ξ΄ ) d r , D^{\gamma\delta}_t=D^{\gamma\delta}_0+\int_{[0,t]}\Big(\big((\mathcal{E}-\tilde{\mathcal{K}}\tilde{\mathcal{E}})D+D(\mathcal{E}-\tilde{\mathcal{K}}\tilde{\mathcal{E}})^{\top}\big)^{\gamma\delta}_r+X^{\gamma\delta}_r+\Delta^{\gamma\delta}_r+\tilde{\Delta}^{\gamma\delta}_r\Big)dr, D t Ξ³ Ξ΄ β = D 0 Ξ³ Ξ΄ β + β« [ 0 , t ] β ( ( ( E β K ~ E ~ ) D + D ( E β K ~ E ~ ) β€ ) r Ξ³ Ξ΄ β + X r Ξ³ Ξ΄ β + Ξ r Ξ³ Ξ΄ β + Ξ ~ r Ξ³ Ξ΄ β ) d r ,
where Ξ r Ξ³ Ξ΄ = E [ Ξ Ξ³ Ξ΄ ( Ξ£ r , Ξ± r ) ] β Ξ Ξ³ Ξ΄ ( S r , A r ) \Delta^{\gamma\delta}_r=\mathbb{E}[\Theta^{\gamma\delta}(\Sigma_r,\alpha_r)]-\Theta^{\gamma\delta}(S_r,A_r) Ξ r Ξ³ Ξ΄ β = E [ Ξ Ξ³ Ξ΄ ( Ξ£ r β , Ξ± r β )] β Ξ Ξ³ Ξ΄ ( S r β , A r β ) and Ξ ~ r Ξ³ Ξ΄ = β Ο
K ~ r Ξ³ Ο
K ~ r Ξ΄ Ο
( E [ b ~ Ο
( Ξ£ r ) ] β b ~ Ο
( S r ) ) \tilde{\Delta}^{\gamma\delta}_r=\sum_\upsilon\tilde{\mathcal{K}}^{\gamma\upsilon}_r\tilde{\mathcal{K}}^{\delta\upsilon}_r(\mathbb{E}[\tilde{b}^\upsilon(\Sigma_r)]-\tilde{b}^\upsilon(S_r)) Ξ ~ r Ξ³ Ξ΄ β = β Ο
β K ~ r Ξ³ Ο
β K ~ r Ξ΄ Ο
β ( E [ b ~ Ο
( Ξ£ r β )] β b ~ Ο
( S r β )) . We bound the three inhomogeneous terms using part (d); write C Λ = ( 4 + C 1 ) \bar{C}=(4+C_1) C Λ = ( 4 + C 1 β ) , so all the second moments named in (d) are at most C Λ ΞΊ 0 \bar{C}\kappa_0 C Λ ΞΊ 0 β and all the fourth moments at most C 1 ΞΊ 0 C_1\kappa_0 C 1 β ΞΊ 0 β , and recall ΞΊ 0 β₯ 1 \kappa_0\ge1 ΞΊ 0 β β₯ 1 , so ΞΊ 0 1 / 2 β€ ΞΊ 0 \kappa_0^{1/2}\le\kappa_0 ΞΊ 0 1/2 β β€ ΞΊ 0 β .
Clamp remainder. We first show that the clamp is rare enough that w w w contributes at the same order as the residuals. If g β = 0 g^*=0 g β = 0 then G r s ^ r N = 0 \mathcal{G}_r\hat{\mathfrak{s}}^N_r=0 G r β s ^ r N β = 0 , so w r = 0 w_r=0 w r β = 0 and the bound below holds trivially; assume therefore g β > 0 g^*>0 g β > 0 . Measurability of the clamp indicator. By hypothesis (C) of the policy lemma the control set A \mathcal{A} A is closed, hence a Borel subset of R m \mathbb{R}^m R m by claim 4 of the Borel measurability lemma on Euclidean space ; the map Ο β¦ A r β N β 1 / 2 G r s ^ r N ( Ο ) \omega\mapsto A_r-N^{-1/2}\mathcal{G}_r\hat{\mathfrak{s}}^N_r(\omega) Ο β¦ A r β β N β 1/2 G r β s ^ r N β ( Ο ) has F \mathcal{F} F -measurable components by Step 1 (A r A_r A r β and G r \mathcal{G}_r G r β being constants at the fixed r r r ), hence is measurable into R m \mathbb{R}^m R m with its Borel Ο \sigma Ο -algebra by claim 2 of the same lemma, so Ο r \chi_r Ο r β , the indicator of the preimage of A \mathcal{A} A , is a random variable, and ( 1 β Ο r ) β£ s ^ r N β£ 2 (1-\chi_r)|\hat{\mathfrak{s}}^N_r|^2 ( 1 β Ο r β ) β£ s ^ r N β β£ 2 is a random variable dominated by the integrable β£ s ^ r N β£ 2 |\hat{\mathfrak{s}}^N_r|^2 β£ s ^ r N β β£ 2 of part (d).
Now fix r r r and work on Ξ© 0 \Omega_0 Ξ© 0 β . Where Ο r = 0 \chi_r=0 Ο r β = 0 the point A r β N β 1 / 2 G r s ^ r N A_r-N^{-1/2}\mathcal{G}_r\hat{\mathfrak{s}}^N_r A r β β N β 1/2 G r β s ^ r N β does not lie in A \mathcal{A} A , so by hypothesis (H5) its Euclidean distance to A r A_r A r β exceeds Ο± \varrho Ο± , that is N β 1 / 2 β£ G r s ^ r N β£ > Ο± N^{-1/2}|\mathcal{G}_r\hat{\mathfrak{s}}^N_r|>\varrho N β 1/2 β£ G r β s ^ r N β β£ > Ο± ; with β£ G r s ^ r N β£ β€ g β β£ s ^ r N β£ |\mathcal{G}_r\hat{\mathfrak{s}}^N_r|\le g^*|\hat{\mathfrak{s}}^N_r| β£ G r β s ^ r N β β£ β€ g β β£ s ^ r N β β£ this gives β£ s ^ r N β£ > Ο± N 1 / 2 / g β |\hat{\mathfrak{s}}^N_r|>\varrho N^{1/2}/g^* β£ s ^ r N β β£ > Ο± N 1/2 / g β there, hence 1 < ( g β ) 2 Ο± β 2 N β 1 β£ s ^ r N β£ 2 1<(g^*)^2\varrho^{-2}N^{-1}|\hat{\mathfrak{s}}^N_r|^2 1 < ( g β ) 2 Ο± β 2 N β 1 β£ s ^ r N β β£ 2 there. Multiplying by β£ s ^ r N β£ 2 |\hat{\mathfrak{s}}^N_r|^2 β£ s ^ r N β β£ 2 where Ο r = 0 \chi_r=0 Ο r β = 0 , and noting that where Ο r = 1 \chi_r=1 Ο r β = 1 the left side of the display below is 0 0 0 while its right side is nonnegative, we obtain the pointwise bound on Ξ© 0 \Omega_0 Ξ© 0 β
( 1 β Ο r ) β β£ s ^ r N β£ 2 Β β€ Β ( g β ) 2 β Ο± β 2 β N β 1 β β£ s ^ r N β£ 4 , (1-\chi_r)\,|\hat{\mathfrak{s}}^N_r|^2\ \le\ (g^*)^2\,\varrho^{-2}\,N^{-1}\,|\hat{\mathfrak{s}}^N_r|^4 , ( 1 β Ο r β ) β£ s ^ r N β β£ 2 Β β€ Β ( g β ) 2 Ο± β 2 N β 1 β£ s ^ r N β β£ 4 ,
so by monotonicity of the integral and part (d), E [ ( 1 β Ο r ) β£ s ^ r N β£ 2 ] β€ ( g β ) 2 Ο± β 2 N β 1 C 1 ΞΊ 0 \mathbb{E}[(1-\chi_r)|\hat{\mathfrak{s}}^N_r|^2]\le(g^*)^2\varrho^{-2}N^{-1}C_1\kappa_0 E [( 1 β Ο r β ) β£ s ^ r N β β£ 2 ] β€ ( g β ) 2 Ο± β 2 N β 1 C 1 β ΞΊ 0 β . Since β£ w r β£ 2 β€ ( b β g β ) 2 ( 1 β Ο r ) β£ s ^ r N β£ 2 |w_r|^2\le(b^*g^*)^2(1-\chi_r)|\hat{\mathfrak{s}}^N_r|^2 β£ w r β β£ 2 β€ ( b β g β ) 2 ( 1 β Ο r β ) β£ s ^ r N β β£ 2 pointwise (1 β Ο r 1-\chi_r 1 β Ο r β taking the values 0 0 0 and 1 1 1 only, so that ( 1 β Ο r ) 2 = 1 β Ο r (1-\chi_r)^2=1-\chi_r ( 1 β Ο r β ) 2 = 1 β Ο r β ),
β₯ w r β₯ 2 Β β€ Β b β β ( g β ) 2 β Ο± β 1 β C 1 β
β N β 1 / 2 β ΞΊ 0 1 / 2 . \Vert w_r\Vert_2\ \le\ b^*\,(g^*)^2\,\varrho^{-1}\,\sqrt{C_1}\;N^{-1/2}\,\kappa_0^{1/2} . β₯ w r β β₯ 2 β Β β€ Β b β ( g β ) 2 Ο± β 1 C 1 β β N β 1/2 ΞΊ 0 1/2 β .
Residual cross terms. By the componentwise Cauchy-Schwarz inequality , β£ X r Ξ³ Ξ΄ β£ β€ 2 β β₯ Ξ΅ r β₯ 2 ( β₯ e r β₯ 2 + k β β₯ e ~ r β₯ 2 + β₯ w r β₯ 2 ) |X^{\gamma\delta}_r|\le2\,\Vert\varepsilon_r\Vert_2\big(\Vert e_r\Vert_2+k^*\Vert\tilde{e}_r\Vert_2+\Vert w_r\Vert_2\big) β£ X r Ξ³ Ξ΄ β β£ β€ 2 β₯ Ξ΅ r β β₯ 2 β ( β₯ e r β β₯ 2 β + k β β₯ e ~ r β β₯ 2 β + β₯ w r β β₯ 2 β ) , where β₯ β
β₯ 2 \Vert\cdot\Vert_2 β₯ β
β₯ 2 β denotes the mean-square norm of the Euclidean norm of the indicated vector. By the quadratic residual bounds and (d): since β£ z r β£ 4 β€ 8 ( β£ s r β£ 4 + β£ a r β£ 4 ) |z_r|^4\le8(|\mathfrak{s}_r|^4+|\mathfrak{a}_r|^4) β£ z r β β£ 4 β€ 8 ( β£ s r β β£ 4 + β£ a r β β£ 4 ) pointwise, E [ β£ z r β£ 4 ] β€ 16 C 1 ΞΊ 0 \mathbb{E}[|z_r|^4]\le16C_1\kappa_0 E [ β£ z r β β£ 4 ] β€ 16 C 1 β ΞΊ 0 β , so β₯ e r β₯ 2 β€ c e N β 1 / 2 β E [ β£ z r β£ 4 ] 1 / 2 β€ 4 c e C 1 β N β 1 / 2 ΞΊ 0 1 / 2 \Vert e_r\Vert_2\le c_eN^{-1/2}\,\mathbb{E}[|z_r|^4]^{1/2}\le4c_e\sqrt{C_1}\,N^{-1/2}\kappa_0^{1/2} β₯ e r β β₯ 2 β β€ c e β N β 1/2 E [ β£ z r β β£ 4 ] 1/2 β€ 4 c e β C 1 β β N β 1/2 ΞΊ 0 1/2 β ; likewise β₯ e ~ r β₯ 2 β€ c ~ e N β 1 / 2 E [ β£ s r β£ 4 ] 1 / 2 β€ c ~ e C 1 N β 1 / 2 ΞΊ 0 1 / 2 \Vert\tilde{e}_r\Vert_2\le\tilde{c}_e N^{-1/2}\mathbb{E}[|\mathfrak{s}_r|^4]^{1/2}\le\tilde{c}_e\sqrt{C_1}N^{-1/2}\kappa_0^{1/2} β₯ e ~ r β β₯ 2 β β€ c ~ e β N β 1/2 E [ β£ s r β β£ 4 ] 1/2 β€ c ~ e β C 1 β β N β 1/2 ΞΊ 0 1/2 β ; and β₯ Ξ΅ r β₯ 2 β€ ( C Λ ΞΊ 0 ) 1 / 2 \Vert\varepsilon_r\Vert_2\le(\bar{C}\kappa_0)^{1/2} β₯ Ξ΅ r β β₯ 2 β β€ ( C Λ ΞΊ 0 β ) 1/2 . Hence β£ X r Ξ³ Ξ΄ β£ β€ c 9 β N β 1 / 2 ΞΊ 0 |X^{\gamma\delta}_r|\le c_9\,N^{-1/2}\kappa_0 β£ X r Ξ³ Ξ΄ β β£ β€ c 9 β N β 1/2 ΞΊ 0 β with c 9 = 2 C Λ ( 4 c e + k β c ~ e + b β ( g β ) 2 Ο± β 1 ) C 1 c_9=2\sqrt{\bar{C}}\big(4c_e+k^*\tilde{c}_e+b^*(g^*)^2\varrho^{-1}\big)\sqrt{C_1} c 9 β = 2 C Λ β ( 4 c e β + k β c ~ e β + b β ( g β ) 2 Ο± β 1 ) C 1 β β , the clamp remainder contributing the last summand through the bound on β₯ w r β₯ 2 \Vert w_r\Vert_2 β₯ w r β β₯ 2 β just proved.
Covariance deviation. By part (b) of the covariance deviation lemma and (d), β£ Ξ r Ξ³ Ξ΄ β£ β€ c Ξ N β 1 / 2 ( E [ β£ s r β£ 2 ] + E [ β£ a r β£ 2 ] ) 1 / 2 β€ c Ξ 2 C Λ β N β 1 / 2 ΞΊ 0 |\Delta^{\gamma\delta}_r|\le c_\Theta N^{-1/2}(\mathbb{E}[|\mathfrak{s}_r|^2]+\mathbb{E}[|\mathfrak{a}_r|^2])^{1/2}\le c_\Theta\sqrt{2\bar{C}}\,N^{-1/2}\kappa_0 β£ Ξ r Ξ³ Ξ΄ β β£ β€ c Ξ β N β 1/2 ( E [ β£ s r β β£ 2 ] + E [ β£ a r β β£ 2 ] ) 1/2 β€ c Ξ β 2 C Λ β N β 1/2 ΞΊ 0 β , with its constant c Ξ = 2 ( l β 1 ) ( B + K l + m ) c_\Theta=2(l-1)(B+K\sqrt{l+m}) c Ξ β = 2 ( l β 1 ) ( B + K l + m β ) .
Observation drift deviation. By parts (i) and (ii) of the observation drift regularity lemma , pointwise β£ b ~ Ο
( Ξ£ r ) β b ~ Ο
( S r ) β£ β€ l ( B ~ + K ~ ) N β 1 / 2 β£ s r β£ |\tilde{b}^\upsilon(\Sigma_r)-\tilde{b}^\upsilon(S_r)|\le\sqrt{l}(\tilde{B}+\tilde{K})N^{-1/2}|\mathfrak{s}_r| β£ b ~ Ο
( Ξ£ r β ) β b ~ Ο
( S r β ) β£ β€ l β ( B ~ + K ~ ) N β 1/2 β£ s r β β£ , so β£ E [ b ~ Ο
( Ξ£ r ) ] β b ~ Ο
( S r ) β£ β€ l ( B ~ + K ~ ) N β 1 / 2 β₯ s r β₯ 2 β€ l ( B ~ + K ~ ) C Λ β N β 1 / 2 ΞΊ 0 |\mathbb{E}[\tilde{b}^\upsilon(\Sigma_r)]-\tilde{b}^\upsilon(S_r)|\le\sqrt{l}(\tilde{B}+\tilde{K})N^{-1/2}\Vert\mathfrak{s}_r\Vert_2\le\sqrt{l}(\tilde{B}+\tilde{K})\sqrt{\bar{C}}\,N^{-1/2}\kappa_0 β£ E [ b ~ Ο
( Ξ£ r β )] β b ~ Ο
( S r β ) β£ β€ l β ( B ~ + K ~ ) N β 1/2 β₯ s r β β₯ 2 β β€ l β ( B ~ + K ~ ) C Λ β N β 1/2 ΞΊ 0 β and β£ Ξ ~ r Ξ³ Ξ΄ β£ β€ l ~ C K ~ 2 l ( B ~ + K ~ ) C Λ β N β 1 / 2 ΞΊ 0 = : c 10 N β 1 / 2 ΞΊ 0 |\tilde{\Delta}^{\gamma\delta}_r|\le\tilde{l}C_{\tilde{K}}^2\sqrt{l}(\tilde{B}+\tilde{K})\sqrt{\bar{C}}\,N^{-1/2}\kappa_0=:c_{10}N^{-1/2}\kappa_0 β£ Ξ ~ r Ξ³ Ξ΄ β β£ β€ l ~ C K ~ 2 β l β ( B ~ + K ~ ) C Λ β N β 1/2 ΞΊ 0 β =: c 10 β N β 1/2 ΞΊ 0 β .
Gronwall. Let u ( t ) = max β‘ Ξ³ , Ξ΄ β£ D t Ξ³ Ξ΄ β£ u(t)=\max_{\gamma,\delta}|D^{\gamma\delta}_t| u ( t ) = max Ξ³ , Ξ΄ β β£ D t Ξ³ Ξ΄ β β£ , continuous on [ 0 , T ] [0,T] [ 0 , T ] (each Ξ N , Ξ³ Ξ΄ \Pi^{N,\gamma\delta} Ξ N , Ξ³ Ξ΄ continuous by (c), each Ξ Ξ³ Ξ΄ \Pi^{\gamma\delta} Ξ Ξ³ Ξ΄ continuous by conclusion 2 of the policy lemma; maxima of finitely many continuous functions are continuous). Entrywise, β£ ( ( E β K ~ E ~ ) D ) r Ξ³ Ξ΄ β£ β€ l β c 1 β u ( r ) |((\mathcal{E}-\tilde{\mathcal{K}}\tilde{\mathcal{E}})D)^{\gamma\delta}_r|\le l\,c_1\,u(r) β£ (( E β K ~ E ~ ) D ) r Ξ³ Ξ΄ β β£ β€ l c 1 β u ( r ) and likewise for the transposed product, so by monotonicity of the integral ,
u ( t ) Β β€ Β u ( 0 ) + 2 l c 1 β« [ 0 , t ] u ( r ) β d r + T β ( c 9 + c Ξ 2 C Λ + c 10 ) β N β 1 / 2 ΞΊ 0 . u(t)\ \le\ u(0)+2lc_1\int_{[0,t]}u(r)\,dr+T\,(c_9+c_\Theta\sqrt{2\bar{C}}+c_{10})\,N^{-1/2}\kappa_0 . u ( t ) Β β€ Β u ( 0 ) + 2 l c 1 β β« [ 0 , t ] β u ( r ) d r + T ( c 9 β + c Ξ β 2 C Λ β + c 10 β ) N β 1/2 ΞΊ 0 β .
As in Part (d) of the published proof of the completion-of-squares theorem , the agreement of the Riemann and Lebesgue integrals for the continuous u u u , by claim 3 of the interval toolkit , and Gronwall's lemma give
u ( t ) Β β€ Β ( u ( 0 ) + T ( c 9 + c Ξ 2 C Λ + c 10 ) N β 1 / 2 ΞΊ 0 ) exp β‘ ( 2 l c 1 T ) , u(t)\ \le\ \Big(u(0)+T(c_9+c_\Theta\sqrt{2\bar{C}}+c_{10})N^{-1/2}\kappa_0\Big)\exp\big(2lc_1T\big), u ( t ) Β β€ Β ( u ( 0 ) + T ( c 9 β + c Ξ β 2 C Λ β + c 10 β ) N β 1/2 ΞΊ 0 β ) exp ( 2 l c 1 β T ) ,
and since u ( 0 ) = max β‘ Ξ³ , Ξ΄ β£ E [ s 0 Ξ³ s 0 Ξ΄ ] β Ξ 0 Ξ³ Ξ΄ β£ u(0)=\max_{\gamma,\delta}|\mathbb{E}[\mathfrak{s}^\gamma_0\mathfrak{s}^\delta_0]-\Pi^{\gamma\delta}_0| u ( 0 ) = max Ξ³ , Ξ΄ β β£ E [ s 0 Ξ³ β s 0 Ξ΄ β ] β Ξ 0 Ξ³ Ξ΄ β β£ by part (a), the conclusion (e) holds with C = exp β‘ ( 2 l c 1 T ) max β‘ ( 1 , β T ( c 9 + c Ξ 2 C Λ + c 10 ) ) C=\exp(2lc_1T)\max\big(1,\,T(c_9+c_\Theta\sqrt{2\bar{C}}+c_{10})\big) C = exp ( 2 l c 1 β T ) max ( 1 , T ( c 9 β + c Ξ β 2 C Λ β + c 10 β ) ) , which depends only on the data named in the statement. β \blacksquare β