Abstract
We investigate the convergence rate in the vanishing viscosity process of the solutions to the subquadratic state-constraint Hamilton–Jacobi equations. We give two different proofs of the fact that, for non-negative Lipschitz data that vanish on the boundary, the rate of convergence is \({\mathcal {O}}(\sqrt{\varepsilon })\) in the interior. Moreover, the one-sided rate can be improved to \({\mathcal {O}}(\varepsilon )\) for non-negative compactly supported data and \({\mathcal {O}}(\varepsilon ^{1/p})\) (where \(1<p<2\) is the exponent of the gradient term) for non-negative data \(f\in \mathrm {C}^2({\overline{\varOmega }})\) such that \(f = 0\) and \(Df = 0\) on the boundary. Our approach relies on deep understanding of the blow-up behavior near the boundary and semiconcavity of the solutions.
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Acknowledgements
The authors would like to express their appreciation to Hung V. Tran for his invaluable guidance. The authors would also like to thank Dohyun Kwon for useful discussions.
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The authors contributed equally to this work. The authors are supported in part by NSF Grant DMS-1664424 and NSF CAREER Grant DMS-1843320. The work of Son N. T. Tu is supported in part by the GSSC Fellowship, University of Wisconsin–Madison.
Appendix
Appendix
1.1 A.1 Estimates on Solutions
We present here a proof for the gradient bound of the solution to (PDE\(_\varepsilon \)) using Bernstein’s method (see also [21, 23]). Another proof using Berstein’s method inside a doubling variable argument is given in [1].
Proof of Theorem 4
Let \(\theta \in (0,1)\) be chosen later, \(\varphi \in \mathrm {C}_c^\infty (\varOmega )\), \(0\le \varphi \le 1\), \(\mathrm {supp}\;\varphi \subset \varOmega \) and \(\varphi = 1\) on \(\varOmega _\delta \) such that
where \(C = C(\delta ,\theta )\) is a constant depending on \(\delta ,\theta \).
Define \(w(x) := \left|Du^\varepsilon (x)\right|^2\) for \(x \in \varOmega \). The equation for w is given by
Then an equation for \((\varphi w)\) can be derived as follows.
Assume that \(\varphi w\) achieves its maximum over \({\overline{\varOmega }}\) at \(x_0\in \varOmega \). And we can further assume that \(x_0\in \mathrm {supp}\;\varphi \), since otherwise the maximum of \(\varphi w\) over \({\overline{\varOmega }}\) is zero. By the classical maximum principle,
Use this in the equation of \(\varphi w\) above to obtain
where all terms are evaluated at \(x_0\). From (66), we have
By Cauchy–Schwartz inequality, \(n\left|D^2u^\varepsilon \right|^2\ge (\varDelta u^\varepsilon )^2\). Thus, if \(n\varepsilon < 1\), then
where C depends on \(\max _{{\overline{\varOmega }}}f\) only. Using (68) in (67), we obtain that
Multiply both sides by \(\varphi ^{p-1}\) to deduce that
Choose \(2p+\theta -1 \ge p+1\), i.e., \(p+\theta \ge 2\). This is always possible with the requirement \(\theta \in (0,1)\), as \(1<p <\infty \). Then we get
As a polynomial in \(z = (\varphi w)(x_0)\), this implies that \((\varphi w)(x_0)\le C\) where C depends on coefficients of the right hand side of (69), which gives our desired gradient bound since \(w(x)=(\varphi w)(x) \le (\varphi w)(x_0)\) for \(x \in {\overline{\varOmega }}_\delta \subset \mathrm {supp}\;\varphi \). \(\square \)
1.2 A.2 Well-Posedness of (PDE\(_\varepsilon \))
Proof of Theorem 5
If \(p\in (1,2)\), we use the ansatz \( u(x) = C_\varepsilon d(x)^{-\alpha }\) to find a solution to (PDE\(_\varepsilon \)). Plug the ansatz into (PDE\(_\varepsilon \)) and compute
Since \(\left|D d(x)\right|= 1\) for x near \(\partial \varOmega \), as \(x\rightarrow \partial \varOmega \), the explosive terms of the highest order are
Set the above to be zero to obtain that
For \(0<\delta < \frac{1}{2}\delta _0\) and \(\eta \) small, define
where \(C_\alpha := \frac{1}{\alpha } (\alpha +1)^{\alpha +1} \), \(M_\eta \) to be chosen. Next, we show that \({\overline{w}}_{\eta ,\delta }\) is a supersolution of (PDE\(_\varepsilon \)) in \(\varOmega _\delta \), while \({\underline{w}}_{\eta ,\delta }\) is a subsolution of (PDE\(_\varepsilon \)) in \(\varOmega ^\delta \). Compute
where we use \((C_\alpha \alpha )^p = C_\alpha \alpha (\alpha +1)\) and \(\nu = \frac{C_\alpha +\eta }{C_\alpha } \in (1,2)\) for small \(\eta \). Let
and \(\delta _\eta \rightarrow 0\) as \(\eta \rightarrow 0\). To get \({\mathcal {L}}^\varepsilon \left[ {\overline{w}}_{\eta ,\delta }\right] \ge 0\), there are two cases to consider, depending on how large \(d(x)-\delta \) is.
-
If \(0< d(x)-\delta<\delta _\eta < \delta _0\) for \(\eta \) small and fixed, then \(\left|Dd(x)\right|= 1\), and thus \(I\ge 0\). Hence, \({\mathcal {L}}^\varepsilon \left[ {\overline{w}}_{\eta ,\delta }\right] \ge 0\) if we choose \(M_\eta \ge \max _{{\overline{\varOmega }}} f\).
-
If \(d(x)-\delta \ge \delta _\eta \), then
$$\begin{aligned} I \le \left( \frac{1}{\delta _\eta }\right) ^{\alpha +2}\nu C_\alpha \alpha (\alpha +1)\left[ \nu ^{p-1}K_1^{p}+K_1^2+K_2K_0\right] \varepsilon ^{\alpha +2}. \end{aligned}$$Thus, we can choose \(M_\eta = \max _{{\overline{\varOmega }}} f + C\varepsilon ^{\alpha +2}\) for C large enough (depending on \(\eta \)) so that \({\mathcal {L}}^\varepsilon \left[ {\overline{w}}_{\eta ,\delta }\right] \ge 0\).
Therefore, \({\overline{w}}_{\eta ,\delta }\) is a supersolution in \(\varOmega _\delta \).
Similarly, we have
where \(\nu = \frac{C_\alpha -\eta }{C_\alpha }\in (0,1)\) for small \(\eta \). Let
and \(\delta _\eta \rightarrow 0\) as \( \eta \rightarrow 0\). To obtain \({\mathcal {L}}^\varepsilon \left[ {\underline{w}}_{\eta ,\delta }\right] \le 0\), there are two cases to consider depending on how large \(d(x)+\delta \) is.
-
If \(0<d(x)+\delta<\delta _\eta < \delta _0\) for \(\eta \) small and fixed, then \(\left|Dd(x)\right|= 1\), and thus \(J\le 0\). Hence, \({\mathcal {L}}^\varepsilon \left[ {\underline{w}}_{\eta ,\delta }\right] \le 0\) if we choose \(M_\eta \ge -\max _{\varOmega }f\).
-
If \(d(x)+\delta \ge \delta _\eta \), then
$$\begin{aligned} \left|J\right|\le \left( \frac{1}{\delta _\eta }\right) ^{\alpha +2} \nu C_\alpha \alpha (\alpha +1)\left[ \nu ^{p-1}K_1^{p}+K_1^2 + \frac{(K_0+1)K_2}{\alpha +1} + \frac{(K_0+1)^2}{\alpha (\alpha +1)\varepsilon }\right] \varepsilon ^{\alpha +2} \end{aligned}$$Thus, we can choose \(M_\eta = -\max _{{\overline{\varOmega }}} f - C\varepsilon ^{\alpha +2}\) for C large enough (depending on \(\eta \)) so that \({\mathcal {L}}^\varepsilon \left[ {\underline{w}}_{\eta ,\delta }\right] \le 0\).
Therefore, \({\underline{w}}_{\eta ,\delta }\) is a subsolution in \(\varOmega ^\delta \).
For \(p=2\), we use the ansatz \(u(x) = -C_\varepsilon \log (d(x))\) instead. Similar to the previous case, one can find \(u(x) = -\varepsilon \log (d(x))\). For \(0<\delta <\frac{1}{2}\delta _0\), define
where \(M_\eta \) is to be chosen so that \({\overline{w}}_{\eta ,\delta }(x)\) is a supersolution in \(\varOmega _\delta \) and \({\underline{w}}_{\eta ,\delta }\) is a subsolution in \(\varOmega ^\delta \). The computations are omitted here, as they are similar to the previous case.
We divide the rest of the proof into 3 steps. We first construct a minimal solution, then a maximal solution to (PDE\(_\varepsilon \)), and finally show that they are equal to conclude the existence and the uniqueness of the solution to (PDE\(_\varepsilon \)).
Step 1 There exists a minimal solution \({\underline{u}}\in \mathrm {C}^2(\varOmega )\) of (PDE\(_\varepsilon \)) such that \(v\ge {\underline{u}}\) for any other solution \(v\in \mathrm {C}^2(\varOmega )\) solving (PDE\(_\varepsilon \)).
Proof
Let \(w_{\eta ,\delta }\in \mathrm {C}^2(\varOmega )\) solve
-
Fix \(\eta >0\). As \(\delta \rightarrow 0^+\), the value of \({\underline{w}}_{\eta ,\delta }\) blows up on the boundary. Therefore, by the standard comparison principle for the second-order elliptic equation with the Dirichlet boundary, \(\delta _1 \le \delta _2\) implies \(w_{\eta ,\delta _1}\ge w_{\eta ,\delta _2}\) on \({\overline{\varOmega }}\).
-
For \(\delta '>0\), since \({\underline{w}}_{\eta ,\delta '}\) is a subsolution in \({\overline{\varOmega }}\) with finite boundary,
$$\begin{aligned} 0<\delta \le \delta '\qquad \Longrightarrow \qquad {\underline{w}}_{\eta ,\delta '} \le w_{\eta _,\delta '}\le w_{\eta ,\delta } \qquad \text {on}\;{\overline{\varOmega }}. \end{aligned}$$(72) -
Similarly, since \({\overline{w}}_{\eta ,\delta '}\) is a supersolution on \(\varOmega _{\delta '}\) with infinity value on the boundary \(\partial \varOmega _{\delta '}\), by the comparison principle,
$$\begin{aligned} w_{\eta ,\delta } \le {\overline{w}}_{\eta , \delta '} \qquad \text {in}\;\varOmega _{\delta '} \qquad \Longrightarrow \qquad w_{\eta ,\delta } \le {\overline{w}}_{\eta ,0} \qquad \text {in}\;\varOmega . \end{aligned}$$(73)
Thus, \(\{w_{\eta ,\delta }\}_{\delta >0}\) is locally bounded in \(L^{\infty }_{\mathrm {loc}}(\varOmega )\) (\(\{w_{\eta ,\delta }\}_{\delta >0}\) is uniformly bounded from below). Using the local gradient estimate for \(w_{\eta ,\delta }\) solving (71), we deduce that \(\{w_{\eta ,\delta }\}_{\delta >0}\) is locally bounded in \(W^{1,\infty }_{\mathrm {loc}}(\varOmega )\). Since \(w_{\eta ,\delta }\) solves (71), we further have that \(\{w_{\eta ,\delta }\}_{\delta >0}\) is locally bounded in \(W^{2,r}_{\mathrm {loc}}(\varOmega )\) for all \(r<\infty \) by Calderon–Zygmund estimates.
Local boundedness of \(\{w_{\eta ,\delta }\}_{\delta >0}\) in \(W^{2,r}_{\mathrm {loc}}(\varOmega )\) implies weak\(^*\) compactness, that is, there exists a function \(u\in W^{2,r}_{\mathrm {loc}}(\varOmega )\) such that (via subsequence and monotonicity)
In particular, \(w_{\eta ,\delta }\rightarrow u\) in \(\mathrm {C}^1_{\mathrm {loc}}(\varOmega )\) thanks to Sobolev compact embedding. Let us rewrite the equation \({\mathcal {L}}^\varepsilon \left[ w_{\eta ,\delta }\right] = 0\) as \(\varepsilon \varDelta w_{\eta ,\delta }(x) = F[w_{\eta ,\delta }](x)\) for \(x \in U\subset \subset \varOmega \), where
Since \(w_{\eta ,\delta }\rightarrow u\) in \(\mathrm {C}^1(U)\) as \(\delta \rightarrow 0\), we have \(F[w_{\eta ,\delta }](x) \rightarrow F(x)\) uniformly in U as \(\delta \rightarrow 0\), where
In the limit, we obtain that \(u\in L^2(U)\) is a weak solution of \(\varepsilon \varDelta u = F\) in U where F is continuous. Thus, \(u\in \mathrm {C}^2(\varOmega )\) and by stability, u solves \({\mathcal {L}}^\varepsilon [u] = 0\) in \(\varOmega \). From (74), we also have
Moreover, \(u(x)\rightarrow \infty \) as \(\mathrm {dist}(x,\partial \varOmega )\rightarrow 0\) with the precise rate like (9) or (10). Note that by construction, u may depend on \(\eta \). But next, we will show that u is independent of \(\eta \), by proving u is the unique minimal solution of \({\mathcal {L}}^\varepsilon [u] = 0\) in \(\varOmega \) with \(u = +\infty \) on \(\partial \varOmega \).
Let \(v\in \mathrm {C}^{2}(\varOmega )\) be a solution to (PDE\(_\varepsilon \)). Fix \(\delta >0\). Since \(v(x)\rightarrow \infty \) as \(x\rightarrow \partial \varOmega \) while \(w_{\eta ,\delta }\) remains bounded on \(\partial \varOmega \), the comparison principle yields
Let \(\delta \rightarrow 0\) and we deduce that \(v\ge u\) in \(\varOmega \). This concludes that u is the minimal solution in \(\mathrm {C}^2(\varOmega )(\forall \,r<\infty )\) and thus u is independent of \(\eta \). \(\square \)
Step 2 There exists a maximal solution \({\overline{u}}\in \mathrm {C}^2(\varOmega )\) of (PDE\(_\varepsilon \)) such that \(v\le {\overline{u}}\) for any other solution \(v\in \mathrm {C}^2(\varOmega )\) solving (PDE\(_\varepsilon \)).
Proof
For each \(\delta >0\), let \(u_\delta \in \mathrm {C}^2(\varOmega _\delta )\) be the minimal solution to \({\mathcal {L}}^\varepsilon [u_\delta ] = 0\) in \(\varOmega _\delta \) with \(u_\delta = +\infty \) on \(\partial \varOmega _\delta \). By the comparison principle, for every \(\eta >0\), there holds
and
The monotoniciy, together with the local boundedness of \(\{u_\delta \}_{\delta >0}\) in \(W^{2,r}_{\mathrm {loc}}(\varOmega )\), implies that there exists \(u\in W^{2,r}_{\mathrm {loc}}(\varOmega )\) for all \(r<\infty \) such that \(u_\delta \rightarrow u\) strongly in \(\mathrm {C}^1_{\mathrm {loc}}(\varOmega )\). Using the equation \({\mathcal {L}}^\varepsilon [u_\delta ] = 0\) in \(\varOmega _\delta \) and the regularity of Laplace’s equation, we can further deduce that \(u\in \mathrm {C}^2(\varOmega )\) solves (PDE\(_\varepsilon \)) and
for all \(\eta >0\). As \(u_\delta \) is independent of \(\eta \) by the previous argument in Step 1, it is clear that u is also independent of \(\eta \). Now we show that u is the maximal solution of (PDE\(_\varepsilon \)). Let \(v\in \mathrm {C}^2(\varOmega )\) solve (PDE\(_\varepsilon \)). Clearly \(v\le u_\delta \) on \(\varOmega _\delta \). Therefore, as \(\delta \rightarrow 0\), we have \(v\le u\). \(\square \)
In conclusion, we have found a minimal solution \({\underline{u}}\) and a maximal solution \({\overline{u}}\) in \(\mathrm {C}^2(\varOmega )\) such that
for any \(\eta >0\). This extra parameter \(\eta \) now enables us to show that \({\overline{u}} = {\underline{u}}\) in \(\varOmega \). The key ingredient here is the convexity in the gradient slot of the operator.
Step 3 We have \({\overline{u}}\equiv {\underline{u}}\) in \(\varOmega \). Therefore, the solution to (PDE\(_\varepsilon \)) in \(\mathrm {C}^2(\varOmega )\) is unique.
Proof
Let \(\theta \in (0,1)\). Define \(w_\theta = \theta {\overline{u}} + (1-\theta ) \inf _{\varOmega } f\). It can be verified that \(w_\theta \) is a subsolution to (PDE\(_\varepsilon \)). Then one may argue that by the comparison principle,
and conclude that \({\overline{u}} \le {\underline{u}}\) by letting \(\theta \rightarrow 1\). But we have to be careful here. As they are both explosive solutions, to use the comparison principle, we need to show that \(w_\theta \le {\underline{u}}\) in a neighborhood of \(\partial \varOmega \). From (75), we see that
for \(x\in \varOmega \). Hence,
Since \(\eta >0\) is chosen arbitrary, we obtain
This means for any \(\varsigma \in (0,1)\), there exists \({\delta _1}(\varsigma )>0\) small such that
For a fixed \(\theta \in (0,1)\), one can always choose \(\varsigma \) small enough so that \(\displaystyle (1+\varsigma )^{-1} \ge \frac{1+\theta }{2}\). Since \({\overline{u}}(x) \rightarrow +\infty \) as \(d(x) \rightarrow 0\), there exists \(\delta _2 > 0\) such that \({\overline{u}}(x) \ge 2 \inf _\varOmega f\) for all \(x \in \varOmega \setminus \varOmega _{\delta _2}\). Now we have
for all \(x \in \varOmega \setminus \varOmega _\delta \) where \(\delta : = \min \{\delta _1, \delta _2\}\). This implies for any fixed \(\theta \in (0,1)\), \(w_\theta \le {\underline{u}}\) in a neighborhood of \(\partial \varOmega \). Hence, by the comparison principle,
for any \(\theta \in (0,1)\). Then let \(\theta \rightarrow 1\) to get the conclusion.
This finishes the proof of the well-posedness of (PDE\(_\varepsilon \)) for \(1<p\le 2\). \(\square \)
Proof of Lemma 6
The proof is a variation of Perron’s method (see [10]) and we proceed by contradiction. Let \(\varphi \in \mathrm {C}({\overline{\varOmega }})\) and \(x_0\in {\overline{\varOmega }}\) such that \(u(x_0) = \varphi (x_0)\) and \(u-\varphi \) has a global strict minimum over \({\overline{\varOmega }}\) at \(x_0\) with
Let \(\varphi ^\varepsilon (x) = \varphi (x) - \left|x-x_0\right|^2 + \varepsilon \) for \(x\in {\overline{\varOmega }}\). Let \(\delta > 0\). We see that for \(x\in \partial B(x_0,\delta )\cap {\overline{\varOmega }}\),
if \(2\varepsilon \le \delta ^2\). We observe that
for \(x\in B(x_0,\delta )\cap {\overline{\varOmega }}\). By the continuity of H(x, p) near \((x_0,D\varphi (x_0))\) and the fact that \(\varphi \in \mathrm {C}^1({\overline{\varOmega }})\), we can deduce from (76) that if \(\delta \) is small enough and \(0<2\varepsilon < \delta ^2\), then
We have found \(\varphi ^\varepsilon \in \mathrm {C}^1({\overline{\varOmega }})\) such that \(\varphi ^\varepsilon (x_0)>u(x_0)\), \(\varphi ^\varepsilon <u\) on \(\partial B(x_0,\delta )\cap {\overline{\varOmega }}\) and (77). Let
We see that \({\tilde{u}}\in \mathrm {C}({\overline{\varOmega }})\) is a subsolution of (PDE\(_0\)) in \(\varOmega \) with \({\tilde{u}}(x_0) > u(x_0)\), which is a contradiction. Thus, u is a supersolution of (PDE\(_0\)) on \({\overline{\varOmega }}\). \(\square \)
1.3 A.3 Semiconcavity
We present a proof for the semiconcavity of solution to first-order Hamilton–Jacobi equation using the doubling variable method (see also [8]).
Theorem 19
Let \(H(x,p) = G(p)-f(x)\) where \(G\ge 0\) with \(G(0) = 0\) is a convex function from \({\mathbb {R}}^n\rightarrow {\mathbb {R}}^n\) and \(f\in \mathrm {C}^2_c({\mathbb {R}}^n)\). Let \(u\in \mathrm {C}_c({\mathbb {R}}^n)\) be a viscosity solution to \(u+H(x,Du) = 0\) in \({\mathbb {R}}^n\). Then u is semiconcave, i.e., u is a viscosity solution of \(-D^2u \ge -c\;{\mathbb {I}}_n\) in \({\mathbb {R}}^n\) where
Proof
Consider the auxiliary functional
for \((x,y,z)\in {\mathbb {R}}^n\times {\mathbb {R}}^n\times {\mathbb {R}}^n\). By the a priori estimate, u is bounded and Lipschitz. Thus, we can assume \(\varPhi \) achieves its maximum over \({\mathbb {R}}^n\times {\mathbb {R}}^n\times {\mathbb {R}}^n\) at \((x_\alpha ,y_\alpha ,z_\alpha )\). The viscosity solution tests give us
where \(p_\alpha = \alpha (x_\alpha -2y_\alpha +z_\alpha )\). By the convexity of G, we have
Therefore,
-
\(\varPhi (x_\alpha ,y_\alpha ,z_\alpha )\ge \varPhi (0,0,0)\) gives us
$$\begin{aligned} \frac{\alpha }{2}\left|x_\alpha -2y_\alpha +z_\alpha \right|^2 + \frac{c}{2}\left|y_\alpha -x_\alpha \right|^2+\frac{c}{2}\left|y_\alpha -z_\alpha \right|^2 \le C. \end{aligned}$$Thus, \((x_\alpha -y_\alpha )\rightarrow h_0\) and \((y_\alpha -z_\alpha )\rightarrow h_0\) as \(\alpha \rightarrow \infty \) for some \(h_0 \in {\mathbb {R}}^n\).
-
\(\varPhi (x_\alpha ,y_\alpha ,z_\alpha )\ge \varPhi (y_\alpha +h_0,y_\alpha ,y_\alpha -h_0)\) gives us
$$\begin{aligned} u(x_\alpha )-2u(y_\alpha ) + u(z_\alpha ) - \frac{\alpha }{2}\left|x_\alpha - 2y_\alpha +z_\alpha \right|^2 - \frac{c}{2}\left|x_\alpha -y_\alpha \right|^2 - \frac{c}{2}\left|y_\alpha -z_\alpha \right|^2 \\ \ge u(y_\alpha +h_0) - 2u(y_\alpha ) + u(y_\alpha -h_0) - c\left|h_0\right|^2. \end{aligned}$$Therefore, by the fact that u is Lipschitz, we have
$$\begin{aligned} \begin{aligned} \frac{\alpha }{2}\left|x_\alpha - 2y_\alpha +z_\alpha \right|^2 \le&c\left( \frac{2\left|h_0\right|^2 - \left|x_\alpha -y_\alpha \right|^2 - \left|y_\alpha -z_\alpha \right|^2}{2}\right) \\&+ C\Big (\left|(x_\alpha -y_\alpha ) - h_0\right|+ \left|(z_\alpha - y_\alpha ) + h_0\right|\Big ) \rightarrow 0 \end{aligned} \end{aligned}$$as \(\alpha \rightarrow \infty \).
For any \(x\in {\mathbb {R}}^n\), we have \(\varPhi (x_\alpha ,y_\alpha ,z_\alpha ) \ge \varPhi (x+h,x,x-h)\), i.e.,
If \(\{y_\alpha \}\) is unbounded, then since \(f\in \mathrm {C}_c^2({\mathbb {R}}^n)\), we have \(f(y_\alpha )\rightarrow 0\) as \(\alpha \rightarrow \infty \). As a consequence, \(x_\alpha ,z_\alpha \rightarrow \infty \) as well and thus \(f(x_\alpha )-2f(y_\alpha ) + f(z_\alpha )\rightarrow 0\) as \(\alpha \rightarrow \infty \). Therefore,
If \(\{y_\alpha \}\) is bounded, then \(y_\alpha \rightarrow y_0\) for some \(y_0 \in {\mathbb {R}}^n\) as \(\alpha \rightarrow \infty \). Thus,
Let \(\xi = h_0\) and we have
Therefore,
which implies
Hence,
and thus u is semiconcave. It is easy to see that if \(\varphi \) is smooth and \(u-\varphi \) has a local min at x, then \(D^2\varphi (x) \le c\;{\mathbb {I}}\), i.e., \(-D^2\varphi (x)\ge -c\;{\mathbb {I}}\). \(\square \)
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Han, Y., Tu, S.N.T. Remarks on the Vanishing Viscosity Process of State-Constraint Hamilton–Jacobi Equations. Appl Math Optim 86, 3 (2022). https://doi.org/10.1007/s00245-022-09874-z
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DOI: https://doi.org/10.1007/s00245-022-09874-z
Keywords
- First-order Hamilton–Jacobi equations
- Second-order Hamilton–Jacobi equations
- State-constraint problems
- Optimal control theory
- Rate of convergence
- Viscosity solutions
- Semiconcavity
- Boundary layer