Data. Let l ≥ 2 l\ge2 l ≥ 2 , m ≥ 1 m\ge1 m ≥ 1 and l ~ ≥ 1 \tilde{l}\ge1 l ~ ≥ 1 be natural numbers , and let B ≥ 0 B\ge0 B ≥ 0 , B ~ ≥ 0 \tilde{B}\ge0 B ~ ≥ 0 , K ≥ 0 K\ge0 K ≥ 0 , K ~ ≥ 0 \tilde{K}\ge0 K ~ ≥ 0 , b ‾ > 0 \underline{b}>0 b > 0 , T > 0 T>0 T > 0 , s ∈ ( 0 , T ] s\in(0,T] s ∈ ( 0 , T ] , Λ ≥ 0 \Lambda\ge0 Λ ≥ 0 , M ≥ 0 \mathsf{M}\ge0 M ≥ 0 , Φ ˉ ≥ 0 \bar\Phi\ge0 Φ ˉ ≥ 0 , c 0 ≥ 0 \mathsf{c}_{0}\ge0 c 0 ≥ 0 , c Q ≥ 0 c_{Q}\ge0 c Q ≥ 0 , κ ♯ ≥ 1 \kappa^{\sharp}\ge1 κ ♯ ≥ 1 , C f l w ≥ 0 C_{\mathrm{flw}}\ge0 C flw ≥ 0 , C c t l ≥ 0 C_{\mathrm{ctl}}\ge0 C ctl ≥ 0 , P ≥ 0 \mathsf{P}\ge0 P ≥ 0 and Q ≥ 0 \mathsf{Q}\ge0 Q ≥ 0 be real numbers (the scalar data ). Put
Λ 1 = l + m ( B + K ) , Λ 2 = 3 2 ( l + m ) K , Λ 3 = 3 K l ( l + m ) , Λ E = 2 l ( l − 1 ) l ( B + K ) , Γ = l ( B ~ + K ~ ) , C L i p = l ( l − 1 ) ( Λ 1 + Λ 3 ) , c ⋆ = c Q κ ♯ , \Lambda_{1}=\sqrt{l+m}\,(B+K),\quad \Lambda_{2}=\tfrac32(l+m)K,\quad \Lambda_{3}=3K\sqrt{l(l+m)},\quad \Lambda_{\mathcal{E}}=\sqrt{2}\,l(l-1)\sqrt{l}\,(B+K),\quad \Gamma=\sqrt{l}\,(\tilde{B}+\tilde{K}),\quad C_{\mathrm{Lip}}=l(l-1)(\Lambda_{1}+\Lambda_{3}),\quad \mathsf{c}_{\star}=c_{Q}\kappa^{\sharp}, Λ 1 = l + m ( B + K ) , Λ 2 = 2 3 ( l + m ) K , Λ 3 = 3 K l ( l + m ) , Λ E = 2 l ( l − 1 ) l ( B + K ) , Γ = l ( B ~ + K ~ ) , C Lip = l ( l − 1 ) ( Λ 1 + Λ 3 ) , c ⋆ = c Q κ ♯ ,
C A = 2 ( 1 + 2 l ( l − 1 ) ) exp ( 2 l ( l − 1 ) Λ 1 s ) , C M = 2 Λ 1 s C A + 5 , c w = 1 16 C M , H = 2 Φ ˉ 2 Λ E s . C_{A}=\sqrt{2}\,\bigl(1+2l(l-1)\bigr)\exp\bigl(\sqrt{2}\,l(l-1)\Lambda_{1}s\bigr),\qquad C_{M}=2\Lambda_{1}sC_{A}+5,\qquad c_{\mathrm{w}}=\frac{1}{16\,C_{M}},\qquad H=\sqrt{2}\,\bar\Phi^{2}\Lambda_{\mathcal{E}}\,s . C A = 2 ( 1 + 2 l ( l − 1 ) ) exp ( 2 l ( l − 1 ) Λ 1 s ) , C M = 2 Λ 1 s C A + 5 , c w = 16 C M 1 , H = 2 Φ ˉ 2 Λ E s .
Conventions. Natural numbers are regarded as real numbers, real powers t a = exp ( a log t ) t^{a}=\exp(a\log t) t a = exp ( a log t ) of a real t > 0 t>0 t > 0 are those of Real Power of a Positive Real Number , and exp \exp exp , log \log log , ⋅ \sqrt{\cdot} ⋅ , ⌊ ⋅ ⌋ \lfloor\cdot\rfloor ⌊ ⋅ ⌋ and limits of sequences are as in Real Powers Through the Exponential, and Elementary Asymptotic Tools: Monotonicity, Null Sequences of Negative Powers, Exponential Domination, Integer Rounding, and Square-Root and Exponential Inequalities , whose claims are used freely. For a real t ≥ 0 t\ge0 t ≥ 0 we write t 1 / 2 = t t^{1/2}=\sqrt{t} t 1/2 = t and t 1 / 4 = ( t 1 / 2 ) 1 / 2 t^{1/4}=(t^{1/2})^{1/2} t 1/4 = ( t 1/2 ) 1/2 , consistent with the real powers for t > 0 t>0 t > 0 by claim 1 of that lemma; in particular N 1 / 2 = N N^{1/2}=\sqrt{N} N 1/2 = N , N 1 / 4 = N N^{1/4}=\sqrt{\sqrt{N}} N 1/4 = N , N − 1 / 2 = 1 / N N^{-1/2}=1/\sqrt{N} N − 1/2 = 1/ N , N − 1 / 4 = 1 / N 1 / 4 N^{-1/4}=1/N^{1/4} N − 1/4 = 1/ N 1/4 and N − 1 = 1 / N N^{-1}=1/N N − 1 = 1/ N . Write a ∧ b a\wedge b a ∧ b for the smaller of two real numbers a , b a,b a , b . For real numbers k > 0 k>0 k > 0 and x ≥ 0 x\ge0 x ≥ 0 let
ϖ k ( x ) = x 2 4 k ∧ x 2 \varpi_{k}(x)=\frac{x^{2}}{4k}\wedge\frac{x}{2} ϖ k ( x ) = 4 k x 2 ∧ 2 x
be the Chernoff exponent of that lemma, extended to x = 0 x=0 x = 0 by the same formula. All objects introduced below are real numbers depending on the scalar data and on a natural number N N N , and "u N → u u_{N}\to u u N → u " refers to the sequence ( u N ) N ∈ N (u_{N})_{N\in\mathbb{N}} ( u N ) N ∈ N . Notational cautions: J N J_{N} J N (a natural number, the number of cells per clock) and J N \mathsf{J}_{N} J N (an information majorant) are distinct, as are w N \mathsf{w}_{N} w N and w 1 , N , w 2 , N w_{1,N},w_{2,N} w 1 , N , w 2 , N ; E N ⋆ \mathsf{E}^{\star}_{N} E N ⋆ and e N ⋆ \mathsf{e}^{\star}_{N} e N ⋆ ; m N \mathsf{m}_{N} m N (a move size) and the control dimension m m m ; M \mathsf{M} M and M N M_{N} M N ; D N D_{N} D N and d N d_{N} d N ; B N \mathsf{B}_{N} B N and B B B ; k N \mathsf{k}_{N} k N and K , K ~ K,\tilde{K} K , K ~ ; a N \mathsf{a}_{N} a N and α N \alpha_{N} α N ; and c 0 \mathsf{c}_{0} c 0 , c ⋆ \mathsf{c}_{\star} c ⋆ (scalar data) and c N \mathsf{c}_{N} c N (a derived quantity indexed by N N N ).
The scale set. For N ∈ N N\in\mathbb{N} N ∈ N put
m N = ⌊ N 1 / 16 ⌋ + 1 , D N = N 3 / 64 , A N = 2 ( m N + l ( l − 1 ) ( D N + m N ) ) exp ( 2 l ( l − 1 ) Λ 1 s ) , L N = Λ 1 s A N + 1 , M N = ⌊ L N ⌋ + 1 , \mathsf{m}_{N}=\lfloor N^{1/16}\rfloor+1,\qquad D_{N}=N^{3/64},\qquad A_{N}=\sqrt{2}\,\bigl(\mathsf{m}_{N}+l(l-1)(D_{N}+\mathsf{m}_{N})\bigr)\exp\bigl(\sqrt{2}\,l(l-1)\Lambda_{1}s\bigr),\qquad L_{N}=\Lambda_{1}sA_{N}+1,\qquad M_{N}=\lfloor L_{N}\rfloor+1, m N = ⌊ N 1/16 ⌋ + 1 , D N = N 3/64 , A N = 2 ( m N + l ( l − 1 ) ( D N + m N ) ) exp ( 2 l ( l − 1 ) Λ 1 s ) , L N = Λ 1 s A N + 1 , M N = ⌊ L N ⌋ + 1 ,
R N = ⌊ N ( B s + 1 ) ⌋ + 1 , J N = ⌊ R N N − 3 / 4 ⌋ + 1 , μ N = R N J N , d N = l ( l − 1 ) J N , R_{N}=\lfloor N(Bs+1)\rfloor+1,\qquad J_{N}=\lfloor R_{N}N^{-3/4}\rfloor+1,\qquad \mu_{N}=\frac{R_{N}}{J_{N}},\qquad d_{N}=l(l-1)J_{N}, R N = ⌊ N ( B s + 1 )⌋ + 1 , J N = ⌊ R N N − 3/4 ⌋ + 1 , μ N = J N R N , d N = l ( l − 1 ) J N ,
η N = N − 3 / 8 , δ N = N − 1 / 8 , ζ N = N − 1 / 2 , θ N = ⌊ N 1 / 4 ⌋ + 1 , x N = μ N 1 / 2 N 1 / 32 , \eta_{N}=N^{-3/8},\qquad \delta_{N}=N^{-1/8},\qquad \zeta_{N}=N^{-1/2},\qquad \theta_{N}=\lfloor N^{1/4}\rfloor+1,\qquad x_{N}=\mu_{N}^{1/2}N^{1/32}, η N = N − 3/8 , δ N = N − 1/8 , ζ N = N − 1/2 , θ N = ⌊ N 1/4 ⌋ + 1 , x N = μ N 1/2 N 1/32 ,
ε S , N = ( C f l w + 1 ) N − 1 / 4 , ε c t l , N = C L i p ( T C c t l ) 1 / 2 N − 1 / 4 , w 1 , N = N ( Λ 1 s ε S , N + ε c t l , N ) , w 2 , N = μ N . \varepsilon_{S,N}=(C_{\mathrm{flw}}+1)N^{-1/4},\qquad \varepsilon_{\mathrm{ctl},N}=C_{\mathrm{Lip}}(TC_{\mathrm{ctl}})^{1/2}N^{-1/4},\qquad w_{1,N}=N\bigl(\Lambda_{1}s\,\varepsilon_{S,N}+\varepsilon_{\mathrm{ctl},N}\bigr),\qquad w_{2,N}=\mu_{N}. ε S , N = ( C flw + 1 ) N − 1/4 , ε ctl , N = C Lip ( T C ctl ) 1/2 N − 1/4 , w 1 , N = N ( Λ 1 s ε S , N + ε ctl , N ) , w 2 , N = μ N .
Derived quantities. For N ∈ N N\in\mathbb{N} N ∈ N put
ε 0 , N = Γ A N N b ‾ , E ˉ N = l ~ s Γ 2 A N 2 N b ‾ , c N = exp ( E ˉ N ) − 1 , E N ⋆ = l ~ s N B ~ ε 0 , N 2 , e N ⋆ = 1 2 ( E N ⋆ ) 2 exp ( E N ⋆ ) + E N ⋆ ( exp ( 9 E N ⋆ ) − 1 ) 1 / 2 , \varepsilon_{0,N}=\frac{\Gamma A_{N}}{N\underline{b}},\qquad \bar{E}_{N}=\frac{\tilde{l}\,s\,\Gamma^{2}A_{N}^{2}}{N\underline{b}},\qquad \mathsf{c}_{N}=\exp(\bar{E}_{N})-1,\qquad \mathsf{E}^{\star}_{N}=\tilde{l}\,s\,N\tilde{B}\,\varepsilon_{0,N}^{2},\qquad \mathsf{e}^{\star}_{N}=\tfrac12(\mathsf{E}^{\star}_{N})^{2}\exp(\mathsf{E}^{\star}_{N})+\mathsf{E}^{\star}_{N}\bigl(\exp(9\mathsf{E}^{\star}_{N})-1\bigr)^{1/2}, ε 0 , N = N b Γ A N , E ˉ N = N b l ~ s Γ 2 A N 2 , c N = exp ( E ˉ N ) − 1 , E N ⋆ = l ~ s N B ~ ε 0 , N 2 , e N ⋆ = 2 1 ( E N ⋆ ) 2 exp ( E N ⋆ ) + E N ⋆ ( exp ( 9 E N ⋆ ) − 1 ) 1/2 ,
E N c h = 8 l ~ s N B ~ θ N 2 ε 0 , N 2 , Π ˉ N = d N ( exp ( − ϖ μ N ( x N ) ) + exp ( − θ N δ N / 2 + E N c h ) ) , \mathsf{E}^{\mathrm{ch}}_{N}=8\,\tilde{l}\,s\,N\tilde{B}\,\theta_{N}^{2}\varepsilon_{0,N}^{2},\qquad \bar\Pi_{N}=d_{N}\Bigl(\exp\bigl(-\varpi_{\mu_{N}}(x_{N})\bigr)+\exp\bigl(-\theta_{N}\delta_{N}/2+\mathsf{E}^{\mathrm{ch}}_{N}\bigr)\Bigr), E N ch = 8 l ~ s N B ~ θ N 2 ε 0 , N 2 , Π ˉ N = d N ( exp ( − ϖ μ N ( x N ) ) + exp ( − θ N δ N /2 + E N ch ) ) ,
g N = d N exp ( − ϖ μ N ( μ N − m N ) ) + 2 l ( l − 1 ) ( R N + 1 ) ( M N + 3 ) exp ( − ϖ M N + 2 ( D N − 2 ) ) \mathsf{g}_{N}=d_{N}\exp\bigl(-\varpi_{\mu_{N}}(\mu_{N}-\mathsf{m}_{N})\bigr)+2\,l(l-1)\,(R_{N}+1)(M_{N}+3)\exp\bigl(-\varpi_{M_{N}+2}(D_{N}-2)\bigr) g N = d N exp ( − ϖ μ N ( μ N − m N ) ) + 2 l ( l − 1 ) ( R N + 1 ) ( M N + 3 ) exp ( − ϖ M N + 2 ( D N − 2 ) )
(the formula for g N \mathsf{g}_{N} g N is read for those N N N for which μ N − m N ≥ 0 \mu_{N}-\mathsf{m}_{N}\ge0 μ N − m N ≥ 0 and D N − 2 ≥ 0 D_{N}-2\ge0 D N − 2 ≥ 0 ; for the remaining N N N put g N = 0 \mathsf{g}_{N}=0 g N = 0 ; the formula for Π ˉ N \bar\Pi_{N} Π ˉ N is read for every N N N ),
κ 0 , N = 1 + m N 2 2 μ N exp ( m N 2 μ N ) , j ˉ N = κ 0 , N m N 2 μ N , j N ⋆ = ( ( 1 + j ˉ N ) 1 / 2 + 1 ) j ˉ N 1 / 2 , \kappa_{0,N}=1+\frac{\mathsf{m}_{N}^{2}}{2\mu_{N}}\exp\Bigl(\frac{\mathsf{m}_{N}^{2}}{\mu_{N}}\Bigr),\qquad \bar{\mathsf{j}}_{N}=\frac{\kappa_{0,N}\mathsf{m}_{N}^{2}}{\mu_{N}},\qquad \mathsf{j}^{\star}_{N}=\bigl((1+\bar{\mathsf{j}}_{N})^{1/2}+1\bigr)\bar{\mathsf{j}}_{N}^{1/2}, κ 0 , N = 1 + 2 μ N m N 2 exp ( μ N m N 2 ) , j ˉ N = μ N κ 0 , N m N 2 , j N ⋆ = ( ( 1 + j ˉ N ) 1/2 + 1 ) j ˉ N 1/2 ,
B N = Π ˉ N + d N ( 1 + j ˉ N ) 1 / 2 ( ( d N Π ˉ N ) 1 / 2 + ( c N Π ˉ N ) 1 / 2 ) + g N + g N 1 / 2 d N ( 1 + j ˉ N ) 1 / 2 , \mathsf{B}_{N}=\bar\Pi_{N}+d_{N}(1+\bar{\mathsf{j}}_{N})^{1/2}\Bigl((d_{N}\bar\Pi_{N})^{1/2}+(\mathsf{c}_{N}\bar\Pi_{N})^{1/2}\Bigr)+\mathsf{g}_{N}+\mathsf{g}_{N}^{1/2}\,d_{N}(1+\bar{\mathsf{j}}_{N})^{1/2}, B N = Π ˉ N + d N ( 1 + j ˉ N ) 1/2 ( ( d N Π ˉ N ) 1/2 + ( c N Π ˉ N ) 1/2 ) + g N + g N 1/2 d N ( 1 + j ˉ N ) 1/2 ,
w N = 2 Λ l ( l − 1 ) R N m N , κ N m v = m N 2 N η N , α N = 2 d N c 0 Φ ˉ 2 , k N = α N ( 3 μ N 2 + μ N ) 1 / 4 , \mathsf{w}_{N}=\frac{\sqrt{2}\,\Lambda\,l(l-1)\,R_{N}}{\mathsf{m}_{N}},\qquad \kappa^{\mathrm{mv}}_{N}=\frac{\mathsf{m}_{N}^{2}}{N\eta_{N}},\qquad \alpha_{N}=\sqrt{2d_{N}}\,\mathsf{c}_{0}\bar\Phi^{2},\qquad \mathsf{k}_{N}=\alpha_{N}\bigl(3\mu_{N}^{2}+\mu_{N}\bigr)^{1/4}, w N = m N 2 Λ l ( l − 1 ) R N , κ N mv = N η N m N 2 , α N = 2 d N c 0 Φ ˉ 2 , k N = α N ( 3 μ N 2 + μ N ) 1/4 ,
e F , N = 2 Λ l ( l − 1 ) ( Λ 1 s ε S , N + ε c t l , N ) + 2 Λ l ( l − 1 ) μ N N ( 3 + 2 ( Λ 1 s A N + μ N ) μ N ) , \mathsf{e}_{F,N}=2\Lambda\,l(l-1)\bigl(\Lambda_{1}s\,\varepsilon_{S,N}+\varepsilon_{\mathrm{ctl},N}\bigr)+\frac{2\Lambda\,l(l-1)\,\mu_{N}}{N}\Bigl(3+\frac{2(\Lambda_{1}sA_{N}+\mu_{N})}{\mu_{N}}\Bigr), e F , N = 2Λ l ( l − 1 ) ( Λ 1 s ε S , N + ε ctl , N ) + N 2Λ l ( l − 1 ) μ N ( 3 + μ N 2 ( Λ 1 s A N + μ N ) ) ,
ϵ ψ , N = ( e F , N + 2 l ( l − 1 ) w N N ( D N + Λ 2 s A N 2 N ) + 2 M ( l ( l − 1 ) Λ 3 s ε S , N + ε c t l , N ) ) exp ( Λ E s ) , \epsilon_{\psi,N}=\Bigl(\mathsf{e}_{F,N}+\frac{\sqrt{2}\,l(l-1)\,\mathsf{w}_{N}}{N}\Bigl(D_{N}+\frac{\Lambda_{2}sA_{N}^{2}}{N}\Bigr)+\sqrt{2}\,\mathsf{M}\bigl(l(l-1)\Lambda_{3}s\,\varepsilon_{S,N}+\varepsilon_{\mathrm{ctl},N}\bigr)\Bigr)\exp(\Lambda_{\mathcal{E}}s), ϵ ψ , N = ( e F , N + N 2 l ( l − 1 ) w N ( D N + N Λ 2 s A N 2 ) + 2 M ( l ( l − 1 ) Λ 3 s ε S , N + ε ctl , N ) ) exp ( Λ E s ) ,
κ N = Γ ( 2 M + ϵ ψ , N ) ( 3 l K ~ ε S , N ( M + ϵ ψ , N ) + Γ ϵ ψ , N ) b ‾ + Γ 3 M 2 ε S , N b ‾ 2 , \kappa_{N}=\frac{\Gamma\,(2\mathsf{M}+\epsilon_{\psi,N})\bigl(3l\tilde{K}\,\varepsilon_{S,N}\,(\mathsf{M}+\epsilon_{\psi,N})+\Gamma\,\epsilon_{\psi,N}\bigr)}{\underline{b}}+\frac{\Gamma^{3}\mathsf{M}^{2}\,\varepsilon_{S,N}}{\underline{b}^{2}}, κ N = b Γ ( 2 M + ϵ ψ , N ) ( 3 l K ~ ε S , N ( M + ϵ ψ , N ) + Γ ϵ ψ , N ) + b 2 Γ 3 M 2 ε S , N ,
Q N = ( 1 + ζ N ) ( Q + l ~ s κ N ) + ( 1 + 1 ζ N ) 9 l ~ l 2 K ~ 2 s w N 2 A N 4 4 N 4 b ‾ , \mathsf{Q}_{N}=(1+\zeta_{N})\bigl(\mathsf{Q}+\tilde{l}\,s\,\kappa_{N}\bigr)+\Bigl(1+\frac{1}{\zeta_{N}}\Bigr)\frac{9\,\tilde{l}\,l^{2}\tilde{K}^{2}\,s\,\mathsf{w}_{N}^{2}A_{N}^{4}}{4N^{4}\underline{b}}, Q N = ( 1 + ζ N ) ( Q + l ~ s κ N ) + ( 1 + ζ N 1 ) 4 N 4 b 9 l ~ l 2 K ~ 2 s w N 2 A N 4 ,
J N = ( 1 + δ N ) [ κ 0 , N P + Q N + w N 2 N ( e N ⋆ + E ˉ N ( N − 1 / 2 + c ⋆ N − 1 ) + c N j N ⋆ ) ] + 2 d N w N 2 B N N , I N = ( J N 1 / 2 + 2 w N ( exp ( κ N m v ) − 1 − κ N m v ) 1 / 2 N − 1 / 2 ) 2 , \mathsf{J}_{N}=(1+\delta_{N})\Bigl[\kappa_{0,N}\mathsf{P}+\mathsf{Q}_{N}+\frac{\mathsf{w}_{N}^{2}}{N}\Bigl(\mathsf{e}^{\star}_{N}+\bar{E}_{N}\bigl(N^{-1/2}+\mathsf{c}_{\star}N^{-1}\bigr)+\mathsf{c}_{N}\mathsf{j}^{\star}_{N}\Bigr)\Bigr]+\frac{2d_{N}\mathsf{w}_{N}^{2}\mathsf{B}_{N}}{N},\qquad \mathcal{I}_{N}=\Bigl(\mathsf{J}_{N}^{1/2}+\sqrt{2}\,\mathsf{w}_{N}\bigl(\exp(\kappa^{\mathrm{mv}}_{N})-1-\kappa^{\mathrm{mv}}_{N}\bigr)^{1/2}N^{-1/2}\Bigr)^{2}, J N = ( 1 + δ N ) [ κ 0 , N P + Q N + N w N 2 ( e N ⋆ + E ˉ N ( N − 1/2 + c ⋆ N − 1 ) + c N j N ⋆ ) ] + N 2 d N w N 2 B N , I N = ( J N 1/2 + 2 w N ( exp ( κ N mv ) − 1 − κ N mv ) 1/2 N − 1/2 ) 2 ,
and the error majorants
e 2 , N = c 0 Φ ˉ 2 ( 2 l ( l − 1 ) Λ 2 s c ⋆ 1 / 2 N − 1 / 2 + 2 l ( l − 1 ) Λ 3 s ( ε S , N c ⋆ 1 / 4 + c ⋆ 1 / 2 N − 1 / 2 ) + 2 ε c t l , N c ⋆ 1 / 4 ) , \mathsf{e}_{2,N}=\mathsf{c}_{0}\bar\Phi^{2}\Bigl(\sqrt{2}\,l(l-1)\Lambda_{2}s\,\mathsf{c}_{\star}^{1/2}N^{-1/2}+\sqrt{2}\,l(l-1)\Lambda_{3}s\bigl(\varepsilon_{S,N}\mathsf{c}_{\star}^{1/4}+\mathsf{c}_{\star}^{1/2}N^{-1/2}\bigr)+\sqrt{2}\,\varepsilon_{\mathrm{ctl},N}\,\mathsf{c}_{\star}^{1/4}\Bigr), e 2 , N = c 0 Φ ˉ 2 ( 2 l ( l − 1 ) Λ 2 s c ⋆ 1/2 N − 1/2 + 2 l ( l − 1 ) Λ 3 s ( ε S , N c ⋆ 1/4 + c ⋆ 1/2 N − 1/2 ) + 2 ε ctl , N c ⋆ 1/4 ) ,
Ξ N = ( ( w 1 , N + 3 ) 1 / 2 + ( w 2 , N + 3 ) 1 / 2 ) N 1 / 32 + 4 + ( 8 ( 4096 + 17 R N 4 ) ) 1 / 4 exp ( − N 1 / 32 / 16 ) [ ( 2 ( R N + 1 ) ( w 1 , N + 4 ) ) 1 / 4 + ( 2 ( R N + 1 ) ( w 2 , N + 4 ) ) 1 / 4 ] , e 3 , N = c 0 N l ( l − 1 ) ( 2 + H ) Ξ N , \Xi_{N}=\Bigl((w_{1,N}+3)^{1/2}+(w_{2,N}+3)^{1/2}\Bigr)N^{1/32}+4+\bigl(8(4096+17R_{N}^{4})\bigr)^{1/4}\exp\bigl(-N^{1/32}/16\bigr)\Bigl[\bigl(2(R_{N}+1)(w_{1,N}+4)\bigr)^{1/4}+\bigl(2(R_{N}+1)(w_{2,N}+4)\bigr)^{1/4}\Bigr],\qquad \mathsf{e}_{3,N}=\frac{\mathsf{c}_{0}}{\sqrt{N}}\,l(l-1)\,(\sqrt{2}+H)\,\Xi_{N}, Ξ N = ( ( w 1 , N + 3 ) 1/2 + ( w 2 , N + 3 ) 1/2 ) N 1/32 + 4 + ( 8 ( 4096 + 17 R N 4 ) ) 1/4 exp ( − N 1/32 /16 ) [ ( 2 ( R N + 1 ) ( w 1 , N + 4 ) ) 1/4 + ( 2 ( R N + 1 ) ( w 2 , N + 4 ) ) 1/4 ] , e 3 , N = N c 0 l ( l − 1 ) ( 2 + H ) Ξ N ,
e 4 , N = η N 1 / 2 α N , e 5 , N = 2 ( g N 1 / 4 + ( N − 1 / 2 + c ⋆ N − 1 ) 1 / 4 ) ( c 0 c ⋆ 1 / 4 + k N N ) , \mathsf{e}_{4,N}=\eta_{N}^{1/2}\alpha_{N},\qquad \mathsf{e}_{5,N}=\sqrt{2}\Bigl(\mathsf{g}_{N}^{1/4}+\bigl(N^{-1/2}+\mathsf{c}_{\star}N^{-1}\bigr)^{1/4}\Bigr)\Bigl(\mathsf{c}_{0}\mathsf{c}_{\star}^{1/4}+\frac{\mathsf{k}_{N}}{\sqrt{N}}\Bigr), e 4 , N = η N 1/2 α N , e 5 , N = 2 ( g N 1/4 + ( N − 1/2 + c ⋆ N − 1 ) 1/4 ) ( c 0 c ⋆ 1/4 + N k N ) ,
e i n j , N = 2 l ( l − 1 ) c 0 Λ Φ ˉ 2 ( Λ E s + 1 ) μ N N , a N = 2 c 0 Φ ˉ 2 m N N . \mathsf{e}_{\mathrm{inj},N}=2\,l(l-1)\,\mathsf{c}_{0}\Lambda\bar\Phi^{2}(\Lambda_{\mathcal{E}}s+1)\frac{\mu_{N}}{N},\qquad \mathsf{a}_{N}=\frac{\sqrt{2}\,\mathsf{c}_{0}\bar\Phi^{2}\mathsf{m}_{N}}{\sqrt{N}} . e inj , N = 2 l ( l − 1 ) c 0 Λ Φ ˉ 2 ( Λ E s + 1 ) N μ N , a N = N 2 c 0 Φ ˉ 2 m N .
Then the following hold.
1. (Eventual validity of the constraints.) There is a natural number N c N_{\mathrm{c}} N c such that for every natural number N ≥ N c N\ge N_{\mathrm{c}} N ≥ N c : (i) m N ∈ N \mathsf{m}_{N}\in\mathbb{N} m N ∈ N and N 1 / 16 < m N ≤ 2 N 1 / 16 N^{1/16}<\mathsf{m}_{N}\le2N^{1/16} N 1/16 < m N ≤ 2 N 1/16 ; (ii) R N ∈ N R_{N}\in\mathbb{N} R N ∈ N and N B s < R N NBs<R_{N} NB s < R N , N ≤ R N ≤ ( B s + 2 ) N N\le R_{N}\le(Bs+2)N N ≤ R N ≤ ( B s + 2 ) N ; (iii) J N ∈ N J_{N}\in\mathbb{N} J N ∈ N , 1 2 N 3 / 4 ≤ μ N ≤ N 3 / 4 \tfrac12N^{3/4}\le\mu_{N}\le N^{3/4} 2 1 N 3/4 ≤ μ N ≤ N 3/4 , μ N ≥ 2 \mu_{N}\ge2 μ N ≥ 2 , and N 1 / 4 ≤ d N ≤ l ( l − 1 ) ( B s + 3 ) N 1 / 4 N^{1/4}\le d_{N}\le l(l-1)(Bs+3)N^{1/4} N 1/4 ≤ d N ≤ l ( l − 1 ) ( B s + 3 ) N 1/4 ; (iv) D N ≤ N 1 / 16 < m N D_{N}\le N^{1/16}<\mathsf{m}_{N} D N ≤ N 1/16 < m N , A N ≤ C A m N ≤ 2 C A N 1 / 16 A_{N}\le C_{A}\mathsf{m}_{N}\le2C_{A}N^{1/16} A N ≤ C A m N ≤ 2 C A N 1/16 , 0 ≤ Λ 1 s A N < L N 0\le\Lambda_{1}sA_{N}<L_{N} 0 ≤ Λ 1 s A N < L N , M N ∈ N M_{N}\in\mathbb{N} M N ∈ N , L N < M N ≤ L N + 1 L_{N}<M_{N}\le L_{N}+1 L N < M N ≤ L N + 1 and M N + 2 ≤ M N + 3 ≤ C M N 1 / 16 M_{N}+2\le M_{N}+3\le C_{M}N^{1/16} M N + 2 ≤ M N + 3 ≤ C M N 1/16 ; (v) D N ≥ 4 D_{N}\ge4 D N ≥ 4 , 0 < η N ≤ 1 0<\eta_{N}\le1 0 < η N ≤ 1 , 0 < δ N ≤ 1 0<\delta_{N}\le1 0 < δ N ≤ 1 , ζ N > 0 \zeta_{N}>0 ζ N > 0 , θ N ∈ N \theta_{N}\in\mathbb{N} θ N ∈ N and N 1 / 4 < θ N ≤ 2 N 1 / 4 N^{1/4}<\theta_{N}\le2N^{1/4} N 1/4 < θ N ≤ 2 N 1/4 ; (vi) m N < μ N / 2 \mathsf{m}_{N}<\mu_{N}/2 m N < μ N /2 ; (vii) ε 0 , N ≤ 1 2 \varepsilon_{0,N}\le\tfrac12 ε 0 , N ≤ 2 1 , 2 θ N ε 0 , N ≤ 1 2\theta_{N}\varepsilon_{0,N}\le1 2 θ N ε 0 , N ≤ 1 , E ˉ N ≤ 1 \bar{E}_{N}\le1 E ˉ N ≤ 1 , E N ⋆ ≤ 1 \mathsf{E}^{\star}_{N}\le1 E N ⋆ ≤ 1 , E N c h ≤ 1 \mathsf{E}^{\mathrm{ch}}_{N}\le1 E N ch ≤ 1 , j ˉ N ≤ 1 \bar{\mathsf{j}}_{N}\le1 j ˉ N ≤ 1 and κ N m v ≤ 1 \kappa^{\mathrm{mv}}_{N}\le1 κ N mv ≤ 1 ; (viii) m N ( x N + m N ) ≤ δ N μ N / 2 \mathsf{m}_{N}(x_{N}+\mathsf{m}_{N})\le\delta_{N}\mu_{N}/2 m N ( x N + m N ) ≤ δ N μ N /2 . Such an N c N_{\mathrm{c}} N c is fixed for the remainder of the statement.
2. (Chernoff exponents.) For all real k > 0 k>0 k > 0 the map x ↦ ϖ k ( x ) x\mapsto\varpi_{k}(x) x ↦ ϖ k ( x ) is nondecreasing on [ 0 , ∞ ) [0,\infty) [ 0 , ∞ ) , and for every real n ≥ 0 n\ge0 n ≥ 0 and every N ∈ N N\in\mathbb{N} N ∈ N , the number y = ( n + 2 ) 1 / 2 N 1 / 32 y=(n+2)^{1/2}N^{1/32} y = ( n + 2 ) 1/2 N 1/32 satisfies ϖ n + 2 ( y ) ≥ N 1 / 32 / 4 \varpi_{n+2}(y)\ge N^{1/32}/4 ϖ n + 2 ( y ) ≥ N 1/32 /4 . Moreover, for every N ≥ N c N\ge N_{\mathrm{c}} N ≥ N c ,
ϖ μ N ( x N ) ≥ N 1 / 32 4 , ϖ μ N ( μ N − m N ) ≥ μ N 16 ≥ N 3 / 4 32 , ϖ M N + 2 ( D N − 2 ) ≥ c w N 1 / 32 . \varpi_{\mu_{N}}(x_{N})\ge\frac{N^{1/32}}{4},\qquad \varpi_{\mu_{N}}(\mu_{N}-\mathsf{m}_{N})\ge\frac{\mu_{N}}{16}\ge\frac{N^{3/4}}{32},\qquad \varpi_{M_{N}+2}(D_{N}-2)\ge c_{\mathrm{w}}N^{1/32}. ϖ μ N ( x N ) ≥ 4 N 1/32 , ϖ μ N ( μ N − m N ) ≥ 16 μ N ≥ 32 N 3/4 , ϖ M N + 2 ( D N − 2 ) ≥ c w N 1/32 .
3. (Limits.) (a) ε S , N → 0 \varepsilon_{S,N}\to0 ε S , N → 0 , ε c t l , N → 0 \varepsilon_{\mathrm{ctl},N}\to0 ε ctl , N → 0 , ε 0 , N → 0 \varepsilon_{0,N}\to0 ε 0 , N → 0 , E ˉ N → 0 \bar{E}_{N}\to0 E ˉ N → 0 , c N → 0 \mathsf{c}_{N}\to0 c N → 0 , e N ⋆ → 0 \mathsf{e}^{\star}_{N}\to0 e N ⋆ → 0 , κ 0 , N → 1 \kappa_{0,N}\to1 κ 0 , N → 1 , j ˉ N → 0 \bar{\mathsf{j}}_{N}\to0 j ˉ N → 0 , j N ⋆ → 0 \mathsf{j}^{\star}_{N}\to0 j N ⋆ → 0 , Π ˉ N → 0 \bar\Pi_{N}\to0 Π ˉ N → 0 , g N → 0 \mathsf{g}_{N}\to0 g N → 0 , e F , N → 0 \mathsf{e}_{F,N}\to0 e F , N → 0 , ϵ ψ , N → 0 \epsilon_{\psi,N}\to0 ϵ ψ , N → 0 , κ N → 0 \kappa_{N}\to0 κ N → 0 , Q N → Q \mathsf{Q}_{N}\to\mathsf{Q} Q N → Q , 2 d N w N 2 B N N → 0 \frac{2d_{N}\mathsf{w}_{N}^{2}\mathsf{B}_{N}}{N}\to0 N 2 d N w N 2 B N → 0 and J N → P + Q \mathsf{J}_{N}\to\mathsf{P}+\mathsf{Q} J N → P + Q . (b) e 2 , N → 0 \mathsf{e}_{2,N}\to0 e 2 , N → 0 , e 3 , N → 0 \mathsf{e}_{3,N}\to0 e 3 , N → 0 , e 4 , N → 0 \mathsf{e}_{4,N}\to0 e 4 , N → 0 , e 5 , N → 0 \mathsf{e}_{5,N}\to0 e 5 , N → 0 , e i n j , N → 0 \mathsf{e}_{\mathrm{inj},N}\to0 e inj , N → 0 and a N → 0 \mathsf{a}_{N}\to0 a N → 0 . (c) I N → P + Q \mathcal{I}_{N}\to\mathsf{P}+\mathsf{Q} I N → P + Q .
4. (Eventual smallness.) For every real ϵ > 0 \epsilon>0 ϵ > 0 there is a natural number N s c ≥ N c N_{\mathrm{sc}}\ge N_{\mathrm{c}} N sc ≥ N c such that for every natural number N ≥ N s c N\ge N_{\mathrm{sc}} N ≥ N sc ,
e 2 , N + e 3 , N + e 4 , N + e 5 , N ≤ ϵ , e i n j , N ≤ ϵ , a N ≤ ϵ , I N ≤ P + Q + ϵ , g N ≤ ϵ . \mathsf{e}_{2,N}+\mathsf{e}_{3,N}+\mathsf{e}_{4,N}+\mathsf{e}_{5,N}\le\epsilon,\qquad \mathsf{e}_{\mathrm{inj},N}\le\epsilon,\qquad \mathsf{a}_{N}\le\epsilon,\qquad \mathcal{I}_{N}\le\mathsf{P}+\mathsf{Q}+\epsilon,\qquad \mathsf{g}_{N}\le\epsilon . e 2 , N + e 3 , N + e 4 , N + e 5 , N ≤ ϵ , e inj , N ≤ ϵ , a N ≤ ϵ , I N ≤ P + Q + ϵ , g N ≤ ϵ .