Throughout, adopt the notation of the statement (g s g_s g s β , z s z_s z s β , Ξ \Lambda Ξ , E s E_s E s β , B s \mathsf{B}_s B s β , e s e_s e s β , Ξ© a \Omega_{\mathfrak{a}} Ξ© a β , R t \mathcal{R}_t R t β ), write x s = ( S s , A s ) x_s=(S_s,A_s) x s β = ( S s β , A s β ) and y s = ( Ξ£ s , Ξ± s ) y_s=(\Sigma_s,\alpha_s) y s β = ( Ξ£ s β , Ξ± s β ) as points of R l + m \mathbb{R}^{l+m} R l + m under the coordinate identification of the extension definition , so that y s β x s = z s / N y_s-x_s=z_s/\sqrt{N} y s β β x s β = z s β / N β pointwise, and write p Λ = ( 1 / l , β¦ , 1 / l ) \bar{p}=(1/l,\dots,1/l) p Λ β = ( 1/ l , β¦ , 1/ l ) , a point of the probability simplex Ξ l \Delta^l Ξ l . All integrals over [ 0 , t ] [0,t] [ 0 , t ] below are 0 0 0 for t = 0 t=0 t = 0 ; at t = 0 t=0 t = 0 the identity of clause (c) reduces to M 0 = 0 M_0=0 M 0 β = 0 , which is the t = 0 t=0 t = 0 case of the definition of M Ξ³ M^\gamma M Ξ³ in clause (b) of the martingale decomposition , and both displays of clause (d) read 0 β€ 0 0\le0 0 β€ 0 . Accordingly, wherever an integral over [ 0 , t ] [0,t] [ 0 , t ] is manipulated we take t > 0 t>0 t > 0 .
Step 1: pointwise bounds (clause (a)). Fix ( s , Ο ) β [ 0 , T ] Γ Ξ© (s,\omega)\in[0,T]\times\Omega ( s , Ο ) β [ 0 , T ] Γ Ξ© . By the definition of the controlled N N N -agent dynamics , the state processes take values in { 1 , β¦ , l } \{1,\dots,l\} { 1 , β¦ , l } at every point, so the empirical state measure Ξ£ s ( Ο ) \Sigma_s(\omega) Ξ£ s β ( Ο ) lies in Ξ l \Delta^l Ξ l ; and S s β Ξ l S_s\in\Delta^l S s β β Ξ l , the mean-field trajectory pair having S : [ 0 , T ] β Ξ l S:[0,T]\to\Delta^l S : [ 0 , T ] β Ξ l . Moreover Ξ± s ( Ο ) β A \alpha_s(\omega)\in\mathcal{A} Ξ± s β ( Ο ) β A at every point of Ξ© \Omega Ξ© β the control process of a solution takes values in A \mathcal{A} A by that definition's solution data, the policy being A \mathcal{A} A -valued β and A s β A A_s\in\mathcal{A} A s β β A (the trajectory pair having A : [ 0 , T ] β A A:[0,T]\to\mathcal{A} A : [ 0 , T ] β A ). Hence x s x_s x s β and y s y_s y s β lie in Ξ l Γ A β Ξ l Γ V \Delta^l\times\mathcal{A}\subseteq\Delta^l\times V Ξ l Γ A β Ξ l Γ V , and every point of the segment { x s + Ο ( y s β x s ) : Ο β [ 0 , 1 ] } \{x_s+\tau(y_s-x_s):\tau\in[0,1]\} { x s β + Ο ( y s β β x s β ) : Ο β [ 0 , 1 ]} lies in Ξ l Γ V \Delta^l\times V Ξ l Γ V : the convex combination ( 1 β Ο ) S s + Ο Ξ£ s ( Ο ) (1-\tau)S_s+\tau\Sigma_s(\omega) ( 1 β Ο ) S s β + Ο Ξ£ s β ( Ο ) of two points of the simplex has nonnegative entries with sum ( 1 β Ο ) + Ο = 1 (1-\tau)+\tau=1 ( 1 β Ο ) + Ο = 1 , and the control coordinates form a convex combination of the two points A s A_s A s β and Ξ± s ( Ο ) \alpha_s(\omega) Ξ± s β ( Ο ) of A β V \mathcal{A}\subseteq V A β V , the set V V V being convex by the extension definition . By clause (i) of the regularity of the extended aggregate state drift , b Λ \bar{b} b Λ agrees with b b b on Ξ l Γ A \Delta^l\times\mathcal{A} Ξ l Γ A β which contains both x s x_s x s β and y s y_s y s β β and each b Λ Ξ³ \bar{b}^\gamma b Λ Ξ³ is a C 1 C^1 C 1 map on the open set U Γ V U\times V U Γ V whose partial derivatives are again C 1 C^1 C 1 ; also Ξ l Γ V β U Γ V \Delta^l\times V\subseteq U\times V Ξ l Γ V β U Γ V . Therefore the Taylor lemma applies to f = b Λ Ξ³ f=\bar{b}^\gamma f = b Λ Ξ³ with n = l + m n=l+m n = l + m , x = x s x=x_s x = x s β , y = y s y=y_s y = y s β , h = z s ( Ο ) / N h=z_s(\omega)/\sqrt{N} h = z s β ( Ο ) / N β . By the definitions of E s E_s E s β and B s \mathsf{B}_s B s β ,
( E s s s + B s a s ) Ξ³ = β i = 1 l + m β i b Λ Ξ³ ( x s ) β z s i , e s Ξ³ = N β ( b Λ Ξ³ ( y s ) β b Λ Ξ³ ( x s ) β β i = 1 l + m β i b Λ Ξ³ ( x s ) β z s i N ) . \big(E_s\mathfrak{s}_s+\mathsf{B}_s\mathfrak{a}_s\big)^\gamma=\sum_{i=1}^{l+m}\partial_i\bar{b}^\gamma(x_s)\,z^i_s,\qquad\qquad e^\gamma_s=\sqrt{N}\,\Big(\bar{b}^\gamma(y_s)-\bar{b}^\gamma(x_s)-\sum_{i=1}^{l+m}\partial_i\bar{b}^\gamma(x_s)\,\frac{z^i_s}{\sqrt{N}}\Big). ( E s β s s β + B s β a s β ) Ξ³ = i = 1 β l + m β β i β b Λ Ξ³ ( x s β ) z s i β , e s Ξ³ β = N β ( b Λ Ξ³ ( y s β ) β b Λ Ξ³ ( x s β ) β i = 1 β l + m β β i β b Λ Ξ³ ( x s β ) N β z s i β β ) .
Part (ii) of the Taylor lemma with M 2 = 3 β l β K M_2=3\,l\,K M 2 β = 3 l K β a bound for all second-order partials of b Λ Ξ³ \bar{b}^\gamma b Λ Ξ³ on Ξ l Γ V \Delta^l\times V Ξ l Γ V , hence on the segment, by clause (iii) of the drift regularity lemma β gives
β£ e s Ξ³ β£ Β β€ Β N β
1 2 β ( l + m ) β 3 β l β K β β£ z s β£ 2 N Β = Β 3 β l β K β ( l + m ) 2 N β β£ z s β£ 2 , |e^\gamma_s|\ \le\ \sqrt{N}\cdot\tfrac{1}{2}\,(l+m)\,3\,l\,K\,\frac{|z_s|^2}{N}\ =\ \frac{3\,l\,K\,(l+m)}{2\sqrt{N}}\,|z_s|^2, β£ e s Ξ³ β β£ Β β€ Β N β β
2 1 β ( l + m ) 3 l K N β£ z s β β£ 2 β Β = Β 2 N β 3 l K ( l + m ) β β£ z s β β£ 2 ,
and β£ e s β£ β€ l β max β‘ Ξ³ β£ e s Ξ³ β£ |e_s|\le\sqrt{l}\,\max_\gamma|e^\gamma_s| β£ e s β β£ β€ l β max Ξ³ β β£ e s Ξ³ β β£ (the elementary inequality β Ξ³ ( e s Ξ³ ) 2 β€ l β max β‘ Ξ³ ( e s Ξ³ ) 2 \sum_\gamma(e^\gamma_s)^2\le l\,\max_\gamma(e^\gamma_s)^2 β Ξ³ β ( e s Ξ³ β ) 2 β€ l max Ξ³ β ( e s Ξ³ β ) 2 ) yields the first bound of clause (a). The Lipschitz estimate of clause (ii) of the drift regularity lemma β available because A \mathcal{A} A is convex by hypothesis β applied to the points x s , y s β Ξ l Γ A x_s,y_s\in\Delta^l\times\mathcal{A} x s β , y s β β Ξ l Γ A , whose Euclidean distance is β£ z s β£ / N |z_s|/\sqrt{N} β£ z s β β£/ N β , gives β£ g s Ξ³ β£ = N β β£ b Λ Ξ³ ( y s ) β b Λ Ξ³ ( x s ) β£ β€ N β
l + m β
β l β ( B + K ) β β£ z s β£ / N |g^\gamma_s|=\sqrt{N}\,\big|\bar{b}^\gamma(y_s)-\bar{b}^\gamma(x_s)\big|\le\sqrt{N}\cdot\sqrt{l+m}\;l\,(B+K)\,|z_s|/\sqrt{N} β£ g s Ξ³ β β£ = N β β b Λ Ξ³ ( y s β ) β b Λ Ξ³ ( x s β ) β β€ N β β
l + m β l ( B + K ) β£ z s β β£/ N β , so β£ g s β£ β€ l β l + m β
β l β ( B + K ) β β£ z s β£ = Ξ β β£ z s β£ |g_s|\le\sqrt{l}\,\sqrt{l+m}\;l\,(B+K)\,|z_s|=\Lambda\,|z_s| β£ g s β β£ β€ l β l + m β l ( B + K ) β£ z s β β£ = Ξ β£ z s β β£ by the same elementary inequality; and β£ ( E s s s + B s a s ) Ξ³ β£ β€ β i = 1 l + m β£ β i b Λ Ξ³ ( x s ) β£ β β£ z s i β£ β€ l β ( B + K ) β l + m β β£ z s β£ |(E_s\mathfrak{s}_s+\mathsf{B}_s\mathfrak{a}_s)^\gamma|\le\sum_{i=1}^{l+m}|\partial_i\bar{b}^\gamma(x_s)|\,|z^i_s|\le l\,(B+K)\,\sqrt{l+m}\,|z_s| β£ ( E s β s s β + B s β a s β ) Ξ³ β£ β€ β i = 1 l + m β β£ β i β b Λ Ξ³ ( x s β ) β£ β£ z s i β β£ β€ l ( B + K ) l + m β β£ z s β β£ , by clause (ii) and the elementary inequality β i = 1 l + m β£ z s i β£ β€ l + m β β£ z s β£ \sum_{i=1}^{l+m}|z^i_s|\le\sqrt{l+m}\,|z_s| β i = 1 l + m β β£ z s i β β£ β€ l + m β β£ z s β β£ (an instance of 2 Ξ» ΞΌ β€ Ξ» 2 + ΞΌ 2 2\lambda\mu\le\lambda^2+\mu^2 2 Ξ» ΞΌ β€ Ξ» 2 + ΞΌ 2 summed over indices), so β£ E s s s + B s a s β£ β€ Ξ β β£ z s β£ |E_s\mathfrak{s}_s+\mathsf{B}_s\mathfrak{a}_s|\le\Lambda\,|z_s| β£ E s β s s β + B s β a s β β£ β€ Ξ β£ z s β β£ . The triangle inequality (the Euclidean distance is a metric ) gives β£ e s β£ β€ β£ g s β£ + β£ E s s s + B s a s β£ β€ 2 β Ξ β β£ z s β£ |e_s|\le|g_s|+|E_s\mathfrak{s}_s+\mathsf{B}_s\mathfrak{a}_s|\le2\,\Lambda\,|z_s| β£ e s β β£ β€ β£ g s β β£ + β£ E s β s s β + B s β a s β β£ β€ 2 Ξ β£ z s β β£ . No use of the hypothesis A 2 < β \mathcal{A}_2<\infty A 2 β < β was made.
Step 2: measurability and the residual process (clause (b)). Fix a point a 0 β A a_0\in\mathcal{A} a 0 β β A (the control set being nonempty) and define Ξ£ ~ s Ξ³ = 1 Ξ© 0 Ξ£ s Ξ³ + ( 1 β 1 Ξ© 0 ) β p Λ Ξ³ \tilde{\Sigma}^\gamma_s=\mathbf{1}_{\Omega_0}\Sigma^\gamma_s+(1-\mathbf{1}_{\Omega_0})\,\bar{p}^\gamma Ξ£ ~ s Ξ³ β = 1 Ξ© 0 β β Ξ£ s Ξ³ β + ( 1 β 1 Ξ© 0 β β ) p Λ β Ξ³ and Ξ± ~ s j = 1 Ξ© 0 Ξ± s j + ( 1 β 1 Ξ© 0 ) β a 0 j \tilde{\alpha}^j_s=\mathbf{1}_{\Omega_0}\alpha^j_s+(1-\mathbf{1}_{\Omega_0})\,a_0^j Ξ± ~ s j β = 1 Ξ© 0 β β Ξ± s j β + ( 1 β 1 Ξ© 0 β β ) a 0 j β , so that ( Ξ£ ~ s ( Ο ) , Ξ± ~ s ( Ο ) ) β Ξ l Γ A (\tilde{\Sigma}_s(\omega),\tilde{\alpha}_s(\omega))\in\Delta^l\times\mathcal{A} ( Ξ£ ~ s β ( Ο ) , Ξ± ~ s β ( Ο )) β Ξ l Γ A at every point (on Ξ© 0 \Omega_0 Ξ© 0 β by Step 1, off Ξ© 0 \Omega_0 Ξ© 0 β by construction). The maps ( s , Ο ) β¦ 1 Ξ© 0 ( Ο ) Ξ£ s Ξ³ ( Ο ) (s,\omega)\mapsto\mathbf{1}_{\Omega_0}(\omega)\Sigma^\gamma_s(\omega) ( s , Ο ) β¦ 1 Ξ© 0 β β ( Ο ) Ξ£ s Ξ³ β ( Ο ) and ( s , Ο ) β¦ 1 Ξ© 0 ( Ο ) Ξ± s j ( Ο ) (s,\omega)\mapsto\mathbf{1}_{\Omega_0}(\omega)\alpha^j_s(\omega) ( s , Ο ) β¦ 1 Ξ© 0 β β ( Ο ) Ξ± s j β ( Ο ) are measurable with respect to the product Ο \sigma Ο -algebra of the trace Borel Ο \sigma Ο -algebra on [ 0 , T ] [0,T] [ 0 , T ] and F \mathcal{F} F , by clauses (b) and (c) of the joint measurability of the state and control ; and ( s , Ο ) β¦ 1 Ξ© 0 ( Ο ) (s,\omega)\mapsto\mathbf{1}_{\Omega_0}(\omega) ( s , Ο ) β¦ 1 Ξ© 0 β β ( Ο ) is product-measurable as the indicator of the measurable rectangle [ 0 , T ] Γ Ξ© 0 [0,T]\times\Omega_0 [ 0 , T ] Γ Ξ© 0 β (Ξ© 0 β F \Omega_0\in\mathcal{F} Ξ© 0 β β F by the controlled-dynamics definition , and rectangles generate the product Ο \sigma Ο -algebra ). Hence Ξ£ ~ Ξ³ \tilde{\Sigma}^\gamma Ξ£ ~ Ξ³ and Ξ± ~ j \tilde{\alpha}^j Ξ± ~ j are product-measurable. The function
F Ξ³ ( s , Ξ£ , Ξ± ) = N β ( b Λ Ξ³ ( Ξ£ , Ξ± ) β b Λ Ξ³ ( S s , A s ) ) β β i = 1 l + m β i b Λ Ξ³ ( S s , A s ) β
( N β ( Ξ£ β S s , Β Ξ± β A s ) ) i F^\gamma(s,\Sigma,\alpha)=\sqrt{N}\,\Big(\bar{b}^\gamma(\Sigma,\alpha)-\bar{b}^\gamma(S_s,A_s)\Big)-\sum_{i=1}^{l+m}\partial_i\bar{b}^\gamma(S_s,A_s)\cdot\big(\sqrt{N}\,(\Sigma-S_s,\ \alpha-A_s)\big)^i F Ξ³ ( s , Ξ£ , Ξ± ) = N β ( b Λ Ξ³ ( Ξ£ , Ξ± ) β b Λ Ξ³ ( S s β , A s β ) ) β i = 1 β l + m β β i β b Λ Ξ³ ( S s β , A s β ) β
( N β ( Ξ£ β S s β , Β Ξ± β A s β ) ) i
is jointly continuous, hence sequentially continuous, on [ 0 , T ] Γ U Γ V β R 1 + l + m [0,T]\times U\times V\subseteq\mathbb{R}^{1+l+m} [ 0 , T ] Γ U Γ V β R 1 + l + m , since b Λ Ξ³ \bar{b}^\gamma b Λ Ξ³ and its partial derivatives are continuous (clause (i) of the drift regularity lemma) and the trajectory pair ( S , A ) (S,A) ( S , A ) is continuous; and, using b Λ = b \bar{b}=b b Λ = b on Ξ l Γ A \Delta^l\times\mathcal{A} Ξ l Γ A (Step 1), 1 Ξ© 0 e s Ξ³ = 1 Ξ© 0 β
F Ξ³ ( s , Ξ£ ~ s , Ξ± ~ s ) \mathbf{1}_{\Omega_0}e^\gamma_s=\mathbf{1}_{\Omega_0}\cdot F^\gamma(s,\tilde{\Sigma}_s,\tilde{\alpha}_s) 1 Ξ© 0 β β e s Ξ³ β = 1 Ξ© 0 β β β
F Ξ³ ( s , Ξ£ ~ s β , Ξ± ~ s β ) at every point of [ 0 , T ] Γ Ξ© [0,T]\times\Omega [ 0 , T ] Γ Ξ© , the arguments lying in the domain of F Ξ³ F^\gamma F Ξ³ everywhere since ( Ξ£ ~ s , Ξ± ~ s ) β Ξ l Γ A β U Γ V (\tilde{\Sigma}_s,\tilde{\alpha}_s)\in\Delta^l\times\mathcal{A}\subseteq U\times V ( Ξ£ ~ s β , Ξ± ~ s β ) β Ξ l Γ A β U Γ V . By measurability of sequentially continuous functions of measurable Euclidean maps β applied to F Ξ³ F^\gamma F Ξ³ composed with the measurable maps ( s , Ο ) β¦ s (s,\omega)\mapsto s ( s , Ο ) β¦ s , Ξ£ ~ Ξ³ \tilde{\Sigma}^\gamma Ξ£ ~ Ξ³ , Ξ± ~ j \tilde{\alpha}^j Ξ± ~ j , and once more to the product with 1 Ξ© 0 \mathbf{1}_{\Omega_0} 1 Ξ© 0 β β β each ( s , Ο ) β¦ 1 Ξ© 0 e s Ξ³ (s,\omega)\mapsto\mathbf{1}_{\Omega_0}e^\gamma_s ( s , Ο ) β¦ 1 Ξ© 0 β β e s Ξ³ β is product-measurable. The same argument makes ( s , Ο ) β¦ 1 Ξ© 0 β£ s s β£ (s,\omega)\mapsto\mathbf{1}_{\Omega_0}|\mathfrak{s}_s| ( s , Ο ) β¦ 1 Ξ© 0 β β β£ s s β β£ , ( s , Ο ) β¦ 1 Ξ© 0 β£ a s β£ (s,\omega)\mapsto\mathbf{1}_{\Omega_0}|\mathfrak{a}_s| ( s , Ο ) β¦ 1 Ξ© 0 β β β£ a s β β£ , their squares, and, for Step 4, ( s , Ο ) β¦ 1 Ξ© 0 w s (s,\omega)\mapsto\mathbf{1}_{\Omega_0}w_s ( s , Ο ) β¦ 1 Ξ© 0 β β w s β with w s = min β‘ ( 3 l l K ( l + m ) 2 N β£ z s β£ 2 , β 2 Ξ β£ z s β£ ) 2 w_s=\min\big(\tfrac{3l\sqrt{l}K(l+m)}{2\sqrt{N}}|z_s|^2,\,2\Lambda|z_s|\big)^2 w s β = min ( 2 N β 3 l l β K ( l + m ) β β£ z s β β£ 2 , 2Ξβ£ z s β β£ ) 2 and ( s , Ο ) β¦ 1 Ξ© 0 β£ z s β£ 4 (s,\omega)\mapsto\mathbf{1}_{\Omega_0}|z_s|^4 ( s , Ο ) β¦ 1 Ξ© 0 β β β£ z s β β£ 4 , product-measurable.
By the Tonelli theorem (the trace Lebesgue measure of the toolkit and P P P being finite, hence Ο \sigma Ο -finite, measures), Ξ¦ a ( Ο ) = β« [ 0 , T ] 1 Ξ© 0 ( Ο ) β β£ a s ( Ο ) β£ 2 β d s \Phi_{\mathfrak{a}}(\omega)=\int_{[0,T]}\mathbf{1}_{\Omega_0}(\omega)\,|\mathfrak{a}_s(\omega)|^2\,ds Ξ¦ a β ( Ο ) = β« [ 0 , T ] β 1 Ξ© 0 β β ( Ο ) β£ a s β ( Ο ) β£ 2 d s defines a measurable [ 0 , β ] [0,\infty] [ 0 , β ] -valued function of Ο \omega Ο with E [ Ξ¦ a ] = A 2 \mathbb{E}[\Phi_{\mathfrak{a}}]=\mathcal{A}_2 E [ Ξ¦ a β ] = A 2 β (the expectations defining A 2 \mathcal{A}_2 A 2 β are unchanged by the 1 Ξ© 0 \mathbf{1}_{\Omega_0} 1 Ξ© 0 β β modification because Ξ© 0 \Omega_0 Ξ© 0 β has probability 1 1 1 , as recorded in clause (a) of the a priori second-moment bound ); for Ο β Ξ© 0 \omega\in\Omega_0 Ο β Ξ© 0 β its defining section is s β¦ β£ a s ( Ο ) β£ 2 s\mapsto|\mathfrak{a}_s(\omega)|^2 s β¦ β£ a s β ( Ο ) β£ 2 , so Ξ© a = Ξ© 0 β© { Ο : Ξ¦ a ( Ο ) < β } \Omega_{\mathfrak{a}}=\Omega_0\cap\{\omega:\Phi_{\mathfrak{a}}(\omega)<\infty\} Ξ© a β = Ξ© 0 β β© { Ο : Ξ¦ a β ( Ο ) < β } is an event. For every natural number n n n one has Ξ¦ a β₯ n β 1 { Ξ¦ a = β } \Phi_{\mathfrak{a}}\ge n\,\mathbf{1}_{\{\Phi_{\mathfrak{a}}=\infty\}} Ξ¦ a β β₯ n 1 { Ξ¦ a β = β } β pointwise, so monotonicity and the integral of a simple function give A 2 β₯ n β P ( Ξ¦ a = β ) \mathcal{A}_2\ge n\,P(\Phi_{\mathfrak{a}}=\infty) A 2 β β₯ n P ( Ξ¦ a β = β ) , forcing P ( Ξ¦ a = β ) = 0 P(\Phi_{\mathfrak{a}}=\infty)=0 P ( Ξ¦ a β = β ) = 0 ; as Ξ© 0 \Omega_0 Ξ© 0 β has probability 1 1 1 , so does Ξ© a \Omega_{\mathfrak{a}} Ξ© a β .
Fix Ο β Ξ© a \omega\in\Omega_{\mathfrak{a}} Ο β Ξ© a β and t β ( 0 , T ] t\in(0,T] t β ( 0 , T ] . The sections s β¦ e s Ξ³ ( Ο ) s\mapsto e^\gamma_s(\omega) s β¦ e s Ξ³ β ( Ο ) are measurable on [ 0 , T ] [0,T] [ 0 , T ] : they are the differences of the sections at Ο \omega Ο of the product-measurable maps ( 1 Ξ© 0 e Ξ³ ) + (\mathbf{1}_{\Omega_0}e^\gamma)^{+} ( 1 Ξ© 0 β β e Ξ³ ) + and ( 1 Ξ© 0 e Ξ³ ) β (\mathbf{1}_{\Omega_0}e^\gamma)^{-} ( 1 Ξ© 0 β β e Ξ³ ) β (product-measurable as continuous functions of 1 Ξ© 0 e Ξ³ \mathbf{1}_{\Omega_0}e^\gamma 1 Ξ© 0 β β e Ξ³ ; sections of product-measurable [ 0 , β ] [0,\infty] [ 0 , β ] -valued maps are measurable, as in the Tonelli theorem ), and 1 Ξ© 0 ( Ο ) = 1 \mathbf{1}_{\Omega_0}(\omega)=1 1 Ξ© 0 β β ( Ο ) = 1 ; the same argument gives measurability of the sections at Ο \omega Ο of 1 Ξ© 0 β£ s s β£ \mathbf{1}_{\Omega_0}|\mathfrak{s}_s| 1 Ξ© 0 β β β£ s s β β£ , 1 Ξ© 0 β£ a s β£ \mathbf{1}_{\Omega_0}|\mathfrak{a}_s| 1 Ξ© 0 β β β£ a s β β£ , and their squares. By Step 1 and the estimates β£ s s ( Ο ) β£ β€ 2 N |\mathfrak{s}_s(\omega)|\le2\sqrt{N} β£ s s β ( Ο ) β£ β€ 2 N β (points of Ξ l \Delta^l Ξ l have Euclidean norm at most 1 1 1 , their entries lying in [ 0 , 1 ] [0,1] [ 0 , 1 ] with sum 1 1 1 , so that β Ξ³ ( Ξ£ Ξ³ ) 2 β€ β Ξ³ Ξ£ Ξ³ = 1 \sum_\gamma(\Sigma^\gamma)^2\le\sum_\gamma\Sigma^\gamma=1 β Ξ³ β ( Ξ£ Ξ³ ) 2 β€ β Ξ³ β Ξ£ Ξ³ = 1 , and β£ Ξ£ s β S s β£ β€ β£ Ξ£ s β£ + β£ S s β£ β€ 2 |\Sigma_s-S_s|\le|\Sigma_s|+|S_s|\le2 β£ Ξ£ s β β S s β β£ β€ β£ Ξ£ s β β£ + β£ S s β β£ β€ 2 by the triangle inequality, the Euclidean distance being a metric ), β£ z s β£ β€ β£ s s β£ + β£ a s β£ |z_s|\le|\mathfrak{s}_s|+|\mathfrak{a}_s| β£ z s β β£ β€ β£ s s β β£ + β£ a s β β£ (the square of the left side being the sum of the squares of the two blocks), and β£ a s β£ β€ 1 2 ( 1 + β£ a s β£ 2 ) |\mathfrak{a}_s|\le\tfrac12(1+|\mathfrak{a}_s|^2) β£ a s β β£ β€ 2 1 β ( 1 + β£ a s β β£ 2 ) ,
β« [ 0 , t ] β£ e s Ξ³ ( Ο ) β£ β d s Β β€ Β 2 Ξ β« [ 0 , t ] ( β£ s s ( Ο ) β£ + β£ a s ( Ο ) β£ ) β d s Β β€ Β 2 Ξ β ( 2 N β T + T 2 + 1 2 β Ξ¦ a ( Ο ) ) Β < Β β , \int_{[0,t]}|e^\gamma_s(\omega)|\,ds\ \le\ 2\Lambda\int_{[0,t]}\big(|\mathfrak{s}_s(\omega)|+|\mathfrak{a}_s(\omega)|\big)\,ds\ \le\ 2\Lambda\,\Big(2\sqrt{N}\,T+\tfrac{T}{2}+\tfrac{1}{2}\,\Phi_{\mathfrak{a}}(\omega)\Big)\ <\ \infty , β« [ 0 , t ] β β£ e s Ξ³ β ( Ο ) β£ d s Β β€ Β 2Ξ β« [ 0 , t ] β ( β£ s s β ( Ο ) β£ + β£ a s β ( Ο ) β£ ) d s Β β€ Β 2Ξ ( 2 N β T + 2 T β + 2 1 β Ξ¦ a β ( Ο ) ) Β < Β β ,
and moreover, by the second bound of clause (a),
β« [ 0 , t ] ( e s Ξ³ ( Ο ) ) 2 β d s Β β€ Β 4 Ξ 2 β« [ 0 , t ] ( β£ s s ( Ο ) β£ 2 + β£ a s ( Ο ) β£ 2 ) β d s Β β€ Β 4 Ξ 2 ( 4 N β T + Ξ¦ a ( Ο ) ) Β < Β β , \int_{[0,t]}\big(e^\gamma_s(\omega)\big)^2\,ds\ \le\ 4\Lambda^2\int_{[0,t]}\big(|\mathfrak{s}_s(\omega)|^2+|\mathfrak{a}_s(\omega)|^2\big)\,ds\ \le\ 4\Lambda^2\big(4N\,T+\Phi_{\mathfrak{a}}(\omega)\big)\ <\ \infty , β« [ 0 , t ] β ( e s Ξ³ β ( Ο ) ) 2 d s Β β€ Β 4 Ξ 2 β« [ 0 , t ] β ( β£ s s β ( Ο ) β£ 2 + β£ a s β ( Ο ) β£ 2 ) d s Β β€ Β 4 Ξ 2 ( 4 N T + Ξ¦ a β ( Ο ) ) Β < Β β ,
both by monotonicity (using β£ e s Ξ³ β£ 2 β€ β£ e s β£ 2 β€ 4 Ξ 2 β£ z s β£ 2 = 4 Ξ 2 ( β£ s s β£ 2 + β£ a s β£ 2 ) |e^\gamma_s|^2\le|e_s|^2\le4\Lambda^2|z_s|^2=4\Lambda^2(|\mathfrak{s}_s|^2+|\mathfrak{a}_s|^2) β£ e s Ξ³ β β£ 2 β€ β£ e s β β£ 2 β€ 4 Ξ 2 β£ z s β β£ 2 = 4 Ξ 2 ( β£ s s β β£ 2 + β£ a s β β£ 2 ) ); so each section is Lebesgue integrable over [ 0 , t ] [0,t] [ 0 , t ] , with square-integrable modulus, and R t \mathcal{R}_t R t β is defined as in the statement. Each R t Ξ³ \mathcal{R}^\gamma_t R t Ξ³ β is a random variable : by the Tonelli theorem the integrals over [ 0 , t ] [0,t] [ 0 , t ] of ( 1 Ξ© 0 e Ξ³ ) Β± (\mathbf{1}_{\Omega_0}e^\gamma)^{\pm} ( 1 Ξ© 0 β β e Ξ³ ) Β± define measurable [ 0 , β ] [0,\infty] [ 0 , β ] -valued functions of Ο \omega Ο , finite on Ξ© a \Omega_{\mathfrak{a}} Ξ© a β by the first bound just displayed, and R t Ξ³ \mathcal{R}^\gamma_t R t Ξ³ β is the difference of the functions equal to them on Ξ© a \Omega_{\mathfrak{a}} Ξ© a β and to 0 0 0 off Ξ© a \Omega_{\mathfrak{a}} Ξ© a β .
Step 3: integral form (clause (c)). Let Ξ© β = Ξ© a \Omega_*=\Omega_{\mathfrak{a}} Ξ© β β = Ξ© a β , an event of probability 1 1 1 (Step 2) contained in Ξ© 0 \Omega_0 Ξ© 0 β , on which clause (a) of the martingale decomposition applies. Fix Ο β Ξ© β \omega\in\Omega_* Ο β Ξ© β β , Ξ³ β { 1 , β¦ , l } \gamma\in\{1,\dots,l\} Ξ³ β { 1 , β¦ , l } , and t β [ 0 , T ] t\in[0,T] t β [ 0 , T ] . First, the relevant sections are measurable and integrable over [ 0 , t ] [0,t] [ 0 , t ] at Ο \omega Ο : the path s β¦ b Ξ³ ( Ξ£ s , Ξ± s ) s\mapsto b^\gamma(\Sigma_s,\alpha_s) s β¦ b Ξ³ ( Ξ£ s β , Ξ± s β ) is measurable and bounded in absolute value by 2 ( l β 1 ) B 2(l-1)B 2 ( l β 1 ) B by clause (a) of the martingale decomposition; the function s β¦ b Ξ³ ( S s , A s ) s\mapsto b^\gamma(S_s,A_s) s β¦ b Ξ³ ( S s β , A s β ) is continuous β this is part of clause 2 of the mean-field trajectory pair β hence measurable , and bounded in absolute value by 2 ( l β 1 ) B 2(l-1)B 2 ( l β 1 ) B as well, since by the definition of the aggregate state drift b Ξ³ ( Ξ£ , Ξ± ) b^\gamma(\Sigma,\alpha) b Ξ³ ( Ξ£ , Ξ± ) is a sum over the l β 1 l-1 l β 1 states Ο β Ξ³ \sigma\neq\gamma Ο ξ = Ξ³ of terms Ξ£ Ο Ξ² ( Ο , Ξ³ , Ξ£ , Ξ± ) β Ξ£ Ξ³ Ξ² ( Ξ³ , Ο , Ξ£ , Ξ± ) \Sigma^\sigma\beta(\sigma,\gamma,\Sigma,\alpha)-\Sigma^\gamma\beta(\gamma,\sigma,\Sigma,\alpha) Ξ£ Ο Ξ² ( Ο , Ξ³ , Ξ£ , Ξ± ) β Ξ£ Ξ³ Ξ² ( Ξ³ , Ο , Ξ£ , Ξ± ) with 0 β€ Ξ£ Ο , Ξ£ Ξ³ β€ 1 0\le\Sigma^\sigma,\Sigma^\gamma\le1 0 β€ Ξ£ Ο , Ξ£ Ξ³ β€ 1 on Ξ l \Delta^l Ξ l and β£ Ξ² β£ β€ B |\beta|\le B β£ Ξ² β£ β€ B by the rate bound of the transition-rate family , so that β£ b Ξ³ β£ β€ 2 ( l β 1 ) B |b^\gamma|\le2(l-1)B β£ b Ξ³ β£ β€ 2 ( l β 1 ) B at every point of Ξ l Γ A \Delta^l\times\mathcal{A} Ξ l Γ A ; hence s β¦ g s Ξ³ ( Ο ) s\mapsto g^\gamma_s(\omega) s β¦ g s Ξ³ β ( Ο ) is measurable and bounded by 4 ( l β 1 ) B N 4(l-1)B\sqrt{N} 4 ( l β 1 ) B N β , and integrable over [ 0 , t ] [0,t] [ 0 , t ] ; the section s β¦ e s Ξ³ ( Ο ) s\mapsto e^\gamma_s(\omega) s β¦ e s Ξ³ β ( Ο ) is measurable and integrable by Step 2; and the section s β¦ ( E s s s + B s a s ) Ξ³ ( Ο ) = g s Ξ³ ( Ο ) β e s Ξ³ ( Ο ) s\mapsto(E_s\mathfrak{s}_s+\mathsf{B}_s\mathfrak{a}_s)^\gamma(\omega)=g^\gamma_s(\omega)-e^\gamma_s(\omega) s β¦ ( E s β s s β + B s β a s β ) Ξ³ ( Ο ) = g s Ξ³ β ( Ο ) β e s Ξ³ β ( Ο ) is measurable as their difference and dominated by Ξ β β£ z s ( Ο ) β£ \Lambda\,|z_s(\omega)| Ξ β£ z s β ( Ο ) β£ , integrable over [ 0 , t ] [0,t] [ 0 , t ] as in Step 2. Now, by the definition of M Ξ³ M^\gamma M Ξ³ in clause (b) of the martingale decomposition β whose integrand 1 Ξ© 0 β b Ξ³ ( Ξ£ s , Ξ± s ) \mathbf{1}_{\Omega_0}\,b^\gamma(\Sigma_s,\alpha_s) 1 Ξ© 0 β β b Ξ³ ( Ξ£ s β , Ξ± s β ) has section at Ο \omega Ο equal to b Ξ³ ( Ξ£ s , Ξ± s ) b^\gamma(\Sigma_s,\alpha_s) b Ξ³ ( Ξ£ s β , Ξ± s β ) , since Ο β Ξ© β β Ξ© a β Ξ© 0 \omega\in\Omega_*\subseteq\Omega_{\mathfrak{a}}\subseteq\Omega_0 Ο β Ξ© β β β Ξ© a β β Ξ© 0 β β
Ξ£ t Ξ³ = Ξ£ 0 Ξ³ + β« [ 0 , t ] b Ξ³ ( Ξ£ s , Ξ± s ) β d s + M t Ξ³ , \Sigma^\gamma_t=\Sigma^\gamma_0+\int_{[0,t]}b^\gamma(\Sigma_s,\alpha_s)\,ds+M^\gamma_t , Ξ£ t Ξ³ β = Ξ£ 0 Ξ³ β + β« [ 0 , t ] β b Ξ³ ( Ξ£ s β , Ξ± s β ) d s + M t Ξ³ β ,
and by clause 2 of the mean-field trajectory pair , S t Ξ³ = S 0 Ξ³ + β« 0 t b Ξ³ ( S s , A s ) β d s S^\gamma_t=S^\gamma_0+\int_0^tb^\gamma(S_s,A_s)\,ds S t Ξ³ β = S 0 Ξ³ β + β« 0 t β b Ξ³ ( S s β , A s β ) d s as a Riemann integral , which agrees with the Lebesgue integral over [ 0 , t ] [0,t] [ 0 , t ] by claim 3 of the toolkit , applied for t > 0 t>0 t > 0 to the restriction of the continuous integrand β continuous by claim 1 of restriction stability β (both integrals are 0 0 0 for t = 0 t=0 t = 0 ). Subtracting and multiplying by N \sqrt{N} N β ,
s t Ξ³ = s 0 Ξ³ + β« [ 0 , t ] g s Ξ³ β d s + N β M t Ξ³ , \mathfrak{s}^\gamma_t=\mathfrak{s}^\gamma_0+\int_{[0,t]}g^\gamma_s\,ds+\sqrt{N}\,M^\gamma_t , s t Ξ³ β = s 0 Ξ³ β + β« [ 0 , t ] β g s Ξ³ β d s + N β M t Ξ³ β ,
and by additivity of the Lebesgue integral (linearity ) applied to the three integrable sections above,
β« [ 0 , t ] g s Ξ³ β d s = β« [ 0 , t ] ( E s s s + B s a s ) Ξ³ β d s + R t Ξ³ atΒ Ο . \int_{[0,t]}g^\gamma_s\,ds=\int_{[0,t]}\big(E_s\mathfrak{s}_s+\mathsf{B}_s\mathfrak{a}_s\big)^\gamma\,ds+\mathcal{R}^\gamma_t\qquad\text{at }\omega. β« [ 0 , t ] β g s Ξ³ β d s = β« [ 0 , t ] β ( E s β s s β + B s β a s β ) Ξ³ d s + R t Ξ³ β atΒ Ο .
Substituting into the previous display gives the identity of clause (c) at every Ο β Ξ© β \omega\in\Omega_* Ο β Ξ© β β , hence almost surely .
Step 4: mean-square bound (clause (d)). Fix t β ( 0 , T ] t\in(0,T] t β ( 0 , T ] (the case t = 0 t=0 t = 0 was disposed of in the preamble). At each Ο β Ξ© a \omega\in\Omega_{\mathfrak{a}} Ο β Ξ© a β and each Ξ³ \gamma Ξ³ , the sections e Ξ³ ( Ο ) e^\gamma(\omega) e Ξ³ ( Ο ) are measurable with β« [ 0 , t ] ( e s Ξ³ ) 2 β d s < β \int_{[0,t]}(e^\gamma_s)^2\,ds<\infty β« [ 0 , t ] β ( e s Ξ³ β ) 2 d s < β (Step 2), so claim 4 (Cauchy--Schwarz) of the interval toolkit , applied to the pair ( 1 , e Ξ³ ) (1,e^\gamma) ( 1 , e Ξ³ ) on [ 0 , t ] [0,t] [ 0 , t ] β the constant function 1 1 1 being measurable with β« [ 0 , t ] 1 2 β d s = t < β \int_{[0,t]}1^2\,ds=t<\infty β« [ 0 , t ] β 1 2 d s = t < β β gives ( R t Ξ³ ) 2 = ( β« [ 0 , t ] e s Ξ³ β d s ) 2 β€ t β« [ 0 , t ] ( e s Ξ³ ) 2 β d s (\mathcal{R}^\gamma_t)^2=\big(\int_{[0,t]}e^\gamma_s\,ds\big)^2\le t\int_{[0,t]}(e^\gamma_s)^2\,ds ( R t Ξ³ β ) 2 = ( β« [ 0 , t ] β e s Ξ³ β d s ) 2 β€ t β« [ 0 , t ] β ( e s Ξ³ β ) 2 d s ; summing over Ξ³ \gamma Ξ³ (linearity of the Lebesgue integral ), β£ R t β£ 2 β€ t β« [ 0 , t ] β£ e s β£ 2 β d s |\mathcal{R}_t|^2\le t\int_{[0,t]}|e_s|^2\,ds β£ R t β β£ 2 β€ t β« [ 0 , t ] β β£ e s β β£ 2 d s on Ξ© a \Omega_{\mathfrak{a}} Ξ© a β , while β£ R t β£ 2 = 0 |\mathcal{R}_t|^2=0 β£ R t β β£ 2 = 0 off Ξ© a \Omega_{\mathfrak{a}} Ξ© a β . By Step 1, β£ e s β£ 2 β€ w s |e_s|^2\le w_s β£ e s β β£ 2 β€ w s β at every point, w s w_s w s β being the square of the minimum of the two bounds of clause (a), so, pointwise on Ξ© \Omega Ξ© ,
β£ R t β£ 2 Β β€ Β t β 1 Ξ© a β« [ 0 , t ] w s β d s Β β€ Β t β« [ 0 , t ] 1 Ξ© 0 β w s β d s , |\mathcal{R}_t|^2\ \le\ t\,\mathbf{1}_{\Omega_{\mathfrak{a}}}\int_{[0,t]}w_s\,ds\ \le\ t\int_{[0,t]}\mathbf{1}_{\Omega_0}\,w_s\,ds , β£ R t β β£ 2 Β β€ Β t 1 Ξ© a β β β« [ 0 , t ] β w s β d s Β β€ Β t β« [ 0 , t ] β 1 Ξ© 0 β β w s β d s ,
using Ξ© a β Ξ© 0 \Omega_{\mathfrak{a}}\subseteq\Omega_0 Ξ© a β β Ξ© 0 β . The function β£ R t β£ 2 |\mathcal{R}_t|^2 β£ R t β β£ 2 is a random variable (a continuous function of the random variables R t Ξ³ \mathcal{R}^\gamma_t R t Ξ³ β of Step 2), so taking expectations and using monotonicity and the Tonelli theorem for the product-measurable map 1 Ξ© 0 w \mathbf{1}_{\Omega_0}w 1 Ξ© 0 β β w of Step 2,
E [ β£ R t β£ 2 ] Β β€ Β t β« [ 0 , t ] E [ 1 Ξ© 0 β w s ] β d s Β = Β t β« [ 0 , t ] E [ w s ] β d s , \mathbb{E}\big[|\mathcal{R}_t|^2\big]\ \le\ t\int_{[0,t]}\mathbb{E}\big[\mathbf{1}_{\Omega_0}\,w_s\big]\,ds\ =\ t\int_{[0,t]}\mathbb{E}\big[w_s\big]\,ds , E [ β£ R t β β£ 2 ] Β β€ Β t β« [ 0 , t ] β E [ 1 Ξ© 0 β β w s β ] d s Β = Β t β« [ 0 , t ] β E [ w s β ] d s ,
the last equality because w s w_s w s β is a random variable (a continuous function of the components of z s z_s z s β , again by the composition lemma ) and expectations are unchanged by the 1 Ξ© 0 \mathbf{1}_{\Omega_0} 1 Ξ© 0 β β modification, Ξ© 0 \Omega_0 Ξ© 0 β having probability 1 1 1 , as recorded in clause (a) of the a priori second-moment bound and in clause (d) of the statement. This is the first display of clause (d). The second display follows from w s β€ 9 β l 3 K 2 ( l + m ) 2 4 N β β£ z s β£ 4 w_s\le\frac{9\,l^3K^2(l+m)^2}{4N}\,|z_s|^4 w s β β€ 4 N 9 l 3 K 2 ( l + m ) 2 β β£ z s β β£ 4 pointwise (the minimum is at most its first argument) by monotonicity of the expectation and of the integral, the map s β¦ E [ β£ z s β£ 4 ] s\mapsto\mathbb{E}[|z_s|^4] s β¦ E [ β£ z s β β£ 4 ] being measurable as recorded in the statement.\ β‘ \square β‘