TheoremBase

Proof

Throughout, "the ledger lemma" is the ledger decomposition lemma, "the energy lemma" is the tracked energy bound lemma, "the cascade lemma" is the block cascade lemma and "the squares theorem" is the completion-of-squares theorem. For an admissible π\pi we write KK, tkt_{k}, LkL_{k}, Λ⋆\Lambda_{\star}, Υesc\Upsilon_{\mathrm{esc}}, Υlev\Upsilon_{\mathrm{lev}}, Z\mathcal{Z}, Str\mathcal{S}^{\mathrm{tr}}, P\mathcal{P}, N\mathcal{N}, BN\mathcal{B}_{N}, Tknr(s)\mathcal{T}^{\mathrm{nr}}_{k}(s) and CΨC_{\Psi}, CNC_{\mathcal{N}} for the corresponding objects of the ledger lemma formed from π\pi for the NN-th solution. Since admissibility is exactly the conjunction of the parameter-dependent requirements of the ledger lemma, and the parameter-free standing hypotheses are assumed here, the ledger lemma and everything it adopts — in particular the energy lemma and the cascade lemma — apply to the NN-th solution for every admissible π\pi and every NN.

Conclusion (a). Fix an admissible π\pi satisfying the absorption condition. Write, as in claim 4 of the energy lemma,

RN=2Ctg∨cQ1/2κ01/2K+2ϵ cQ1/2κ01/2+4R2T c⋆ cQκ0q0−4N−1+2N(CDT+CDG)cQκ0q0−4N−2.\mathcal{R}_{N}=2C^{\vee}_{tg}c_{Q}^{1/2}\kappa_{0}^{1/2}\sqrt{K}+2\epsilon\,c_{Q}^{1/2}\kappa_{0}^{1/2}+4R^{2}T\,c_{\star}\,c_{Q}\kappa_{0}q_{0}^{-4}N^{-1}+2N\bigl(C_{\mathcal{D}}T+C_{\mathcal{D}G}\bigr)c_{Q}\kappa_{0}q_{0}^{-4}N^{-2}.

By (I′'), κ0≤κ♯\kappa_{0}\le\kappa^{\sharp} for every NN, so the last two summands are at most (4R2Tc⋆+2CDT+2CDG)cQκ♯q0−4N−1\bigl(4R^{2}Tc_{\star}+2C_{\mathcal{D}}T+2C_{\mathcal{D}G}\bigr)c_{Q}\kappa^{\sharp}q_{0}^{-4}N^{-1}, a fixed constant times N−1N^{-1}; choose a natural number N1′N_{1}' beyond which their sum is at most 11. Then, for N≥N1′N\ge N_{1}', and using ϵ≤1\epsilon\le1,

RN ≤ R♯:=2Ctg∨cQ1/2(κ♯)1/2K+2 cQ1/2(κ♯)1/2+1,\mathcal{R}_{N}\ \le\ \mathcal{R}^{\sharp}:=2C^{\vee}_{tg}c_{Q}^{1/2}(\kappa^{\sharp})^{1/2}\sqrt{K}+2\,c_{Q}^{1/2}(\kappa^{\sharp})^{1/2}+1 ,

a real independent of NN.

Step 1: a crude NN-free bound. The absorption condition is the hypothesis of claim 5 of the energy lemma, and JN≤J♯\mathcal{J}_{N}\le\mathcal{J}^{\sharp} by (CB). That claim therefore gives, for every N≥N1′N\ge N_{1}',

Z ≤ C†♯:=2c⋆(J♯+R♯)+128(CnsΛ⋆3/4Υesc)4c⋆4,\mathcal{Z}\ \le\ C^{\sharp}_{\dagger}:=\frac{2}{c_{\star}}\bigl(\mathcal{J}^{\sharp}+\mathcal{R}^{\sharp}\bigr)+\frac{128\bigl(C_{ns}\Lambda_{\star}^{3/4}\Upsilon_{\mathrm{esc}}\bigr)^{4}}{c_{\star}^{4}},

a finite real not depending on NN (the right-hand side of claim 5 is nondecreasing in RN\mathcal{R}_{N} and in J♯\mathcal{J}^{\sharp}).

Step 2: absorption at large NN. By Step 1 and the monotonicity of x↦x3/4x\mapsto x^{3/4} on [0,∞)[0,\infty),

Cns(Λ⋆Z)3/4N−1/4Υesc ≤ Cns(Λ⋆C†♯)3/4Υesc N−1/4(N≥N1′),C_{ns}\bigl(\Lambda_{\star}\mathcal{Z}\bigr)^{3/4}N^{-1/4}\Upsilon_{\mathrm{esc}}\ \le\ C_{ns}\bigl(\Lambda_{\star}C^{\sharp}_{\dagger}\bigr)^{3/4}\Upsilon_{\mathrm{esc}}\,N^{-1/4}\qquad(N\ge N_{1}'),

and the right-hand side tends to 00; choose N1≥N1′N_{1}\ge N_{1}' beyond which it is at most 11. For N≥N1N\ge N_{1}, claim 4 of the energy lemma and (CB) give

c⋆Z ≤ J♯+(2Ctg∨Λ⋆+2ϵCS2)Z+1+R♯ ≤ J♯+c⋆4Z+1+R♯,c_{\star}\mathcal{Z}\ \le\ \mathcal{J}^{\sharp}+\bigl(2C^{\vee}_{tg}\Lambda_{\star}+2\epsilon C_{S}^{2}\bigr)\mathcal{Z}+1+\mathcal{R}^{\sharp}\ \le\ \mathcal{J}^{\sharp}+\tfrac{c_{\star}}{4}\mathcal{Z}+1+\mathcal{R}^{\sharp},

by the absorption condition. Since Z\mathcal{Z} is finite (claim 1 of the energy lemma), the term c⋆4Z\tfrac{c_{\star}}{4}\mathcal{Z} may be subtracted, giving 34c⋆Z≤J♯+1+R♯\tfrac{3}{4}c_{\star}\mathcal{Z}\le\mathcal{J}^{\sharp}+1+\mathcal{R}^{\sharp}, that is Z≤Z♯(π)\mathcal{Z}\le\mathcal{Z}^{\sharp}(\pi) after substituting the value of R♯\mathcal{R}^{\sharp}. Finally claim 1(b) of the ledger lemma and (I′') give

Str+Z ≤ (1+2CS2T)Z+2T cQ1/2κ01/2 ≤ W♯(π).\mathcal{S}^{\mathrm{tr}}+\mathcal{Z}\ \le\ \bigl(1+2C_{S}^{2}T\bigr)\mathcal{Z}+2T\,c_{Q}^{1/2}\kappa_{0}^{1/2}\ \le\ W^{\sharp}(\pi).

Conclusion (b). Let ε′>0\varepsilon'>0. We choose the entries of π\pi in the following order; at each step the quantities already fixed are treated as constants.

Step 1 (T0T_{0}, λc\lambda_{c}, λo\lambda_{o}). Put λc=λo=T0\lambda_{c}=\lambda_{o}=T_{0}, so that Λ⋆=max⁡(4Ca2K22T0,T0)=c1T0\Lambda_{\star}=\max(4C_{a}^{2}K_{2}^{2}T_{0},T_{0})=c_{1}T_{0} with c1=max⁡(4Ca2K22,1)c_{1}=\max(4C_{a}^{2}K_{2}^{2},1), a constant of the common data. By claim 1 of the cascade lemma KK is the least natural number with KT0≥TKT_{0}\ge T, so K≤TT0−1+1K\le TT_{0}^{-1}+1 and K≤(TT0−1+1)1/2\sqrt{K}\le(TT_{0}^{-1}+1)^{1/2}, whence

Λ⋆ Z♯(π) ≤ 4c13c⋆(T0(J♯+2+2cQ1/2(κ♯)1/2)+2Ctg∨cQ1/2(κ♯)1/2 T01/2(T+T0)1/2),\Lambda_{\star}\,\mathcal{Z}^{\sharp}(\pi)\ \le\ \frac{4c_{1}}{3c_{\star}}\Bigl(T_{0}\bigl(\mathcal{J}^{\sharp}+2+2c_{Q}^{1/2}(\kappa^{\sharp})^{1/2}\bigr)+2C^{\vee}_{tg}c_{Q}^{1/2}(\kappa^{\sharp})^{1/2}\,T_{0}^{1/2}(T+T_{0})^{1/2}\Bigr),

using T0(TT0−1+1)1/2=T01/2(T+T0)1/2T_{0}(TT_{0}^{-1}+1)^{1/2}=T_{0}^{1/2}(T+T_{0})^{1/2}. The right-hand side tends to 00 as T0T_{0} decreases to 00. Choose T0∈(0,T]T_{0}\in(0,T] so small that

2(Ctg∨+lCZ)Λ⋆Z♯(π)≤ε′6and2Ctg∨Λ⋆≤c⋆8.2\bigl(C^{\vee}_{tg}+lC_{Z}\bigr)\Lambda_{\star}\mathcal{Z}^{\sharp}(\pi)\le\frac{\varepsilon'}{6}\qquad\text{and}\qquad 2C^{\vee}_{tg}\Lambda_{\star}\le\frac{c_{\star}}{8}.

This fixes KK, the grid tkt_{k}, and the numbers Z♯(π)\mathcal{Z}^{\sharp}(\pi) and W♯(π)W^{\sharp}(\pi), none of which depends on the remaining entries of π\pi.

Step 2 (ϵ\epsilon). Choose ϵ∈(0,1]\epsilon\in(0,1] with 2ϵ(CS2Z♯(π)+cQ1/2(κ♯)1/2)≤ε′/62\epsilon\bigl(C_{S}^{2}\mathcal{Z}^{\sharp}(\pi)+c_{Q}^{1/2}(\kappa^{\sharp})^{1/2}\bigr)\le\varepsilon'/6 and 2ϵCS2≤c⋆/82\epsilon C_{S}^{2}\le c_{\star}/8. Together with Step 1 this gives the absorption condition 2Ctg∨Λ⋆+2ϵCS2≤c⋆/42C^{\vee}_{tg}\Lambda_{\star}+2\epsilon C_{S}^{2}\le c_{\star}/4. Fix ρG∗>0\rho^{*}_{G}>0 for this ϵ\epsilon as prescribed in the ledger lemma.

Step 3 (η\eta, ϱ\varrho). Choose η>0\eta>0 with η W♯(π)≤ε′/6\eta\,W^{\sharp}(\pi)\le\varepsilon'/6, fix a radius ρη>0\rho_{\eta}>0 for it as in the ledger lemma, and put ϱ=ρη/2\varrho=\rho_{\eta}/2.

Step 4 (δcl\delta_{\mathrm{cl}}). Choose δcl∈(0,ρ∗/2]\delta_{\mathrm{cl}}\in(0,\rho^{*}/2].

Step 5 (ε1\varepsilon_{1}, q0q_{0}). All of the following hold as soon as the positive real ε1+q0\varepsilon_{1}+q_{0} is small enough, each condition being satisfied on an interval (0,c](0,c] for some c>0c>0 determined by the quantities already fixed: (ε1+q0)2+δcl2≤(ρ∗)2(\varepsilon_{1}+q_{0})^{2}+\delta_{\mathrm{cl}}^{2}\le(\rho^{*})^{2} (possible since δcl≤ρ∗/2\delta_{\mathrm{cl}}\le\rho^{*}/2), C3(ε1+q0)2≤r04δcl2C_{3}(\varepsilon_{1}+q_{0})^{2}\le\tfrac{r_{0}}{4}\delta_{\mathrm{cl}}^{2}, ε1+q0≤εtg\varepsilon_{1}+q_{0}\le\varepsilon_{tg} — these three are (SM) — together with ε1+q0≤ρG∗\varepsilon_{1}+q_{0}\le\rho^{*}_{G}, with (ε1+q0)2+ϱ2≤ρη2(\varepsilon_{1}+q_{0})^{2}+\varrho^{2}\le\rho_{\eta}^{2}, which is (SN) and holds as soon as (ε1+q0)2≤34ρη2(\varepsilon_{1}+q_{0})^{2}\le\tfrac{3}{4}\rho_{\eta}^{2}, and with

2lCZce(ε1+q0) W♯(π)+CΨ Z♯(π)(ε1+q0ϱ+(ε1+q0)2ϱ2) ≤ ε′6.2lC_{Z}c_{e}(\varepsilon_{1}+q_{0})\,W^{\sharp}(\pi)+C_{\Psi}\,\mathcal{Z}^{\sharp}(\pi)\Bigl(\frac{\varepsilon_{1}+q_{0}}{\varrho}+\frac{(\varepsilon_{1}+q_{0})^{2}}{\varrho^{2}}\Bigr)\ \le\ \frac{\varepsilon'}{6}.

Choose ε1>0\varepsilon_{1}>0 and q0>0q_{0}>0 accordingly. The tuple π\pi is now admissible and satisfies the absorption condition, and it determines Υesc\Upsilon_{\mathrm{esc}} and Υlev\Upsilon_{\mathrm{lev}}, which are finite positive reals independent of NN.

Step 6 (N0N_{0}). Let N1N_{1} be as in conclusion (a) for this π\pi. By claim 1 of the energy lemma, P(N)≤cQκ0q0−4N−2≤cQκ♯q0−4N−2P(\mathcal{N})\le c_{Q}\kappa_{0}q_{0}^{-4}N^{-2}\le c_{Q}\kappa^{\sharp}q_{0}^{-4}N^{-2}, so NP(N)≤cQκ♯q0−4N−1NP(\mathcal{N})\le c_{Q}\kappa^{\sharp}q_{0}^{-4}N^{-1}; and by claim 1(d) of the ledger lemma together with conclusion (a), P≤Λ⋆Z♯(π)ΥlevN−1\mathcal{P}\le\Lambda_{\star}\mathcal{Z}^{\sharp}(\pi)\Upsilon_{\mathrm{lev}}N^{-1} for N≥N1N\ge N_{1}. Each of the four quantities

2(Ctg∨+lCZ)cQ1/2(κ♯)1/2P1/2,Cns(Λ⋆Z♯(π))3/4N−1/4Υesc,l2CZ(12cΘN−1/2(T+W♯(π))+ΘˉTP),CNcQκ♯q0−4N−12\bigl(C^{\vee}_{tg}+lC_{Z}\bigr)c_{Q}^{1/2}(\kappa^{\sharp})^{1/2}\mathcal{P}^{1/2},\quad C_{ns}\bigl(\Lambda_{\star}\mathcal{Z}^{\sharp}(\pi)\bigr)^{3/4}N^{-1/4}\Upsilon_{\mathrm{esc}},\quad l^{2}C_{Z}\Bigl(\tfrac{1}{2}c_{\Theta}N^{-1/2}\bigl(T+W^{\sharp}(\pi)\bigr)+\bar{\Theta}T\mathcal{P}\Bigr),\quad C_{\mathcal{N}}c_{Q}\kappa^{\sharp}q_{0}^{-4}N^{-1}

is therefore bounded by a constant independent of NN times a strictly negative power of NN — for the first and third this uses the substitution of the bound P≤Λ⋆Z♯(π)ΥlevN−1\mathcal{P}\le\Lambda_{\star}\mathcal{Z}^{\sharp}(\pi)\Upsilon_{\mathrm{lev}}N^{-1} just displayed, which turns P1/2\mathcal{P}^{1/2} into a constant times N−1/2N^{-1/2} and P\mathcal{P} into a constant times N−1N^{-1} — so all four tend to 00. Moreover P(Ω0)=1P(\Omega_{0})=1 and ∣s0∣≤2N|\mathfrak{s}_{0}|\le2\sqrt{N}, so E[1Ω0s0⋅Z0s0]=∑γ,δZ0γδE[s0γs0δ]\mathbb{E}[\mathbf{1}_{\Omega_{0}}\mathfrak{s}_{0}\cdot Z_{0}\mathfrak{s}_{0}]=\sum_{\gamma,\delta}Z^{\gamma\delta}_{0}\mathbb{E}[\mathfrak{s}^{\gamma}_{0}\mathfrak{s}^{\delta}_{0}] by linearity of the expectation, and by (I) each of the l2l^{2} summands converges to Z0γδΠ0γδZ^{\gamma\delta}_{0}\Pi^{\gamma\delta}_{0}. Choose N0≥N1N_{0}\ge N_{1} so that for every N≥N0N\ge N_{0} the sum of the four displayed quantities is at most ε′/6\varepsilon'/6 and

∣E[1Ω0s0⋅Z0s0]−∑γ,δZ0γδΠ0γδ∣ ≤ ε′6.\Bigl|\mathbb{E}\bigl[\mathbf{1}_{\Omega_{0}}\mathfrak{s}_{0}\cdot Z_{0}\mathfrak{s}_{0}\bigr]-\sum_{\gamma,\delta}Z^{\gamma\delta}_{0}\Pi^{\gamma\delta}_{0}\Bigr|\ \le\ \frac{\varepsilon'}{6}.

Conclusion. Let N≥N0N\ge N_{0}. By conclusion (a), Z≤Z♯(π)\mathcal{Z}\le\mathcal{Z}^{\sharp}(\pi) and Str+Z≤W♯(π)\mathcal{S}^{\mathrm{tr}}+\mathcal{Z}\le W^{\sharp}(\pi). Every summand of BN\mathcal{B}_{N} is nondecreasing in Z\mathcal{Z}, in Str+Z\mathcal{S}^{\mathrm{tr}}+\mathcal{Z}, in P\mathcal{P} and in κ0\kappa_{0}, so, grouping the summands of BN\mathcal{B}_{N} as in Steps 1, 2, 3, 5 and 6 and using the five displayed bounds,

BN ≤ ηW♯+(2lCZce(ε1+q0)W♯+CΨZ♯(ε1+q0ϱ+(ε1+q0)2ϱ2))+2ϵ(CS2Z♯+cQ1/2(κ♯)1/2)+2(Ctg∨+lCZ)Λ⋆Z♯+ε′6 ≤ 5ε′6.\mathcal{B}_{N}\ \le\ \eta W^{\sharp}+\Bigl(2lC_{Z}c_{e}(\varepsilon_{1}+q_{0})W^{\sharp}+C_{\Psi}\mathcal{Z}^{\sharp}\bigl(\tfrac{\varepsilon_{1}+q_{0}}{\varrho}+\tfrac{(\varepsilon_{1}+q_{0})^{2}}{\varrho^{2}}\bigr)\Bigr)+2\epsilon\bigl(C_{S}^{2}\mathcal{Z}^{\sharp}+c_{Q}^{1/2}(\kappa^{\sharp})^{1/2}\bigr)+2\bigl(C^{\vee}_{tg}+lC_{Z}\bigr)\Lambda_{\star}\mathcal{Z}^{\sharp}+\frac{\varepsilon'}{6}\ \le\ \frac{5\varepsilon'}{6}.

Claim 7 of the ledger lemma gives

JN ≥ E[1Ω0s0⋅Z0s0]+∫[0,T]∑γ,δZsγδΘs⋆γδ ds+∑k=0K−1∫[tk,tk+1]E[1Tknr(s)us⋅Rsus]ds−BN,\mathcal{J}_{N}\ \ge\ \mathbb{E}\bigl[\mathbf{1}_{\Omega_{0}}\mathfrak{s}_{0}\cdot Z_{0}\mathfrak{s}_{0}\bigr]+\int_{[0,T]}\sum_{\gamma,\delta}Z^{\gamma\delta}_{s}\Theta^{\star\gamma\delta}_{s}\,ds+\sum_{k=0}^{K-1}\int_{[t_{k},t_{k+1}]}\mathbb{E}\bigl[\mathbf{1}_{\mathcal{T}^{\mathrm{nr}}_{k}(s)}u_{s}\cdot R_{s}u_{s}\bigr]ds-\mathcal{B}_{N},

and replacing E[1Ω0s0⋅Z0s0]\mathbb{E}[\mathbf{1}_{\Omega_{0}}\mathfrak{s}_{0}\cdot Z_{0}\mathfrak{s}_{0}] by ∑γ,δZ0γδΠ0γδ\sum_{\gamma,\delta}Z^{\gamma\delta}_{0}\Pi^{\gamma\delta}_{0} at the cost of a further ε′/6\varepsilon'/6 gives conclusion (b). The displayed sum is nonnegative by claim 2 of the ledger lemma.

Conclusion (c). Let ε′>0\varepsilon'>0 and let π\pi and N0N_{0} be as furnished by (b). Discarding the nonnegative filtering sum from the inequality of (b) gives JN≥V0−ε′\mathcal{J}_{N}\ge V_{0}-\varepsilon' for every N≥N0N\ge N_{0}, which is the assertion. □\square

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