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Proof of Comparison Principle for Slope-Based Solutions of the Discounted Hopf-Lax Equation on a Complete Metric Space with Interpolation Points

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· 12,614 chars · 17 deps · depth 17 Reason: Proof of comparison for the discounted Hopf-Lax equation by doubling variables and Ekeland.

By contradiction: doubling variables with a quadratic penalty, Ekeland's principle on the product space gives near-maximizers at which the sub- and supersolution tests yield an inequality that the uniform continuity of f makes impossible.

Proof

Each result cited below is universally quantified over the data in its own statement.

Throughout, H(x,r,p)=ρ r+12p2−f(x)H(x,r,p)=\rho\,r+\frac{1}{2}p^{2}-f(x) for x∈Xx\in X, r∈Rr\in\mathbb{R} and p∈Tp\in T is the Hamiltonian Hρ,fH_{\rho,f} on XX of The Discounted Stationary Hopf-Lax Equation on an Open Subset of a Metric Space, so that by The Discounted Stationary Hopf-Lax Equation on an Open Subset of a Metric Space §discounted-hopf-lax the hypotheses say that uu is an s-subsolution and vv an s-supersolution of H=0H=0 in XX. In particular, by Slope-Based Viscosity Subsolutions, Supersolutions and Solutions on a Metric Space §subsolution and Slope-Based Viscosity Subsolutions, Supersolutions and Solutions on a Metric Space §supersolution, uu is upper semicontinuous on XX and vv is lower semicontinuous on XX, and by Slope-Based Viscosity Subsolutions, Supersolutions and Solutions on a Metric Space §hamiltonian we have H(x,r,p)≤H(x,r,p′)H(x,r,p)\le H(x,r,p') whenever p,p′∈Tp,p'\in T and p≤p′p\le p'.

We argue by contradiction. Suppose that there is z∈Xz\in X with v(z)<u(z)v(z)<u(z), and put θ=u(z)−v(z)\theta=u(z)-v(z), a positive real. The constants are chosen in the order MM, β\beta, σ\sigma, γ\gamma, ε\varepsilon of Step 2; the points (x0,y0)(x_{0},y_{0}) and (xε,yε)(x_{\varepsilon},y_{\varepsilon}) of Step 3 are chosen after ε\varepsilon.

Step 1 (the doubled space). Let Z=X×XZ=X\times X and ϱ((x,y),(x′,y′))=d(x,x′)+d(y,y′)\varrho\bigl((x,y),(x',y')\bigr)=d(x,x')+d(y,y'). Conditions 1, 3 and 4 of Metric Space for ϱ\varrho follow by adding the same conditions for dd in the two coordinates; and since both summands are nonnegative, ϱ((x,y),(x′,y′))=0\varrho\bigl((x,y),(x',y')\bigr)=0 holds exactly when d(x,x′)=0d(x,x')=0 and d(y,y′)=0d(y,y')=0, that is, by condition 2 for dd, exactly when (x,y)=(x′,y′)(x,y)=(x',y'). So (Z,ϱ)(Z,\varrho) is a metric space.

It is complete: let ((xm,ym))\bigl((x_{m},y_{m})\bigr) be a Cauchy sequence in (Z,ϱ)(Z,\varrho). Since d(xm,xℓ)≤ϱ((xm,ym),(xℓ,yℓ))d(x_{m},x_{\ell})\le\varrho\bigl((x_{m},y_{m}),(x_{\ell},y_{\ell})\bigr) and d(ym,yℓ)≤ϱ((xm,ym),(xℓ,yℓ))d(y_{m},y_{\ell})\le\varrho\bigl((x_{m},y_{m}),(x_{\ell},y_{\ell})\bigr), the sequences (xm)(x_{m}) and (ym)(y_{m}) are Cauchy sequences in (X,d)(X,d), so by completeness of (X,d)(X,d) they converge to some xˉ∈X\bar{x}\in X and yˉ∈X\bar{y}\in X. Given a real τ>0\tau>0, take N1,N2∈NN_{1},N_{2}\in\mathbb{N} with d(xm,xˉ)<τ/2d(x_{m},\bar{x})<\tau/2 for m≥N1m\ge N_{1} and d(ym,yˉ)<τ/2d(y_{m},\bar{y})<\tau/2 for m≥N2m\ge N_{2}; then ϱ((xm,ym),(xˉ,yˉ))<τ\varrho\bigl((x_{m},y_{m}),(\bar{x},\bar{y})\bigr)<\tau for m≥max⁡{N1,N2}m\ge\max\{N_{1},N_{2}\}, so ((xm,ym))\bigl((x_{m},y_{m})\bigr) converges to (xˉ,yˉ)(\bar{x},\bar{y}) in (Z,ϱ)(Z,\varrho).

Now let ε\varepsilon be a positive real and Φ(x,y)=u(x)−v(y)−1εd(x,y)2\Phi(x,y)=u(x)-v(y)-\frac{1}{\varepsilon}d(x,y)^{2} on ZZ. Then Φ\Phi is upper semicontinuous on ZZ in the sense of Upper Semicontinuous Function on a Subset of a Metric Space (for the metric space (Z,ϱ)(Z,\varrho)). Indeed, fix (xˉ,yˉ)∈Z(\bar{x},\bar{y})\in Z and a real τ>0\tau>0, and put ℓ=d(xˉ,yˉ)\ell=d(\bar{x},\bar{y}). Upper semicontinuity of uu at xˉ\bar{x} gives a real δ1>0\delta_{1}>0 with u(x)<u(xˉ)+τ/3u(x)<u(\bar{x})+\tau/3 for all x∈Xx\in X with d(xˉ,x)<δ1d(\bar{x},x)<\delta_{1}; lower semicontinuity of vv at yˉ\bar{y} gives a real δ2>0\delta_{2}>0 with v(yˉ)−τ/3<v(y)v(\bar{y})-\tau/3<v(y) for all y∈Xy\in X with d(yˉ,y)<δ2d(\bar{y},y)<\delta_{2}. Let δ3=min⁡{1,ετ/(3(2ℓ+1))}\delta_{3}=\min\{1,\varepsilon\tau/(3(2\ell+1))\} and δ0=min⁡{δ1,δ2,δ3}\delta_{0}=\min\{\delta_{1},\delta_{2},\delta_{3}\}, and let (x,y)∈Z(x,y)\in Z with s=ϱ((x,y),(xˉ,yˉ))<δ0s=\varrho\bigl((x,y),(\bar{x},\bar{y})\bigr)<\delta_{0}. Then d(xˉ,x)≤sd(\bar{x},x)\le s and d(yˉ,y)≤sd(\bar{y},y)\le s, and the triangle inequality (condition 4 of Metric Space) gives ℓ≤d(xˉ,x)+d(x,y)+d(y,yˉ)\ell\le d(\bar{x},x)+d(x,y)+d(y,\bar{y}) and d(x,y)≤d(x,xˉ)+ℓ+d(yˉ,y)d(x,y)\le d(x,\bar{x})+\ell+d(\bar{y},y), so ∣d(x,y)−ℓ∣≤s|d(x,y)-\ell|\le s. If d(x,y)≤ℓd(x,y)\le\ell then

ℓ2−d(x,y)2=(ℓ−d(x,y))(ℓ+d(x,y))≤s (2ℓ+s)≤s (2ℓ+1)<ετ/3,\ell^{2}-d(x,y)^{2}=\bigl(\ell-d(x,y)\bigr)\bigl(\ell+d(x,y)\bigr)\le s\,(2\ell+s)\le s\,(2\ell+1)<\varepsilon\tau/3 ,

and if ℓ<d(x,y)\ell<d(x,y) then ℓ2−d(x,y)2<0<ετ/3\ell^{2}-d(x,y)^{2}<0<\varepsilon\tau/3. Adding the three estimates, Φ(x,y)<Φ(xˉ,yˉ)+τ\Phi(x,y)<\Phi(\bar{x},\bar{y})+\tau.

Step 2 (constants). Since uu and vv are bounded above and below in the sense of The Real Numbers: Standing Notation and Background §bounds, there are reals a1,b1,a2,b2a_{1},b_{1},a_{2},b_{2} with a1≤u(x)≤b1a_{1}\le u(x)\le b_{1} and a2≤v(x)≤b2a_{2}\le v(x)\le b_{2} for every x∈Xx\in X; with M=1+∣a1∣+∣b1∣+∣a2∣+∣b2∣M=1+|a_{1}|+|b_{1}|+|a_{2}|+|b_{2}|, a positive real, we get ∣u(x)∣≤M|u(x)|\le M and ∣v(x)∣≤M|v(x)|\le M for every x∈Xx\in X, hence u(x)−v(y)≤2Mu(x)-v(y)\le 2M for all x,y∈Xx,y\in X. Let β=ρθ/4\beta=\rho\theta/4, a positive real. By uniform continuity of ff on XX there is a real σ>0\sigma>0 with ∣f(x)−f(y)∣<β|f(x)-f(y)|<\beta for all x,y∈Xx,y\in X with d(x,y)<σd(x,y)<\sigma. Let γ=min⁡{σ,β/4}\gamma=\min\{\sigma,\beta/4\}, and finally

ε=min⁡{12, γ22(2M+1), β2(2+ρ)}.\varepsilon=\min\Bigl\{\frac{1}{2},\ \frac{\gamma^{2}}{2(2M+1)},\ \frac{\beta}{2(2+\rho)}\Bigr\}.

Then 0<ε<10<\varepsilon<1, so ε2≤ε\varepsilon^{2}\le\varepsilon, and

ε (2M+1)≤γ2/2<γ2,(2+ρ) ε2≤(2+ρ) ε≤β/2<β.(2.1)\varepsilon\,(2M+1)\le\gamma^{2}/2<\gamma^{2},\qquad(2+\rho)\,\varepsilon^{2}\le(2+\rho)\,\varepsilon\le\beta/2<\beta. \tag{2.1}

Step 3 (doubling of variables and Ekeland's principle). Let Φ\Phi be the function of Step 1 for this ε\varepsilon. For all (x,y)∈Z(x,y)\in Z we have Φ(x,y)≤u(x)−v(y)≤2M\Phi(x,y)\le u(x)-v(y)\le 2M, so the nonempty set Φ(Z)\Phi(Z) is bounded above and S=sup⁡(x,y)∈ZΦ(x,y)S=\sup_{(x,y)\in Z}\Phi(x,y) exists by The Real Numbers: Standing Notation and Background §bounds, with θ=Φ(z,z)≤S\theta=\Phi(z,z)\le S. By claim 3 of Approximation Property of the Supremum and the Infimum in R\mathbb{R}, applied with the positive real ε2\varepsilon^{2}, there is (x0,y0)∈Z(x_{0},y_{0})\in Z with S−ε2<Φ(x0,y0)S-\varepsilon^{2}<\Phi(x_{0},y_{0}). By Step 1, Ekeland's Variational Principle for Upper Semicontinuous Functions on a Complete Metric Space applies to F=ΦF=\Phi on the complete metric space (Z,ϱ)(Z,\varrho) with η=ε2\eta=\varepsilon^{2} and κ=ε\kappa=\varepsilon, so that η/κ=ε\eta/\kappa=\varepsilon; it gives (xε,yε)∈Z(x_{\varepsilon},y_{\varepsilon})\in Z such that, by Ekeland's Variational Principle for Upper Semicontinuous Functions on a Complete Metric Space §value,

θ−ε2≤S−ε2≤Φ(x0,y0)≤Φ(xε,yε),\theta-\varepsilon^{2}\le S-\varepsilon^{2}\le\Phi(x_{0},y_{0})\le\Phi(x_{\varepsilon},y_{\varepsilon}),

and, by Ekeland's Variational Principle for Upper Semicontinuous Functions on a Complete Metric Space §perturbed, Φ(x,y)−ε d(x,xε)−ε d(y,yε)<Φ(xε,yε)\Phi(x,y)-\varepsilon\,d(x,x_{\varepsilon})-\varepsilon\,d(y,y_{\varepsilon})<\Phi(x_{\varepsilon},y_{\varepsilon}) for every (x,y)≠(xε,yε)(x,y)\ne(x_{\varepsilon},y_{\varepsilon}). Since the left-hand side equals Φ(xε,yε)\Phi(x_{\varepsilon},y_{\varepsilon}) at (x,y)=(xε,yε)(x,y)=(x_{\varepsilon},y_{\varepsilon}), we get

u(x)−v(y)−1εd(x,y)2−ε d(x,xε)−ε d(y,yε)≤u(xε)−v(yε)−1εd(xε,yε)2for all x,y∈X.(3.1)u(x)-v(y)-\tfrac{1}{\varepsilon}d(x,y)^{2}-\varepsilon\,d(x,x_{\varepsilon})-\varepsilon\,d(y,y_{\varepsilon})\le u(x_{\varepsilon})-v(y_{\varepsilon})-\tfrac{1}{\varepsilon}d(x_{\varepsilon},y_{\varepsilon})^{2}\quad\text{for all }x,y\in X. \tag{3.1}

Put δ=d(xε,yε)\delta=d(x_{\varepsilon},y_{\varepsilon}) and p=2δ/εp=2\delta/\varepsilon, a nonnegative real. From θ−ε2≤Φ(xε,yε)=u(xε)−v(yε)−δ2/ε\theta-\varepsilon^{2}\le\Phi(x_{\varepsilon},y_{\varepsilon})=u(x_{\varepsilon})-v(y_{\varepsilon})-\delta^{2}/\varepsilon we get

θ−ε2≤u(xε)−v(yε)(3.2)\theta-\varepsilon^{2}\le u(x_{\varepsilon})-v(y_{\varepsilon}) \tag{3.2}

and δ2/ε≤u(xε)−v(yε)−θ+ε2≤2M+1\delta^{2}/\varepsilon\le u(x_{\varepsilon})-v(y_{\varepsilon})-\theta+\varepsilon^{2}\le 2M+1, because 0<θ0<\theta and ε2<1\varepsilon^{2}<1. Hence δ2≤ε(2M+1)<γ2\delta^{2}\le\varepsilon(2M+1)<\gamma^{2} by (2.1), and since δ\delta and γ\gamma are nonnegative, claim 1 of Monotonicity of Squaring on the Nonnegative Elements of an Ordered Field gives

δ<γ≤σand4δ<β.(3.3)\delta<\gamma\le\sigma\qquad\text{and}\qquad4\delta<\beta . \tag{3.3}

Step 4 (subsolution test at xεx_{\varepsilon}). Define ψ1,ψ2:X→R\psi_{1},\psi_{2}:X\to\mathbb{R} by ψ1(x)=1εd(x,yε)2+v(yε)\psi_{1}(x)=\frac{1}{\varepsilon}d(x,y_{\varepsilon})^{2}+v(y_{\varepsilon}) and ψ2(x)=ε d(x,xε)\psi_{2}(x)=\varepsilon\,d(x,x_{\varepsilon}). Since (X,d)(X,d) has interpolation points, Elementary Properties of Local Slopes: Order, Negation, Bounds from Difference Quotients, Lipschitz Functions and Squared Distances §squared-distance, applied with Ω=X\Omega=X, x0=yεx_{0}=y_{\varepsilon}, k=1/εk=1/\varepsilon and C=v(yε)C=v(y_{\varepsilon}), shows that ψ1∈C‾(X)\psi_{1}\in\underline{\mathcal{C}}(X) and ∣∇ψ1∣(xε)=2 d(xε,yε)/ε=p|\nabla\psi_{1}|(x_{\varepsilon})=2\,d(x_{\varepsilon},y_{\varepsilon})/\varepsilon=p. For y,w∈Xy,w\in X the triangle inequality gives ∣d(y,xε)−d(w,xε)∣≤d(y,w)|d(y,x_{\varepsilon})-d(w,x_{\varepsilon})|\le d(y,w), so ∣ψ2(y)−ψ2(w)∣≤ε d(y,w)|\psi_{2}(y)-\psi_{2}(w)|\le\varepsilon\,d(y,w); by Elementary Properties of Local Slopes: Order, Negation, Bounds from Difference Quotients, Lipschitz Functions and Squared Distances §lipschitz with L=εL=\varepsilon, ψ2\psi_{2} is locally Lipschitz on XX and e1=∣∇ψ2∣∗(xε)e_{1}=|\nabla\psi_{2}|^{*}(x_{\varepsilon}) satisfies e1≤εe_{1}\le\varepsilon. Taking y=yεy=y_{\varepsilon} in (3.1) and noting ψ2(xε)=0\psi_{2}(x_{\varepsilon})=0, we get u(x)−ψ1(x)−ψ2(x)≤u(xε)−ψ1(xε)−ψ2(xε)u(x)-\psi_{1}(x)-\psi_{2}(x)\le u(x_{\varepsilon})-\psi_{1}(x_{\varepsilon})-\psi_{2}(x_{\varepsilon}) for every x∈Xx\in X, so u−ψ1−ψ2u-\psi_{1}-\psi_{2} has a local maximum at xεx_{\varepsilon} relative to XX (with any radius). By Slope-Based Viscosity Subsolutions, Supersolutions and Solutions on a Metric Space §subsolution,

H(xε,u(xε),max⁡{p−e1,0})≤0.H\bigl(x_{\varepsilon},u(x_{\varepsilon}),\max\{p-e_{1},0\}\bigr)\le0 .

Let p−=max⁡{p−ε,0}∈Tp_{-}=\max\{p-\varepsilon,0\}\in T. Since p−ε≤p−e1p-\varepsilon\le p-e_{1}, claim 1 of Elementary Properties of the Maximum of Two Elements gives p−ε≤max⁡{p−e1,0}p-\varepsilon\le\max\{p-e_{1},0\} and 0≤max⁡{p−e1,0}0\le\max\{p-e_{1},0\}, so claim 3 of the same lemma gives p−≤max⁡{p−e1,0}p_{-}\le\max\{p-e_{1},0\}. By the monotonicity of HH recalled above, H(xε,u(xε),p−)≤0H(x_{\varepsilon},u(x_{\varepsilon}),p_{-})\le0, that is,

ρ u(xε)+12p−2≤f(xε).(4.1)\rho\,u(x_{\varepsilon})+\tfrac{1}{2}p_{-}^{2}\le f(x_{\varepsilon}). \tag{4.1}

Step 5 (supersolution test at yεy_{\varepsilon}). Define ψ3,ψ4:X→R\psi_{3},\psi_{4}:X\to\mathbb{R} by ψ3(y)=−1εd(y,xε)2+u(xε)\psi_{3}(y)=-\frac{1}{\varepsilon}d(y,x_{\varepsilon})^{2}+u(x_{\varepsilon}) and ψ4(y)=−ε d(y,yε)\psi_{4}(y)=-\varepsilon\,d(y,y_{\varepsilon}). Then ψ3=−φ\psi_{3}=-\varphi with φ(y)=1εd(y,xε)2−u(xε)\varphi(y)=\frac{1}{\varepsilon}d(y,x_{\varepsilon})^{2}-u(x_{\varepsilon}), so the last sentence of Elementary Properties of Local Slopes: Order, Negation, Bounds from Difference Quotients, Lipschitz Functions and Squared Distances §squared-distance (with Ω=X\Omega=X, x0=xεx_{0}=x_{\varepsilon}, k=1/εk=1/\varepsilon, C=−u(xε)C=-u(x_{\varepsilon})) shows that ψ3∈C‾(X)\psi_{3}\in\overline{\mathcal{C}}(X) and ∣∇ψ3∣(yε)=2 d(yε,xε)/ε=p|\nabla\psi_{3}|(y_{\varepsilon})=2\,d(y_{\varepsilon},x_{\varepsilon})/\varepsilon=p. As in Step 4, ∣ψ4(y)−ψ4(w)∣≤ε d(y,w)|\psi_{4}(y)-\psi_{4}(w)|\le\varepsilon\,d(y,w) for y,w∈Xy,w\in X, so by Elementary Properties of Local Slopes: Order, Negation, Bounds from Difference Quotients, Lipschitz Functions and Squared Distances §lipschitz ψ4\psi_{4} is locally Lipschitz on XX and e2=∣∇ψ4∣∗(yε)e_{2}=|\nabla\psi_{4}|^{*}(y_{\varepsilon}) satisfies e2≤εe_{2}\le\varepsilon. Taking x=xεx=x_{\varepsilon} in (3.1) and using d(xε,y)=d(y,xε)d(x_{\varepsilon},y)=d(y,x_{\varepsilon}), we get u(xε)−v(y)−1εd(y,xε)2−ε d(y,yε)≤u(xε)−v(yε)−1εδ2u(x_{\varepsilon})-v(y)-\frac{1}{\varepsilon}d(y,x_{\varepsilon})^{2}-\varepsilon\,d(y,y_{\varepsilon})\le u(x_{\varepsilon})-v(y_{\varepsilon})-\frac{1}{\varepsilon}\delta^{2}, which rearranges to v(yε)−ψ3(yε)−ψ4(yε)≤v(y)−ψ3(y)−ψ4(y)v(y_{\varepsilon})-\psi_{3}(y_{\varepsilon})-\psi_{4}(y_{\varepsilon})\le v(y)-\psi_{3}(y)-\psi_{4}(y) for every y∈Xy\in X. So v−ψ3−ψ4v-\psi_{3}-\psi_{4} has a local minimum at yεy_{\varepsilon} relative to XX, and Slope-Based Viscosity Subsolutions, Supersolutions and Solutions on a Metric Space §supersolution gives H(yε,v(yε),p+e2)≥0H(y_{\varepsilon},v(y_{\varepsilon}),p+e_{2})\ge0. Since p+e2≤p+εp+e_{2}\le p+\varepsilon and both lie in TT, monotonicity of HH gives H(yε,v(yε),p+ε)≥0H(y_{\varepsilon},v(y_{\varepsilon}),p+\varepsilon)\ge0, that is,

f(yε)≤ρ v(yε)+12(p+ε)2.(5.1)f(y_{\varepsilon})\le\rho\,v(y_{\varepsilon})+\tfrac{1}{2}(p+\varepsilon)^{2}. \tag{5.1}

Step 6 (the quadratic terms). We show 12(p+ε)2−12p−2≤2εp+2ε2\frac{1}{2}(p+\varepsilon)^{2}-\frac{1}{2}p_{-}^{2}\le 2\varepsilon p+2\varepsilon^{2}. If ε≤p\varepsilon\le p, then 0≤p−ε≤p−0\le p-\varepsilon\le p_{-} by claim 1 of Elementary Properties of the Maximum of Two Elements, so (p−ε)2≤p−2(p-\varepsilon)^{2}\le p_{-}^{2} by claim 2 of Monotonicity of Squaring on the Nonnegative Elements of an Ordered Field, and 12(p+ε)2−12(p−ε)2=2εp\frac{1}{2}(p+\varepsilon)^{2}-\frac{1}{2}(p-\varepsilon)^{2}=2\varepsilon p. If p<εp<\varepsilon, then 0≤p+ε≤2ε0\le p+\varepsilon\le2\varepsilon, so (p+ε)2≤4ε2(p+\varepsilon)^{2}\le4\varepsilon^{2} by claim 2 of Monotonicity of Squaring on the Nonnegative Elements of an Ordered Field, and with 0≤p−20\le p_{-}^{2} we get 12(p+ε)2−12p−2≤2ε2≤2εp+2ε2\frac{1}{2}(p+\varepsilon)^{2}-\frac{1}{2}p_{-}^{2}\le2\varepsilon^{2}\le2\varepsilon p+2\varepsilon^{2}. Since εp=2δ\varepsilon p=2\delta,

12(p+ε)2−12p−2≤4δ+2ε2.(6.1)\tfrac{1}{2}(p+\varepsilon)^{2}-\tfrac{1}{2}p_{-}^{2}\le4\delta+2\varepsilon^{2}. \tag{6.1}

Step 7 (contradiction). Adding (4.1) and (5.1) and using (6.1),

ρ(u(xε)−v(yε))≤f(xε)−f(yε)+4δ+2ε2.\rho\bigl(u(x_{\varepsilon})-v(y_{\varepsilon})\bigr)\le f(x_{\varepsilon})-f(y_{\varepsilon})+4\delta+2\varepsilon^{2}.

Since 0<ρ0<\rho, (3.2) gives ρθ−ρε2≤ρ(u(xε)−v(yε))\rho\theta-\rho\varepsilon^{2}\le\rho\bigl(u(x_{\varepsilon})-v(y_{\varepsilon})\bigr). By (3.3), d(xε,yε)=δ<σd(x_{\varepsilon},y_{\varepsilon})=\delta<\sigma, so ∣f(xε)−f(yε)∣<β|f(x_{\varepsilon})-f(y_{\varepsilon})|<\beta by the choice of σ\sigma, and 4δ<β4\delta<\beta. Together with (2.1),

4β=ρθ≤∣f(xε)−f(yε)∣+4δ+(2+ρ) ε2<3β,4\beta=\rho\theta\le|f(x_{\varepsilon})-f(y_{\varepsilon})|+4\delta+(2+\rho)\,\varepsilon^{2}<3\beta ,

which is impossible because 0<β0<\beta. Hence there is no z∈Xz\in X with v(z)<u(z)v(z)<u(z), that is, u(x)≤v(x)u(x)\le v(x) for every x∈Xx\in X.

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