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{\tenrm\ifodd\pageno\rightheadline \else \leftheadline\fi}\fi}
%
\def\Swiech{\'Swie\kern -0.21em\lower0.79ex\hbox{$\scriptstyle\lhook$}ch}
\def\rightheadline{EJDE--1999/24\hfil Existence results for boundary problems 
    \hfil\folio}
\def\leftheadline{\folio\hfil M. G. Crandall, M. Kocan, P. L. Lions, 
    \& A. \Swiech \hfil EJDE--1999/24}

\voffset=2\baselineskip
\vbox {\eightrm\noindent\baselineskip 9pt %
 Electronic Journal of Differential Equations,
Vol. {\eightbf 1999}(1999) No.~24, pp. 1--20.\hfill\break
ISSN: 1072-6691. URL: http://ejde.math.swt.edu or http://ejde.math.unt.edu
\hfil\break ftp  ejde.math.swt.edu \quad ftp ejde.math.unt.edu (login: ftp)}
\footnote{}{\vbox{\hsize=10cm\eightrm\noindent\baselineskip 9pt %
1991 {\eighti Subject Classification:} 35J25, 35J60, 35J65,
35K20, 35K55, 35K60, 49L25.
\hfil\break
{\eighti Key words and phrases:} Uniformly elliptic and parabolic equations, 
viscosity solutions, good solutions, exterior cone condition, barrier functions.
\hfil\break
\copyright 1999 Southwest Texas State University  and
University of North Texas.\hfil\break
Submitted May 20, 1999. Published July 1, 1999.\hfil\break
} }
\bigskip\bigskip

\centerline{EXISTENCE RESULTS FOR BOUNDARY PROBLEMS FOR  UNIFORMLY}
\centerline{ELLIPTIC AND PARABOLIC FULLY NONLINEAR  EQUATIONS }

\medskip
\centerline{M. G. Crandall, M. Kocan, P. L. Lions, \& A. \Swiech}
\bigskip\bigskip

{\eightrm\baselineskip=10pt \narrower
\centerline{\eightbf Abstract}
We study existence of continuous weak (viscosity) solutions of
Dirichlet and Cauchy-Dirichlet problems for fully nonlinear uniformly 
elliptic and parabolic equations. Two types of results are obtained in
contexts where uniqueness of solutions fails or is unknown.
For equations with merely measurable coefficients we prove 
solvability of the problem, while in the continuous 
case we construct maximal and minimal solutions. Necessary
barriers on external cones are also constructed.
\bigskip}

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\def\eq{\global\advance\equationno by 1 \eqno(\secno.\the\equationno)}

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   Theorem #1. }{\it\ignorespaces#2} }
\long\def\proposition#1#2{\removelastskip\vskip\baselineskip\noindent{\bf
  Proposition #1. }{\it\ignorespaces#2}\vskip\baselineskip}
\long\def\proof#1{\removelastskip\vskip0.5\baselineskip\noindent{\it 
  Proof. }\ignorespaces#1\hfill\square\vskip\baselineskip}
\long\def\proofof#1#2{\removelastskip\vskip0.5\baselineskip\noindent{\it 
  Proof of #1. }\ignorespaces#2\hfill\square\vskip\baselineskip}
\long\def\remark#1#2{\removelastskip\vskip\baselineskip\noindent{\bf
  Remark #1. }{\ignorespaces#2}\vskip\baselineskip}


\def\secno{0} 
\section{INTRODUCTION}
The main results of this note concern existence of continuous solutions of the
Dirichlet problem for fully nonlinear elliptic  equations as well as parabolic
variants.  To illustrate the issues, we consider  the Isaacs' equation
$$
\sup_\alpha\inf_\beta\Big(-\sum_{i,j=1}^na^{\alpha,\beta}_{i,j}(x)u_{x_i,x_j}(x)
+\sum_{j=1}^n b_j^{\alpha,\beta}(x)u_{x_j}(x)
+c^{\alpha,\beta}(x)u(x)-f^{\alpha,\beta}(x)\Big)=0\eq
$$ 
in a bounded open domain $\Omega\subset {\Bbb R}^n$ coupled with the Dirichlet condition
$$u(x)=\psi(x)
\text{for}x\in\partial \Omega\eq$$
in two situations.  In both cases the indices $\alpha, \beta$ can range over
countable sets while the symmetric
matrices $A^{\alpha,\beta}=\big(a_{i,j}^{\alpha,\beta}\big)$, the vectors
$b^{\alpha,\beta}=(b_1^{\alpha,\beta},\ldots,b_n^{\alpha,\beta})$, and the
functions $c^{\alpha,\beta}$ satisfy
$$\lambda I\le A^{\alpha,\beta}(x)\le \Lambda I\eq$$ for some positive constants
$0<\lambda\le\Lambda$, and
$$|b^{\alpha,\beta}(x)|\le \gamma, \qquad 0\le c^{\alpha,\beta}(x)\le \gamma \eq$$
for some constant $\gamma$, both uniformly in $\alpha,\beta$.
In the first situation, the functions $A^{\alpha,\beta}$, $b^{\alpha,\beta}$,
$c^{\alpha,\beta}$ and $f^{\alpha,\beta}$ are equicontinuous and equibounded on $\overline \Omega$;
we will call this the {\it continuous coefficient case}.  The
continuous coefficient case stands in contrast to the {\it measurable
coefficient case} which assumes (0.3), (0.4), the mere
measurability of the data
$A^{\alpha,\beta},b^{\alpha,\beta},c^{\alpha,\beta}, f^{\alpha,\beta}$, and the  technical but
essential condition $\inf_\alpha\sup_\beta f^{\alpha,\beta}\in L^n(\Omega)$. In both cases,
the
domain
$\Omega$ satisfies a uniform exterior cone condition while $\psi\in
C(\partial \Omega)$.

As far as we know,  no existence result  in the literature covers the
Dirichlet problem for (0.1) for the continuous coefficient case in the
generality stated. 
When speaking of solutions in this note, we mean continuous viscosity
solutions.  For background color, we note that the continuous coefficient
linear equation 
$$-\sum_{i,j=1}^na_{i,j}(x)u_{x_i,x_j}(x)+\sum_{j=1}^n
b_j(x)u_{x_j}(x)+c(x)u(x)-f(x)=0\eq$$
is a special case of (0.1). 
Of course, the Dirichlet problem for (0.5) has a unique strong
(here meaning $W_{\rm loc}^{2,n}$ pointwise a.e.) solution, which by [4],
Theorem 2.10 and Proposition 2.9, is a unique viscosity solution.  However, it is an
interesting
artifact of the history of the subject that there seems to be no quotable direct 
statement of the  existence of viscosity solutions of the Dirichlet problem  
in the literature covering this case.  However, there are ``good solutions" - see
e.g.\ Cerutti, Fabes and Manselli [6] - and ``good solutions" are standard
viscosity solutions in the continuous coefficient linear case.   The current note 
handles the general Isaacs' equations in a similar manner, and puts the matter in some
perspective.  Moreover, we treat the parabolic analogue as well.   Finally, existence
is proved for the  measurable coefficient case in both the elliptic and parabolic
settings.

 We will use two viscosity solution contexts.  The continuous
coefficient case lies within the  ``classical" viscosity solutions theory
outlined in [8].  The measurable coefficient case requires infrastructure
from Caffarelli, Crandall, Kocan and \Swiech\ [4], and Crandall, Fok,
Kocan and \Swiech\ [7].  The body of the paper is organized to accommodate the
reader who is not interested in the more technical measurable coefficient case at
this time.

The outline of our method is standard. In both cases, a fully nonlinear
equation $F=0$ including the Isaacs' equation as a special case is treated.
The equation $F=0$ is approximated by better equations $F^\epsilon =0$ for
which the Dirichlet problem is uniquely solvable, the solutions of the
approximate problems are uniformly bounded and equicontinuous, and the
approximations were set up so that available results guarantee that the
original problem is solved by uniform limits of solutions of the approximate
problems.  This last step uses the appropriate result from viscosity solutions
theory, which varies between the two cases.  

In the continuous coefficient case, we exploit the additional structure to
bracket the  original equation by approximations $F_\epsilon\le F\le F^\epsilon$ which
are monotone in the parameter $\epsilon$. This  automatically constructs  maximal
and
minimal solutions of the original Dirichlet problem.  The approximation
process is
interesting and replaces linear equations by nonlinear equations.  In the
measurable coefficient case (which of course includes the continuous
coefficient case),  approximation is by simple mollification of the equation in the
independent
variables.  We remark that as this paper goes to print 
R. Jensen and A. \Swiech\ have a paper in preparation 
which establishes
 the existence of maximal and 
minimal solutions in the measurable case using different arguments than employed 
by us in the continuous case.

Part of our motivation arises from the desire to quote these results
elsewhere.  Part of our motivation is that others should have a quotable
source for these results.  But there is a bit more to the matter than that.
For example, if the viscosity solution framework  is
to provide a basic existence platform for uniformly elliptic equations 
(in particular, we mean to exclude the use of
second derivative estimates on solutions of the equation under discussion, as
these are not available in general), as perhaps it should, then certainly  it is
nice to have the linear equation appear as special case of a general nonlinear result
for (0.1) with little cost for the added generality. 

The existence of continuous solutions is historically linked to uniqueness via
Ishii's implementation of Perron's method (e.g., [8], Section 4).  The issue
of
uniqueness of viscosity solutions of Isaacs' equation fans out in two
directions. 
If additional restrictions are put on the coefficients beyond those of the 
continuous coefficient case, one can establish uniqueness and then existence
by
standard viscosity solutions theory (see Ishii and Lions [15] and [8])
even for some  degenerate equations ((0.3) need not hold).  If the equation is
uniformly elliptic and either convex or concave in the Hessian matrix -- as is the
case for (0.1) when $a^{\alpha,\beta}$ is independent of $\beta$ -- the existence of
strong
solutions in the continuous coefficient case is a consequence of Caffarelli's
estimates [2] (see Caffarelli and Cabr\'e [3]) and some further
arguments, see [4].
   \Swiech\ [28], Theorem 3.1, provides   a sufficiently general statement.  In
the presence of strong solutions, viscosity solutions are unique as noted above.
For other
available results on the existence of continuous viscosity solutions we refer
to
[8],   [15] and Trudinger [31].

Existence for the problems studied here is decoupled from uniqueness and
higher regularity by means of simple approximations and compactness arguments.
Uniqueness in general remains an interesting issue for the continuous
coefficient case
of Isaacs' equation and fails even for the linear equation in the measurable
coefficient case according to Nadirashvili [24], see also Safonov [27].
Further
comments on uniqueness issues can be found in Section 1.

Our results in the measurable coefficient case  may be regarded as a
fully nonlinear generalization of the well-known ``good solution" existence theory
for the linear problem (0.5), (0.2); see  Cerrutti,  Escauriaza and
  Fabes [5].  Existence for the linear problem in the good solution
framework is demonstrated by smoothing the coefficients of the problem, using
the estimates of Krylov and Safonov [19], [14] to obtain compactness and
defining by fiat the limit of strong solutions of approximate problems to be
a good solution. We follow this outline, but do not have regular solutions
available at any stage of approximation.  Thus we rely on viscosity solution
theory to provide solutions of approximate problems and on a suitable
intrinsic notion of solution of the equation itself when passing to the limit.

Section 1 contains some preliminaries and the statement of the result on
maximal and minimal solutions in the continuous coefficient case.   Section 2
contains the proof of existence together with its parabolic analogue. An
ingredient used in the proof of Section 2 is the existence of subsolutions and
supersolutions.  These   are constructed in Section 3. We present explicit
constructions here since a quotable  reference is needed and the literature
concerning this issue under the exterior cone condition is a little hazy
(see Remark 3.3\ and various  comments made in Section 3). Section 4
treats  the measurable coefficient case.


\def\secno{1}
\section{PRELIMINARIES}
The equation (0.1) can be written as $F(x,u(x),Du(x),D^2u(x))=0$,
where $F(x,r,p,X)$ is defined for $x\in\overline \Omega$, $r\in{\Bbb R}$, $p\in {\Bbb R}^n$  and
$X\in{\cal S}(n)$ (the set of symmetric $n\times n$ real matrices) by
$$ F(x,r,p,X)
=\sup_{\alpha}\inf_{\beta}\left(-\trace{A^{\alpha,\beta}(x)X}
+\langle b^{\alpha,\beta}(x),p\rangle 
+c^{\alpha,\beta}(x)r-f^{\alpha,\beta}(x)\right).\eq
$$ 
Here $\langle \cdot,\cdot\rangle$ denotes the Euclidean inner-product.

Properties of
$F$ guaranteed by (0.3) and (0.4) are recalled next.
Let $X^+$, $X^-$ denote the positive and negative parts of $X\in
{\cal S}(n)$; e.g. $X=X^+-X^-$ and  $\trace {X^+} $ is the sum of the
positive eigenvalues of $X$.  Let
$${\cal P}^+(X)=-\lambda\trace{X^+}+\Lambda\trace{X^-},\quad
{\cal P}^-(X)=-\Lambda\trace{X^+} +\lambda\trace{X^-}$$ be the ``Pucci extremal
operators''.  It is standard and straightforward to show that $F$  satisfies
the following conditions:
$$\eqalign{{\cal P}^-(X-Y)-\gamma|p-q|\le F(x,r ,p,X)-F(x,r,q,Y)\le
{\cal P}^+(X-Y)+\gamma |p-q|}\eq$$
for $x\in\overline \Omega$,
$r\in{\Bbb R}$, $p,q\in {\Bbb R}^n$ and $X,Y\in{\cal S}(n)$, and
$$F(x,r,p,X)\text{is nondecreasing in}r.\eq$$
To prove (1.2), one first treats a single linear operator and then
observes that the  inequalities are preserved under sup-infs. For convenience, we
adopt the shorthand:
$$F\in{\cal SC}\iff\ (1.2) \ \&\  (1.3)  \quad {\rm hold}.$$
The parameters $\lambda, \Lambda, \gamma$ are fixed throughout the discussion. ${\cal SC}$
corresponds to ``structure conditions''.

The first inequality of (1.2) with $p=q$  shows that
$F(x,r,p,X)$ is nonincreasing in $X$, which together with the
monotonicity in $r$ is the meaning of ``$F$ is proper" in the
language of [8].  When $F$ is proper and continuous, [8]
outlines the basic theory of merely continuous viscosity solutions
of $F=0$.



Our main result in the continuous coefficient elliptic case concerns the
Dirichlet problem (DP) below. In (DP) and everywhere else, $\Omega$ is  assumed
to
be a bounded open domain in ${\Bbb R}^n$, $n\ge2$.
$$F(x,u,Du,D^2u)=0\text{in}\Omega,\quad u=\psi\text{on}\partial \Omega.
\eqno{(\rm DP)}$$ 
Terminology used in the statement is explained following it.

\theorem{1.1}{Let $\Omega$ satisfy a uniform exterior cone condition,
$F\in{\cal SC}$ and
$\psi\in C(\partial \Omega)$.  Assume also that $F$ is continuous.  Then there
are
$C$-viscosity  solutions $\overline u,\ \underline u\in C(\overline \Omega)$ of (DP) such
that any other  $C$-viscosity    solution   $u$ of  (DP) satisfies  
$\underline u\le u\le\overline u$.}


We note again that neither the theory of [8] nor  additional results of
[15]  applicable to the case $F\in{\cal SC}$ provide  uniqueness of solutions
of the Dirichlet problem for continuous $F\in {\cal SC}$; the question seems to be
open. This is one reason the  existence issue has not been treated to date.
It
remains   possible that uniqueness holds and $\underline u= u=\overline u$.
Further comments on the current situation regarding uniqueness can be found
at the end of this section.

The ``uniform exterior cone condition'' is recalled in Section 3, during the
construction of appropriate subsolutions and supersolutions. One of the
resources provided by this work is a quotable source for these subsolutions
and supersolutions under this general assumption on the boundary.

It remains to explain the term  a ``$C$-viscosity   solution of (DP)''. There are two
parts to this: the equation and the boundary condition. The boundary condition
is interpreted in the strict sense:
$$\overline u(x)= \underline u(x)=\psi(x)\text{for}x\in\partial\Omega.$$
 Regarding the equation ``$C$-viscosity'' means what ``viscosity'' means in
[8].  That is, $u$ is a  $C$-viscosity   solution  of $F\le 0$ (equivalently, a  
$C$-viscosity
subsolution of $F= 0$) if $u\in{\rm USC}(\Omega)$ -- the space of all upper
semicontinuous functions on $\Omega$ -- and for every
$\varphi\in C^2(\Omega)$ and local maximum point $\hat x\in\Omega$ of $u-\varphi$,
one has $F\left(\hat x,u(\hat x),D\varphi(\hat x),D^2\varphi(\hat x)\right)\le 0$. The notion of a
$C$-viscosity supersolution (equivalently, a solution of $F\ge 0$) arises by
replacing  ``upper semicontinuous'' by ``lower semicontinuous'',
``max'' by ``min'' and reversing the inequality to
$$
F\left(\hat x,u(\hat x),D\varphi(\hat x),D^2\varphi(\hat x)\right)\ge 0\,. $$
 $C$-viscosity solutions are
functions which are simultaneously a $C$-viscosity subsolution and a $C$-viscosity
supersolution. The appendage of the modifier ``$C$'' here results
from the fact that ``$L^p$-viscosity'' notions are used in Section
4, and it will be necessary to refer to both concepts there.  The
parabolic case is incorporated in the obvious way (or see [8]).

At this juncture, we revisit the uniqueness issue. In the course of proof of
 Theorem 1.1, continuous $C$-viscosity subsolutions and supersolutions of (DP)
satisfying the boundary condition will be constructed.  This demonstration
uses
$F\in{\cal SC}$. If we also know that a subsolution $u$ and a supersolution $v$ of
$F=0$ in $\Omega$ satisfying $u,-v\in {\rm USC}(\overline \Omega)$ and $u\le v$ on $\partial \Omega$
must
satisfy $u\le v$ in $\Omega$, then it is standard that there is a unique solution
of (DP). When this strong comparison result holds, we say {\it comparison
holds}.

To assert that comparison holds via the theorems of [8] and [15] 
one must  impose structure on the continuity of $F(x,r,p,X)$ in $x$.  In the
current case, for $F$ given by (1.1), if the $A^{\alpha,\beta}$, etc., are
uniformly continuous in $x$ uniformly in $\alpha,\beta$, then
$$|F(x,r,p,X)-F(y,r,p,X)|\le \omega(|x-y|)(1+|r|+|p|+\|X\|)\eq$$ for
some continuous $\omega\colon\,[0,\infty)\rightarrow[0,\infty)$ satisfying
$\omega(0)=0$ ($\|X\|$ is any  matrix norm of $X$);  $\omega$ is obtained
from the uniform moduli of continuity of the coefficients of the
linear operators.

While proving uniqueness it is enough however to establish comparison for two
solutions, say $u$ and $v$. It follows from the results of Caffarelli [2],
 that $F\in{\cal SC}$
and (1.4) are enough to guarantee that $C$-viscosity solutions of $F=0$ are
$C_{\rm loc}^{1,\alpha}$ for all $0<\alpha<\bar\alpha$, where $\bar\alpha =\bar\alpha(\lambda,\Lambda,n)\in
(0,1)$. (See also Trudinger [29] for an early result in this direction
and \Swiech\ [28], Theorem 2.1, for a more general statement.) In
particular,
$u,v\in C_{\rm loc}^{1,\alpha}$, and then uniqueness can be proved under
restrictions on $\omega$ as follows. First, by Section V.1 of [15], without
loss of generality we can assume that $u$ solves $F\le -\kappa$ for some
$\kappa>0$.  Then we can combine the proof of Proposition III.1 (2) of [15]
with the arguments from Section 5.A of [8] (which show how to relax the
standard comparison assumptions when functions are $C^{1,\alpha}$) to prove
comparison if $\omega$ in (1.4) satisfies
$\omega(r)\le  Cr^\theta$ for some $\theta>(1-\bar\alpha)/(2-\bar\alpha)$.  This
approach makes full use of ${\cal SC}$. If $\theta>\frac12$ then $F\in{\cal SC}$ can be
somewhat weakened, and uniqueness of solutions still holds, see [15]. For
other results in this direction see Jensen [16] and Trudinger
[31].


For the continuous coefficient linear case (0.5) existence of $W^{2,n}_{\rm loc}(\Omega)$
solutions is known. These solutions are also unique $C$-viscosity solutions -- this is
a special case of  Theorem 2.10 of [4] aided by Proposition 2.9 of the
same
work. For the elliptic case, the most general results on existence of
$W^{2,n}_{\rm loc}(\Omega)$ solutions for $F\in{\cal SC}$ and convex or concave in the Hessian are
found in [28]; the parabolic analogue is in [10] (which makes use of the
results herein).  These latter results rely on foundational estimates of Caffarelli
[3], Wang [32] and the contributions of Escauriaza [11].

Finally, in the good solution framework for linear equations, the results and
commentary of Safonov [25] and  Cerutti, Fabes and Manselli [6]
indicate what is known on the positive side.  As mentioned in the
introduction, Nadirashvili [24] shows nonuniqueness in general.  See also
Safonov [27].

\def\secno{2}
\section{EXISTENCE PROOF FOR CONTINUOUS $F$}
{\it Throughout  this section, the terms subsolution, supersolution
and solution mean, respectively, $C$-viscosity subsolution, $C$-viscosity supersolution
and $C$-viscosity solution (see above).}



We are ready for the proof of Theorem 1.1.
\proofof{Theorem 1.1}{The idea for the proof, once conceived,
makes the rest simple.  The point is to find approximating equations
$F_\epsilon =0$
and $F^\epsilon =0$ with better dependence on $x$ and satisfying $F_\epsilon\le
F\le F^\epsilon$.  Even if $F$ is linear, there is in general no linear
approximation with the properties we need. Put
$$F_\epsilon(x,r,p,X)= \min_{y\in \overline \Omega}\left(F(y,r,p,X)
+\frac1\epsilon |x-y|\right).\eq$$ Since for each fixed $y\in\overline \Omega$
$$ F(y,r,p,X) +\frac1\epsilon |x-y|$$ belongs to ${\cal SC}$ and has
  the same parameters $\gamma, \lambda, \Lambda$ and
continuity in $r$ as $F$, $F_\epsilon$ shares these properties. The striking
thing is that $F_\epsilon$ is Lipschitz continuous in
$x$ with constant $1/\epsilon$ uniformly in $r,p,X$ while preserving the rest of
the structure.  The operation of ``inf-convolution" used here is standard,
but this use of it is unusual.
 By the
definition $F_\epsilon\le F$ (choose $y=x$ in
(2.1)).  Next,  $F$ is continuous on $\overline \Omega\times{\Bbb R}\times{\Bbb R}^n\times{\cal S}(n)$,
so for  $R>0$ there exists $\omega_R\colon\,[0,\infty)\rightarrow[0,\infty)$ such that
$\omega_R(0+)=0$ and
$$|F(x,r,p,X)-F(y,r,p,X)|\le \omega_R(|x-y|)\text{for}|r|+|p|+\|X\|\le R\eq$$
when $x,y\in\overline \Omega$.  Then for $|r|+|p|+\|X\|\le R$
$$\eqalign{F(x,r,p,X)\le& F(y,r,p,X)+\omega_R(|x-y|)\cr
&\le F(y,r,p,X)+\frac1\epsilon|x-y|+\omega_R(|x-y|)-\frac1\epsilon|x-y|,}$$
so  we have
$$F_\epsilon(x,r,p,X)\le F(x,r,p,X)\le F_\epsilon(x,r,p,X)+\delta_R(\epsilon),$$
where
$$\delta_R(\epsilon)=\sup_{0< s\le {\rm diam}(\Omega)}
\left(\omega_R(s)-\frac s\epsilon\right)\rightarrow 0\text{as}\epsilon\downarrow 0.\eq$$ 
In particular,
$$F_\epsilon(x,r,p,X)\rightarrow F(x,r,p,X)\text{uniformly for} x\in\overline \Omega\text{and
bounded} r,p, X\eq$$
as  $\epsilon\downarrow 0$.  Similarly, we define
$$F^\epsilon(x,r,p,X)=\sup_{y\in\overline
\Omega}\left(F(y,r,p,X)-\frac1\epsilon|x-y|\right),\eq$$
which has all the same structure properties as $F_\epsilon$ and
satisfies
(2.4) in place of $F_\epsilon$.  Moreover for $0<\hat\epsilon<\epsilon$
$$F_\epsilon \le F_{\hat\epsilon}\le F\le F^{\hat\epsilon}\le F^\epsilon.$$

We next claim that the Dirichlet problem (DP) with $F_\epsilon$ in
place of
$F$ has a unique solution $u_\epsilon\in C(\overline \Omega)$.  To prove this in the standard
way (see Section 4 of [8]), we need to know that comparison holds. Since
$F_\epsilon$ is {\it globally Lipschitz continuous in $x$ with constant $1/\epsilon$}
and proper, if $X\le Y$ then
$$F_\epsilon(y,r,p,Y)-F_\epsilon(x,r,p,X)\le F_\epsilon(y,r,p,Y)-F_\epsilon(x,r,p,Y)\le
\frac1{\epsilon}|x- y|$$
whenever $x,y\in\overline \Omega$, $r\in R,\ p\in{\Bbb R}^n$; in particular, (3.14)
of [8] trivially holds.
Moreover, any subsolution may be perturbed to a strict subsolution via
[15], Section V, so comparison holds, see Section 5.C in [8].  Suitable
supersolutions and subsolutions achieving boundary values in a continuous
fashion are constructed in Section 3, so we may invoke Perron's method  to obtain
the result. The same analysis produces a solution
$u^\epsilon$ of the Dirichlet problem for $F^\epsilon=0$.

Since $F_\epsilon\le F\le F^\epsilon$, if $u$ is any solution of the Dirichlet
problem for $F=0$,  it is also a
subsolution for $F_\epsilon$ and a supersolution for
$F^\epsilon$ and so $u^\epsilon\le u\le u_\epsilon$ by comparison for the approximate
equations.  In the same way, if $0<\hat\epsilon\le \epsilon$, then $u^\epsilon\le
u^{\hat\epsilon}
\le u_{\hat\epsilon}\le u_\epsilon$, so these families of functions attain
the boundary values in an equicontinuous manner. According to e.g.
Trudinger [30] (see also Caffarelli [2], Caffarelli and
Cabr\'e [3], Fok [13] and [28]), they are also locally equi-H\"older
continuous in $\Omega$, so there are uniform limits
$$\lim_{\epsilon\downarrow 0}u^\epsilon =\underline u\le \overline u
=\lim_{\epsilon\downarrow
0}u_\epsilon.$$ By the standard stability result for viscosity
solutions (see Section 6 of [8]) and (2.4) for $F_\epsilon$
and $F^\epsilon$, $\underline u,
\overline u$ are  solutions of $F=0$ and thus they are minimal and
maximal solutions of the Dirichlet problem for $F=0$. }

We turn to the parabolic case. In this situation, we have $0<T$,
set $Q=\Omega\times(0,T]$, and use
$$\partial_pQ=\partial \Omega\times(0,T]\cup \overline \Omega\times\{0\}$$ to denote the
parabolic boundary of $Q$.

We consider the Cauchy-Dirichlet problem
$$u_t+F(x,t,u,Du,D^2u)=0\text{in}
Q\text{and}u=\psi\text{on}\partial_pQ,\eqno{\rm (CDP)}$$ where $\psi\in
C(\partial_pQ)$. Now $F\in{\cal SC}$ will mean that for each
$t\in[0,T]$ the mapping $(x,r,p,X)\mapsto F(x,t,r,p,X)$ belongs to
${\cal SC}$ in the sense of Section 1.

The analogue of Theorem 1.1\ is:
\theorem{2.1}{Let $\Omega$ satisfy a uniform exterior cone condition,
$F\in{\cal SC}$ be continuous on $\overline \Omega\times[0,T]\times{\Bbb R}\times{\Bbb R}^n\times {\cal S}(n)$ and
$\psi\in C(\partial_pQ)$.  Then there are $C$-viscosity solutions $\overline u,\ \underline
u\in
C(\overline Q)$ of (CDP) such that  if $u$ is another $C$-viscosity  solution, then
$\underline u\le u\le
\overline u$.}


Precisely the same outline as succeeds for the elliptic case proves Theorem
2.1. The subsolutions and supersolutions required are provided in the
next section. Concerning the  interior H\"older continuity of viscosity
solutions of parabolic equations see Wang [32] and Section 5 of [10] (see
Krylov [18] and Lieberman [20] for classical results). See [8] Section 8 for
other standard adaptations to prove existence in the parabolic case.

The compactness of the approximations $u_\epsilon$, $u^\epsilon$ 
in $C(\overline  \Omega)$ (or $C(\overline Q)$) is used above.  The monotonicity of these
families
was  invoked to control continuity up to the boundary.  However, this does not
reveal the
full compactness available in these circumstances.  In Section 4 more is
needed, and the
appropriate general compactness result is given. 

\def\secno{3}
\section{CONSTRUCTION OF SUBSOLUTIONS AND SUPERSOLUTIONS}

\noindent{\bf Elliptic Case.} 

We turn to the construction of subsolutions and supersolutions.
There is only one task here, not two, as the next remark recalls:

\remark{3.1}{We note the following standard reduction:  $u$ is a
supersolution of an equation $F(x,u,Du,D^2u)=0$ if and only if $
v=-u$ is a subsolution of $\tilde F(x,v,Dv,D^2v)=0$, where $\tilde
F(x,r,p,X)=-F(x,-r,-p,-X)$; moreover,  noting that if $F(p,X)
={\cal P}^-(X)-\gamma|p|$, then $\tilde F(p,X)={\cal P}^+(X)+\gamma|p|$, one sees
$\tilde F\in{\cal SC}$ if and only if $F\in{\cal SC}$. Thus it suffices to
construct either supersolutions or subsolutions.}

We will construct a supersolution $U\in C(\overline \Omega)$ of (DP) for $F_\epsilon$ such
that
$U(x)=\psi(x)$ on $\partial \Omega$ and $U\ge R=\inf_{\partial\Omega}\psi$. Moreover, we
will track the continuity properties of $U$. To begin, we use
$F_\epsilon\in{\cal SC}$ so that by (1.2)
$$F_\epsilon(x,r,p,X)\ge
{\cal P}^-(X)-\gamma|p|+F_\epsilon(x,r,0,0)$$ and therefore a supersolution of
${\cal P}^-(D^2U)-\gamma|DU|+F_\epsilon(x,U,0,0)=0$ in $\Omega$ is also a
supersolution for $F_\epsilon$.  If $U\ge R$, then
$-F_\epsilon(x,U,0,0)\le -F_\epsilon(x,R,0,0)$. It follows that if $M\ge
-F_\epsilon(x,R,0,0)$ for all $x\in\Omega$, and $U\ge R$ solves
$${\cal P}^-(D^2U)-\gamma|DU|\ge M,\eq$$  then $U$ is a supersolution for
$F_\epsilon$.

On the other hand it is true in general that if $U$ is a $C$-viscosity solution
of (3.1)   with $M\ge 0$  and $U\ge\psi$ on $\partial \Omega$,  then the
Alexandrov--Bakelman--Pucci maximum principle for viscosity supersolutions
(see, e.g., [3], [30] or [4], Proposition 2.12) implies  that
$u\ge\inf_{\partial \Omega}\psi$. Thus if $M\ge
\sup_{x\in\Omega}\left(-F_\epsilon(x,\inf_{\partial \Omega}\psi,0,0)\right)$ and
$M\ge0$, a solution of (3.1) satisfying $U=\psi$ on $\partial \Omega$ is a
supersolution of the Dirichlet problem for $F_\epsilon$.

Let $M>0$. The results of Miller [22], [23] provide
the existence of local barriers for the Dirichlet problem for
(3.1) under a uniform exterior cone condition.  We do not know
a place in the literature where global barriers (supersolutions)
are constructed, although the case $\gamma=0$ is treated in Michael
[21] and the proof there may be modified to handle the
general case -- see Remark 3.4. We present another option, using the
flexibility of viscosity solutions.

First we recall the nature of the barriers on exterior cones for
extremal elliptic operators constructed by Miller [22],
[23]. For $n\ge2$ and $\beta\in(0,\pi)$ let
$$T_\beta=\left\{x\in{\Bbb R}^n\colon\ x_n\ge(\cos\beta)|x|\right\}$$ be
the closed circular cone of aperture $\beta$ with axis in the
direction of $-e_n$. Consider barriers of the form
$$w(x)=r^b f(\theta),\eq$$ where $r=|x|$ and
$\theta=\arccos\left(x_n/|x|\right)$. It is shown in [23], Theorem 3
and  Section 7, that for every $\beta\in(0,\pi)$ there exist
$b\in(0,1)$ and $f\in C^2([0,\pi))$, depending only on
$\lambda,\Lambda,n,\beta, \gamma$, such that $f'(0)=0$ and $f>1$ on $[0,\beta]$,
so that $w$ given by (3.2) is continuous on $T_\beta$ and $C^2$ on
${\Bbb R}^n\setminus\{$closed negative $x_n$ axis$\}$ and
$$w>r^b\ \ {\rm on}\ T_\beta\setminus\{0\},\ \ w(0)=0,\eq$$ and,
crucially,
$${\cal P}^-(D^2w)-\gamma|Dw|\ge r^{b-2}\quad{\rm on}\ \ {\rm
int}(T_\beta).\eq$$


Now let $\Omega$ be a bounded domain in ${\Bbb R}^n$, $n\ge2$, satisfying a
uniform exterior cone condition. This means that there exist
$\beta\in(0,\pi)$ and
$r_0>0$ so that for every $z\in\partial\Omega$ there is a rotation
$\Theta=\Theta(z)$ such that
$$\overline\Omega\cap B_{r_0}(z)\subset z+\Theta T_\beta.\eq$$ Here,
$B_{r_0}(z)$ denotes the open ball in ${\Bbb R}^n$ of radius $r_0$ centered
at $z$. The ``local'' nature of the barriers below is due to the
possibility that $\Omega\subset z+\Theta T_\beta$ does not hold.
Setting
$w_z(x)=w(\Theta^{-1}(x-z))$, from
(3.3) we have
$$w_z(z)=0,\quad w_z(x)\ge|z-x|^b\quad{\rm on}\ \ \overline\Omega\cap
B_{r_0}(z).\eq$$ In particular,  we have
$$w_z\ge (r_0)^b\quad{\rm on}\ \ \{x\in\overline\Omega
\colon\ \ |x-z|=r_0\}.\eq$$ 
Using (3.4) and (3.5) we arrive at
$${\cal P}^-(D^2w_z(x))-\gamma|Dw_z(x)|\ge |x-z|^{b-2}\quad{\rm for}
\ \ x\in\Omega\cap B_{r_0}(z).\eq$$

We need to extend these local barriers to global ones. Choose any
point $y\not\in\overline \Omega$ and $2r_1<{\rm distance }\,(y,\partial \Omega)$. For 
$\sigma>0$
put
$$G(x)=\left(\frac1{r_1^\sigma}-\frac1{|x-y|^\sigma}\right).\eq$$ Clearly
$$G(x)\ge {2^\sigma-1\over (2r_1)^\sigma}>0\text{on}\overline \Omega\eq$$ and a
standard computation ([14])   shows that
$${\cal P}^-(D^2 G(x))-\gamma|DG(x)|\ge {\sigma\over
|x-y|^{\sigma+2}}\left((\sigma+1)\lambda-\Lambda(n-1)-\gamma|x-y|\right)>0\eq$$ on $\overline \Omega$ for
large $\sigma$ (depending only on $n,\lambda,\Lambda,\gamma$ and diam$\,(\Omega$)).
Replacing $G$ by $aG$ for a suitable $a>0$  we can achieve all of:
$$G>0\text{and} {\cal P}^-(D^2 G)-\gamma|DG|\ge\kappa \text{on}\overline \Omega\eq $$ for some
$\kappa>0$ and
$$G(x)<\frac12(r_0)^b\text{for}x\in\overline \Omega.\eq$$ Then the function
$$
W_z(x)=\cases{G(x)             & for $x\in\overline\Omega,\ |x-z|>r_0$,  \cr 
  \min\left(G(x),w_z(x)\right) & for $x\in\overline\Omega,\ |x-z|\le r_0$\cr}\eq
$$ 
agrees with $w_z$ in a neighborhood of $z\in\partial \Omega$ 
relative to $\overline \Omega$ (in view of (3.6)
and (3.12)), agrees with $G$ on $\overline \Omega\setminus B_{r_2}(z)$ for
some $0<r_2<r_0$ (due to (3.7), (3.13)), and is a solution of
${\cal P}^-(D^2 W_z)-\gamma|DW_z|\ge \kappa_1$ in $\Omega$ provided that both
$w_z$ and $G$ satisfy the same relation in
$B_{r_0}(z)\cap\Omega$ and $G$ does in all of $\Omega$. Hence, in view of
(3.12) and (3.8), we may multiply $W_z$ by a constant and have
all of the following properties of the resulting function (still
called $W_z$):
$$W_z\in C(\overline \Omega),\quad W_z(z)=0,\quad
W_z>0\text{on}\overline \Omega\setminus\{z\}\eq$$ and
$${\cal P}^-(D^2W_z)-\gamma|DW_z|\ge 1\quad{\rm on}\
\ \Omega.\eq$$

The task of satisfying the boundary condition remains.  Let $\psi\in
C(\partial \Omega)$ and
$$|\psi(x)-\psi(z)|\le \rho(|x-z|)\quad{\rm for\quad}x,z\in\partial \Omega,\eq$$
where $\rho(0+)=0$, so $\rho$ is a modulus of continuity for $\psi$.
In addition to ${\cal P}^-(D^2U)-\gamma|DU|\ge M$, the supersolution $U$ we
construct will satisfy
$$|U(x)-\psi(z)|\le \omega(|x-z|)\text{for}x\in\Omega,\ z\in\partial \Omega,\eq $$
where $\omega(0+)=0$; that is the boundary values are assumed
uniformly. Moreover, $\omega$ will depend only on the parameters of
the cone condition,
$\lambda,\Lambda,n,\gamma$ and the diameter of $\Omega$ (which already determine
the character of each $W_z$), and $M$ and $\rho$.  For each
$\kappa>0$ and
$z\in\partial \Omega$ put
$$W_{\kappa,z}(x)=\psi(z)+\kappa +M_\kappa W_z(x),$$ where
$M_\kappa\ge M$ (guaranteeing
${\cal P}^-(D^2W_{\kappa,z})-\gamma|DW_{\kappa,z}|\ge M$ by (3.16)) is
chosen so that
$$\psi(z)+\kappa +M_\kappa W_z(x)\ge \psi(x)\text{for}x\in\partial \Omega. $$
 In view of  (3.17), it suffices to take
$$M_\kappa\ge \sup_{x\in\partial \Omega,x\not=z}{(\rho(|x-z|)-\kappa)^+\over
W_z(x)};$$ this may evidently be done uniformly in $z\in\partial \Omega$.
Finally we put
$$W(x)=\inf_{z\in\partial \Omega,\kappa>0}W_{\kappa,z}(x).$$ By construction $W\ge
R$. Since for all $\kappa$
$$W(x)-\psi(z)\le W_{\kappa,z}(x)-\psi(z)=\kappa +M_\kappa W_z(x) $$
and $W_z(x)$ is uniformly continuous in $x$ uniformly in $z$, we
conclude that for all $z\in\partial \Omega$ and $x\in\Omega$
$$W(x)-\psi(z)\le \omega(|z-x|)\eq$$ for some $\omega$ satisfying
$\omega(0+)=0$. We now use Remark 3.1\ -- the supersolutions of
(3.1) we have constructed imply the existence of corresponding
subsolutions of $F_\epsilon\le 0$ (or
${\cal P}^-(D^2U)-\gamma|DU|\le-M$ for an appropriate $M$) with boundary
values below $\psi$, call them $Y_{\kappa,z}$ and the supremum
$Y$.  By the analogue of (3.19) for $Y$ we have
$$-\omega(|x-z|)\le Y(x)-\psi(z).\eq$$ According to [8], $U=W_*$,
the lower semicontinuous envelope of $W$, is a supersolution of
(3.1), and consequently of $F_\epsilon=0$. Similarly,
$V=Y^*$, the upper semicontinuous envelope of $Y$, is a subsolution
of
$F_\epsilon=0$. Since $V=U=\psi$ on $\partial \Omega$, comparison gives $V\le U$
and using this together with (3.19) and (3.20) yields
$$|V(x)-\psi(z)|,\ |U(x)-\psi(z)|\le \omega(|z-x|)$$ and we are done.

For convenient reference, we summarize the results of this
construction in terms of extremal equations:

\proposition{3.2}{Let $\Omega$ satisfy a uniform exterior cone
condition, $\psi\in C(\partial \Omega)$ and $M\in{\Bbb R}$. Then the problems
$${\cal P}^-(D^2u)-\gamma|Du|=M\quad{in}\ \ \Omega,\quad  u=\psi\quad{on}\ \ \partial \Omega\eq$$ and
$${\cal P}^+(D^2v)+\gamma|Dv|=-M\quad{in}\ \ \Omega,\quad v=\psi\quad{on}\ \ \partial \Omega\eq$$ have
unique $C$-viscosity solutions $u,v\in C(\overline \Omega)$ satisfying $u=v=\psi$ on
$\partial \Omega$. Moreover, there is a modulus $\omega$ depending only on the
parameters of the cone condition, $\lambda,\Lambda,n,\gamma$, ${\rm
diam}\,(\Omega)$, $M$ and the modulus of continuity of $\psi$ such that
$$|u(x)-\psi(z)|,\  |v(x)-\psi(z)|\le \omega(|x-z|)\quad{for}\ \ z\in
\partial \Omega,\ x\in\Omega.$$}

Regarding the statement, recall Remark 3.1; moreover, given the
subsolutions and supersolutions exhibited above, we may assert the
existence of solutions, not only subsolutions and supersolutions.  


\remark{3.3}{ Bellman equations (3.22) and (3.21) are
concave/convex in the Hessian matrix
and as such can be studied by classical methods, see Krylov
[18]. In particular, Safonov [26], Theorem 1.1, proves that under
the assumptions of Proposition 3.2, the problems (3.22) and (3.21)
have classical $C^{2,\alpha}_{_{\rm loc}}(\Omega)\cap C(\overline \Omega)$ solutions. From
uniqueness it follows that $C$-viscosity solutions $u,v$ of Proposition
3.2\ coincide with Safonov's; in particular $u,v\in C^2(\Omega)$.
However, we feel that the construction presented here is
 useful. The problems (3.22) and (3.21) were solved here --
albeit in a weaker sense -- without invoking the apparatus of hard
$C^{2,\alpha}$ estimates for nonlinear equations. Our objective is to
solve equations $F_\epsilon=0$ that are not expected to have
classical solutions. $F_\epsilon=0$ is solved by Perron's method, and
for this purpose the information summarized in Proposition
3.2\ is sufficient.  Corollary 3.10 of [4] extends the existence
to cover the situation when $M$ is replaced by $f\in L^p(\Omega)$ for 
suitable $p$, a fact used in Section 4. 

As for the parabolic result, Proposition 3.5\ below, we were
not able to locate a quotable result in literature asserting
classical solvability of (3.25) and (3.26). However, Krylov
in [18], Theorem 6.4.3, proves an analogous result in the case of
$\Omega$ satisfying an exterior sphere condition, and this generalizes to handle
the cone condition. Krylov's method consists of approximating $\Omega$ from the
inside by more regular domains; a delicate argument involving barrier
functions
and H\"older  estimates is used to pass to the limit.   The result of Krylov
shows that $C$-viscosity solutions of Proposition 3.5\ are $C^{2,1}$ (and more).
This follows easily by  solving (CDP) classically on regular subdomains of
$\Omega\times (0,T]$ using $u$  ($v$, respectively) as the boundary data, and
invoking uniqueness.}


\remark{3.4}{ Our construction of barriers relies on the barrier
$w$ from (3.2) for a canonical unbounded cone $T_\beta$ at the origin, taken
from [22], [23]. We used uniform exterior cone
condition to obtain a local barrier $w_z$ at every $z\in\partial \Omega$;
$w_z$ is obtained by composing $w$ with an appropriate isometry
making $T_\beta$ into an exterior cone at $z$. Then $w_z$ was
extended to a global barrier $W_z$ (3.14) by means of a fixed
function $G$ in
(3.9).

Another possibility would be to first construct a barrier $W_0$ on the
exterior of a canonical bounded cone $C_{\beta,\delta}$ at the origin:
$$C_{\beta,\delta}=\left\{x\in{\Bbb R}^n\colon\ |x|\le\delta,\ x_n
\le(\cos\beta)|x|\right\}.$$ This can be accomplished by a similar
procedure as above. Namely, taking $y=-\frac\delta 2 e_n$, sufficiently
small $r_1>0$ (determined only by $\delta,\beta$) and $G$ as in
(3.9), for $\sigma$ large, depending only on $n,\lambda,\Lambda,\gamma$
and ${\rm diam}(\Omega)$ known in advance, one can guarantee
$$G>0\text{and} {\cal P}^-(D^2 G)-\gamma|DG|>0 \text{on}B_{{\rm diam}(\Omega)}(0)
\setminus C_{\beta,\delta}.$$ As in (3.14), a multiple of this $G$
combined with $w$ would produce a desired barrier $W_0$. Now one can
use uniform exterior cone condition to find for every $z\in\partial \Omega$ a
rotation $\Theta=\Theta(z)$ such that
$$\overline\Omega\cap\left( z+\Theta C_{\beta,\delta}\right)=\{z\},$$ and then
$W_z(x)=W_0\left(\Theta^{-1}(x-z)\right)$ defines a global barrier at
$z$.

Michael [21] considers barriers
$$\varphi(x)=1-e^{-Kw(x)},$$ where $w$ is Miller's barrier (3.2) and
$K>0$. [21] gives explicit recipes for $K,b$ and $f$ so that
$\varphi$ becomes a barrier for ${\cal P}^-(D^2\varphi)\ge r^{b-2}$ on the
exterior of $C_{\beta,\delta}$. This construction can be easily modified
to handle first order terms to obtain ${\cal P}^-(D^2\varphi)-\gamma|D\varphi|\ge1$
on $B_{{\rm diam}(\Omega)}(0)\setminus C_{\beta,\delta}$. This canonical
barrier $\varphi$ can be used instead of $W_0$ constructed above; note
that $\varphi$ is $C^2$ unlike $W_0$.

Finally, if $n=2$ the exterior cone condition can be replaced
by a weaker condition, see [22], [23] and Section 2.8
of [14].
}

\noindent{\bf Parabolic Case.} 

The work done above renders the parabolic case simple. To construct
supersolutions, we reduce as before to the problem
$$U_t+{\cal P}^-(D^2U)-\gamma|DU|\ge M.$$ Reviewing the preceding
construction, we see that all we need will follow if we produce a
function
$W_{z,\tau}$  for  each point $(z,\tau)$ of the (parabolic) boundary
$\partial \Omega\times (0,T]\cup
\overline \Omega\times\{0\}$ of
$Q$ satisfying the analogues of (3.15) and (3.16):
$$W_{z,\tau}\in C(\overline Q),\quad W_{z,\tau}(z,\tau)=0, \quad
W_{z,\tau}>0\text{on}\overline Q\setminus\{(z,\tau)\}\eq$$  and
$$(W_{z,\tau})_t+{\cal P}^-(D^2W_{z,\tau})-\gamma|DW_{z,\tau}|\ge 1\text{on} Q.\eq $$

For $\tau>0$ and $z\in\partial \Omega$ we set
$$W_{z,\tau}(x,t)=\frac1{2T}(t-\tau)^2+2W_z(x),$$ where $W_z$ was
constructed above and satisfies (3.15) and (3.16). It is clear
that (3.23) holds. Moreover, by (3.16),
$$\eqalign{(W_{z,\tau})_t+{\cal P}^-(D^2W_{z,\tau})&-\gamma|DW_{z,\tau}|\cr
=\frac1T(t-\tau)+&2\left({\cal P}^-(D^2W_z)-\gamma|DW_z|\right)\ge-1+2=1} $$ and we have
(3.24).

For $\tau=0$ and $z\in\overline \Omega$ we set
$$W_{z,0}(x,t)=At+\frac12|x-z|^2;$$ again if $A>0$ we clearly have
(3.23). Finally,
$$\eqalign{(W_{z,0})_t&+{\cal P}^-(D^2W_{z,0})-\gamma|DW_{z,0}|=\cr
&A+{\cal P}^-(I)-\gamma|x-z|=A-n\Lambda-\gamma|x-z|\ge A-n\Lambda-\gamma{\rm diam\,}(\Omega).
} $$ Thus we have (3.24) if $A=n\Lambda+\gamma{\rm diam\,}(\Omega)+1$.  The
rest of the analysis follows that of the elliptic case step by step.

Here is the parabolic version of Proposition 3.2. We use the
notation introduced in Section 2.
\proposition{3.5}{Let $\Omega$ satisfy a uniform exterior cone
condition, $\psi\in C(\partial_pQ)$ and $M\in{\Bbb R}$. Then the problems
$$u_t+{\cal P}^-(D^2u)-\gamma|Du|=M\quad{in}\ \ Q,\quad  u=\psi\quad{on}\ \ \partial_pQ\eq$$ and
$$v_t+{\cal P}^+(D^2v)+\gamma|Dv|=-M\quad{in}\ \ Q,\quad v=\psi\quad{on}\ \ \partial_pQ\eq$$
have unique $C$-viscosity solutions $u,v\in C(\overline{Q})$ satisfying
$u=v=\psi$ on
$\partial_pQ$. Moreover, there is a modulus $\omega$ depending only on the
parameters of the cone condition, $\lambda,\Lambda,n,\gamma,T$, ${\rm
diam}\,(\Omega)$, $M$ and the modulus of continuity of $\psi$ such that
$$|u(x,t)-\psi(z,\tau)|,\  |v(x,t)-\psi(z,\tau)|\le
\omega(|x-z|+|t-\tau|)\quad{for}\ \ (z,\tau)\in\partial_pQ,\ (x,t)\in Q.$$}


\def\secno{4}
\section{$L^p$ THEORY:  GENERAL EXISTENCE}

The requirements (1.2) and (1.3)
constituting the basic structure conditions require no continuity of
$F(x, r,p,X)$  in $x$ and very little in $r$.  In this section, we assume
that $F$ is merely measurable in $x$ (or $(x,t)$ in the parabolic case) while
satisfying the structure conditions for almost every $x$ (or $(x,t)$).  Due to
this generality we have to impose a requirement on the $r$ dependence: for
$R>0$ there exists $\omega_R\colon\,[0,\infty)\rightarrow [0,\infty)$ such that
$\omega_R(0+)=0$ and
$$|F(x,r,p,X)-F(x,s,p,X)|\le \omega_R(|r-s|)\eq$$
for almost all $x\in\Omega$ and $|r|+|s|+|p|+\|X\|\le R$. (Obviously, if $F$ is
continuous then (4.1) automatically holds.) In the parabolic case,
$x$ is replaced by $(x,t)\in Q$.

Of course, the notions of $C$-viscosity subsolutions, etc., are no longer appropriate in
this measurable situation, and there is now a well-developed theory using
corresponding ``$L^p$-viscosity''  notions ([4], [9],
[28], [7], [10]) which is built up from the fundamental
regularity results of Caffarelli [2] (see [3]) as further developed
by Escuariaza [11] and Wang [32]. In the linear case other notions of weak
solutions were proposed, see Cerrutti, Escauriaza and Fabes [5] and Jensen
[17]; relationships between various notions of solutions are studied in
[17] and [9].

\noindent{\bf $\bf L^p$-Viscosity  Notions}

In contrast to the $C$-viscosity notions recalled at the end of
Section 1, $L^p$-viscosity notions use ``test functions'' 
$\varphi\in W^{2,p}_{\rm loc}(\Omega)$
(functions whose distributional second derivatives are in
$L^p_{\rm loc}(\Omega)$) in the elliptic case and $\varphi\in W^{2,1,p}_{\rm loc}(Q)$  (functions
whose distributional first derivatives and second order spatial
derivatives are in $L^p_{\rm loc}(Q)$) in the parabolic case. In
addition, all subsolutions, etc., are required to be continuous.
For example, a continuous function $u$ on $\Omega$ is an $L^p$-viscosity
subsolution of
$F(x,u,Du,D^2u)=0$ if for every $\varphi\in W^{2,p}_{\rm loc}(\Omega)$ and local maximum
$\hat x$ of
$u-\varphi$ one has
$${\rm ess}\liminf_{x\rightarrow\hat x}F(x,u(x),D\varphi(x),D^2\varphi(x))\le
0;$$ equivalently, if for some $\epsilon>0$
$$F(x,u(x),D\varphi(x),D^2\varphi(x))\ge \epsilon\text{a.e.}$$ in some
neighborhood of $\hat x$, then $\hat x$ is not a local maximum of
$u-\varphi$. The  corresponding notions of $L^p$-viscosity
supersolutions, $L^p$-viscosity solutions, and the parabolic versions are what
then one expects.


Consulting the literature mentioned above, one finds that there is an
equation dependent appropriate range of $p$   determined by the
parameters $\lambda, \Lambda,n,\gamma{\rm diam}(\Omega)$ (or $\gamma{\rm diam}(Q)$ for
parabolic equations).  One always has $n/2<p$ in the elliptic case and
$(n+2)/2<p$ in the parabolic case. The range also  extends below $n$ in the
elliptic case and below $n+1$ in the parabolic case. The choices $p=n$ and
$p=n+1$ are the least possible which are appropriate for all choices of
$\lambda,\Lambda,\gamma, \Omega$.  In statements below we restrict our attention to the
``universal" choices $p=n$ and $p=n+1$ for simplicity.  However,  certain  
explicit arguments as well as  proofs of quoted results 
use the fact that extended ranges exist.

Note that if $q<p$, then the $L^q$-viscosity notions imply the
corresponding $L^p$-viscosity notions, as there are more test functions to check in the
$L^q$-viscosity case.  Thus $L^n$-viscosity solutions are automatically $L^p$-viscosity solutions for
$n<p$.   Similarly, if $F$ happens to be continuous, $L^n$-viscosity notions imply $C$-viscosity
notions. It is a substantial result that the converse is true in this form: if
$F$ is continuous and  $u$ is a continuous $C$-viscosity subsolution, etc., then it is
an $L^n$-viscosity subsolution, etc. In the elliptic case this is proved in Proposition
2.9 of [4], for the parabolic case see [10].

\smallskip
\noindent{\bf General Existence of $\bf L^n$-Viscosity Solutions}

We consider the Dirichlet problem for $G(x,u,Du,D^2u)=0$, where
$G\in{\cal SC}$ is merely measurable in $x$:
$$G(x,u,Du,D^2u)=0\text{in}\Omega,\quad u=\psi\text{on}\partial \Omega.\eq $$ As
usual, $\psi\in C(\partial \Omega)$.  However, it will be convenient to rewrite
(4.2) as
$$F(x,u,Du,D^2u)=f(x)\text{in}\Omega,\quad u=\psi\text{on}\partial \Omega,\eq  $$
where
$$F(x,r,p,X)=G(x,r,p,X)-G(x,0,0,0)\text{and}f(x)=-G(x,0,0,0),$$ so that
$$F(x,0,0,0)\equiv 0.\eq $$ Without loss of generality we hereafter
assume that (4.4)   holds. Note that then, via $F\in {\cal SC}$, (4.1) and
 (4.4)
$$  F(x,r,p,X)\le F(x,r,0,0)+{\cal P}^+(X)+\gamma|p|\le \beta(r) +{\cal P}^+(X)+\gamma|p|,$$
where $\beta(r)=\omega_{|r|}(|r|)$.  The analogous estimate from below combines
with this to yield
$$ |F(x,r,p,X)|\le \Lambda\|X\|+\gamma|p|+  \beta(r),\eq$$
where    we used the trace norm $\|X\|= \trace{X^+}+\trace {X^-}$ and
invoked $|{\cal P}^{\pm}(X)|\le \Lambda\|X\|$.  In particular,
$F(x,r,p,X)$ is bounded and measurable in $x$ for fixed $r,p,X$. This
guarantees that integrals occurring below are well defined.  We have the
following theorem:
\theorem{4.1}{Let $F\in{\cal SC}$ satisfy (4.1) and (4.4), let $f\in
L^n(\Omega)$, $\psi\in C(\partial \Omega)$ and let $\Omega$ satisfy a uniform exterior cone
condition. Then (4.3) has an $L^n$-viscosity solution. }

As a tool in the proof we will use:


\proposition{4.2}{Let $\Omega$ satisfy a uniform exterior cone
condition and ${\cal C}\subset C(\partial \Omega)$ be compact, $R>0$ and 
$B_R=\{f\in L^n(\Omega)\colon\ \|f\|_{L^n(\Omega)}\le R\}$.   
Then the set of all functions
$u\in C(\overline \Omega)$ such that there exists
$\psi\in{\cal C}$ and $f\in B_R$ for which $u$ is an $L^n$-viscosity solution of both
$${\cal P}^-(D^2 u)-\gamma|Du|\le f\text{\it and} -f\le 
{\cal P}^+(D^2 u)+\gamma|Du| \eq$$
in $\Omega$ and $u=\psi$ on $\partial \Omega$ is
precompact in $C(\overline \Omega)$. }

\proof{According to [4] Corollary 3.10, if $(\varphi,g)\in
C(\partial \Omega)\times L^n(\Omega)$, there exist a unique $U=U(\varphi,g)
 \in C(\overline \Omega)\cap W^{2,n}_{\rm loc}(\Omega)$ such that  
$$ {\cal P}^-(D^2 U)-\gamma|DU|=g\text{a.e. in}\Omega\text{and} u
=\varphi\text{on}\partial \Omega.  $$
We require several facts.  First, there exist $p\in(n/2,n)$ 
depending on $\lambda, \Lambda, n, \gamma\,{\rm
diam}\,(\Omega)$ 
(see [13], [11], [4], [28], [1]) and $C$ such that
$$U(\varphi,g)\le \sup_{\partial \Omega}\varphi+ C\left(\int_{\Omega}(g^+)^p\right)^{1\over
p}\text{for}(\varphi,g)\in  C(\partial \Omega)\times L^n(\Omega).\eq$$
Next the mapping 
$$  \ C(\partial \Omega)\times L^n(\Omega)\ni(\varphi,g)\rightarrow U(\varphi,g)\text{is sublinear and
order preserving.}\eq 
$$
Finally, if $u\in C(\overline \Omega)$ is an $L^n$-viscosity solution of 
$$ {\cal P}^-(D^2 u)-\gamma|Du|\le f\text{in}\Omega\text{and}u=\psi\text{on}\partial \Omega, \eq$$
where $f\in L^n(\Omega)$, then
$$ u\le U(\psi,f).\eq$$
We review the genesis of these results in Remark 4.4\ below.

The second inequality of (4.6) may be restated as $w=-u$ is an
$L^n$-viscosity solution of ${\cal P}^-(D^2 w)-\gamma|Dw|\le f$, so if (4.6) holds (4.10) implies $-u\le
U(-\psi,f)$ or
$-U(-\psi,f)\le u$. All told, (4.6) and $u=\psi$ on $\partial \Omega$ yield
$$-U(-\psi,f)\le u\le U(\psi,f).\eq$$

From (4.11) and (4.7) it follows that $u$ remains bounded in $C(\overline \Omega)$ 
if $(\psi,f)$ remains bounded in
$C(\partial \Omega)\times L^n(\Omega)$ (or even in $C(\partial \Omega)\times L^p(\Omega)$). We now use
(4.11)
to show that $u$ assumes the boundary values $\psi$ in an equicontinuous
manner. 
In this regard, let
$f_M=\max(\min(f,M),-M)$ be the standard truncation of
$f$ for
$M>0$.  We note that for $f\in B_R$
$$\|f-f_M\|_{L^p(\Omega)}\le \left({\rm measure}(\{|f|>M\})\right)^{{n-p\over
np}}R\le R\left({R\over M}\right)^{{n-p\over p }},$$
which tends to 0 as $M\rightarrow \infty$ uniformly in $f\in B_R$.
Using the properties  (4.8), (4.7) of $U$   we  thus have
$$\eqalign{U(\psi,f)\le U(\psi,f_M)+U(0,f-f_M)&\le U(\psi,M)+C\|f-
f_M\|_{L^p(\Omega)}\cr
&\qquad\le U(\psi,M)+CR\left({R\over M}\right)^{{n-p\over p }}.}$$
According to Proposition 3.2, $U(\psi, M)$ assumes the boundary values $\psi$
in a  manner controlled by the modulus of continuity of $\psi$ for fixed $M$.  The
``error term" on the right above can be made as small as desired by choosing
$M$ sufficiently large, and $u\le U(\psi,f)$ thus guarantees an estimate 
$u(x)-\psi(y)\le \rho(|x-y|)$ for $x\in\overline \Omega, y\in \partial \Omega$, where $\rho(0+)=0$.
Similarly,
$-U(-\psi,f)\le u$ provides control of $u-\psi$ at the boundary from below. 
 
Finally,  once
$u$ is bounded, (4.6) guarantees equi-H\"older continuity of $u$ on
compact subsets of $\Omega$ so long as $f$ remains bounded in $L^n(\Omega)$ 
(see, for example, [13] for a sufficiently general statement and Remark 
4.7  below). The result follows.}

\remark{4.3}{ Proposition 4.2\ can be reformulated by saying that
if $u$ satisfies (4.6) and $u=\psi$ on $\partial \Omega$ then $u$ has a modulus
of continuity on $\overline\Omega$ that only depends on the parameters 
of the cone 
condition, $\lambda,\Lambda,n,\gamma$, ${\rm
diam}\,(\Omega)$, $R$ and the modulus of continuity of $\psi$.}

\remark{4.4}{The inequality (4.7) generalizes 
the original work of Fabes and Stroock
[12] and is proved in [13] in the spirit of this
work, but
it could also be deduced from Cabr\'e [1];
its relevance in this arena was first shown by Escauriaza [11]. In fact,
the
existence of $U(\varphi,g)$ for $\gamma=0$ was proved in [11] relying on (4.7)
with
$\gamma=0$. The properties
(4.8) are a consequence of the positive homogeneity and superlinearity of
$(p,X)\rightarrow {\cal P}^-(X)-\gamma|p|$ and (4.7) ($p=n$ suffices). For example, the
superadditivity implies that $W=U(\varphi,g)-U(\hat\varphi,\hat g)$ solves
$${\cal P}^-(D^2 W )-\gamma|DW|\le g-\hat g\le 0$$  if $g\le\hat g$ and an application of (4.7)
($p=n$ suffices) then proves the order preserving property.   The relation
(4.10)
given (4.9) follows upon observing that $v=u-U(\psi,f)$ is an $L^n$-viscosity  solution of
${\cal P}^-(D^2 v)-\gamma|Dv|\le 0$ and the 
Alexandrov-Bakelman-Pucci maximum principle for viscosity
solutions
proved in  [2] ($\gamma=0$), [30], [4].  
Finally, Proposition 4.2\ itself appears in
[3],
Theorem 4.14, in the situation where $\gamma=0$, $\Omega$ is a ball, and all functions $f$
appearing  in
(4.6) are continuous. This proof could be adapted, with effort, to the
current
case. The current proof uses the work already done in Section 3.}

\proofof{Theorem 4.1}{First we assume that $F(x,r,p,X)$ is defined for
all
$(r,p,X)$ for all $x\in{\Bbb R}^n$ and satisfies the structure conditions
(1.2), (1.3) and (4.1) for  all $x\in{\Bbb R}^n$.  To
achieve this, if necessary extend
$F(x,r,p,X)$ to be ${\cal P}^-(X)-\gamma|p|$ (or ${\cal P}^+(X)+\gamma|p|$) for those
$x$'s where it was not originally defined. Now mollify $F$ in $x$:
$$F_\epsilon(x,r,p,X)={1\over\epsilon^n}
\int_{{\Bbb R}^n}\eta\left({x-y\over\epsilon}\right)F(y,r,p,X)\,dy, $$ where $\eta\in
C_0^\infty({\Bbb R}^n)$ satisfies $\eta\ge 0$ and
$\int_{{\Bbb R}^n}\eta(x)\,dx=1$. The structure conditions are preserved
under this sort of averaging, so $F_\epsilon\in{\cal SC}$.

Clearly $F_\epsilon$ satisfies (4.1), (4.4) and (4.5) as well as $F$.
  Moreover, the bound (4.5) on $|F|$ gives us
$$|F_\epsilon(x,r,p,X) -F_\epsilon(y,r,p,X)|
\le \frac C\epsilon|x-y|\left(\Lambda\|X\|+\gamma|p|+\beta(r)\right)
$$
for some $C$.
Fix $f\in L^n(\Omega)$ and let $f_j\in C(\overline \Omega)$ satisfy
$$\|f_j-f\|_{L^n(\Omega)}\rightarrow 0\text{as}j\rightarrow \infty.$$
Since $F_\epsilon\in{\cal SC}$ is continuous, according to Theorem 1.1\  the problem
$$F_\epsilon(x,u,Du,D^2u)=f_j\text{in}\Omega\text{and} u=\psi\text{on}\partial \Omega\eq$$
has a $C$-viscosity solution (and hence $L^n$-viscosity solution) $u=u_{\epsilon,j}$. Clearly
$u=u_{\epsilon,j}$ also solves
$${\cal P}^-(D^2u)-\gamma|Du|+F_\epsilon(x,u,0,0)\le f_j\text{and}f_j\le
{\cal P}^+(D^2u)+\gamma|Du|+F_\epsilon(x,u,0,0).
$$ Since $F_\epsilon(x,u,0,0)\ge F_\epsilon(x,0,0,0)=0$ if $u\ge 0$, the first
relation
above and the  maximum principle for
viscosity solutions   implies
$$u\le
\sup_{\partial \Omega}u^++C\|f_j\|_{L^n(\Omega)}\le\sup_{\partial \Omega}\psi^+
+C\sup_j\|f_j\|_{L^n(\Omega )}
$$ and we conclude that the $u_{\epsilon,j}$ are bounded above independently
of $\epsilon, j$. Likewise, the $u_{\epsilon,j}$ are bounded below independently
of $\epsilon, j$, and hence the family is uniformly bounded. Using this
information and (4.5) for $F_\epsilon$, there exists a constant $K$ such that
$|F_\epsilon(x,u_{\epsilon,j},0,0)|\le K$ and the
$u_{\epsilon,j}$ satisfy
$${\cal P}^-(D^2u_{\epsilon,j})-\gamma|Du_{\epsilon,j}|\le g_j\text{and}-g_j\le
{\cal P}^+(D^2u_{\epsilon,j})+\gamma|Du_{\epsilon,j}|,$$ where $g_j=|f_j|+K$.  

Therefore, using Proposition 4.2,  there exists $\epsilon_m\downarrow 0$,
$j_m\rightarrow\infty$ such that $u_m=u_{\epsilon_m,j_m}$ converges
uniformly on $\overline \Omega$ to a limit $u$. By Theorem 3.8 of [4] this
$u$ is an $L^n$-viscosity solution of (4.3); indeed, what we need to check to
use this result is only that for $\varphi\in W^{2,n}_{\rm loc}(\Omega)$ we have
$$F_{\epsilon_m}(x,u_m(x),D\varphi(x),D^2\varphi(x)) \rightarrow
F(x,u(x),D\varphi(x),D^2\varphi(x))\eq$$ in $L^n_{\rm loc}(\Omega)$. However,
$F_\epsilon(x,r,p,X)\rightarrow F(x,r,p,X)$ whenever $x$ is a Lebesgue point of
$F(\cdot,r,p,X)$, and almost every $x$ has this property for all
$r,p,X$ by
$F\in{\cal SC}$ (see [4], page 382), which together with (4.5)
shows that (4.13)  holds pointwise a.e. and (locally) dominated, hence in
$L^n_{\rm loc}(\Omega)$.}

We now turn to the parabolic analogue of Theorem 4.1. In this
case the initial boundary value problem can be rewritten as before
as
$$u_t+F(x,t,u,Du,D^2u)=f(x,t)\text{in}Q=\Omega\times (0,T],\quad
u=\psi\text{on}
\partial_pQ,\eq  $$ where 
$$F(x,t,0,0,0)\equiv 0.\eq$$ The proof of the
theorem below is similar to the one in the elliptic case and is
therefore omitted, save for the remarks to follow. 


\theorem{4.5}{Let $F\in{\cal SC}$ satisfy (4.1) and (4.15), let $f\in
L^{n+1}(Q)$, $\psi\in C(\partial_pQ)$ and let $\Omega$ satisfy a uniform exterior cone
condition.  Then (4.14) has an $L^{n+1}$-viscosity solution.} 

The  parabolic
version of the compactness result Proposition 4.2\ is
\proposition{4.6}{Let $\Omega$ satisfy a uniform exterior cone
condition and ${\cal C}\subset C(\partial_pQ)$ be compact, $R>0$ and 
$B_R=\{f\in L^{n+1}(Q)\colon\ \|f\|_{L^{n+1}(Q)}\le R\}$.   Then the set of all functions $u\in
C(\overline Q)$
such that there exists
$ \psi \in{\cal C}$ and $f\in B_R$ for which $u$ is an $L^{n+1}$-viscosity solution
of both
$$u_t+{\cal P}^-(D^2u)-\gamma|Du|\le f\text{\it and} -f\le u_t+{\cal P}^+(D^2u)+\gamma|Du| \eq$$
in $Q$ and $u=\psi$ on $\partial_pQ$ is
precompact in $C(\overline Q)$. }

A version of the maximum principle and an existence result sufficient for
the proof of this proposition is  given in [7].  The interior H\"older
continuity is established in [10], Section 5. The limit theorem needed to complete
the proof of Theorem 4.5\ is proved in [10], Section 6.   

\remark{4.7}{ The proofs of the existence results above do not require
full Propositions 4.2\ and 4.6\ but rather their versions
with $B_R$ replaced by $B_R\cap C(\Omega)$ (or $B_R\cap C(Q)$). In this
case, the proofs of the versions of the maximum principles and equi-H\"older
continuity results found in Caffarelli [2], Trudinger [30]  (elliptic case),
and Wang [32] (parabolic case) could be used. This leaves aside (4.7), upon
which we have commented. The parabolic analogue is proved in [7]. The proofs of
the various maximum principles sketched in [7] might interest the reader in
any case.}

\remark{4.8}{ We note again, for emphasis, that Theorems 4.1\ and
4.5\ are also true  if $n$ and $n+1$ are replaced by $p$ in (parameter
dependent) appropriate ranges of the form $n-\delta < p $ and $n+1-\delta <p $
respectively.  To  document  this fully in the elliptic case  requires results 
from [4],  [28]  while [10] contains the parabolic story.}

\noindent {\bf Acknowledgments.}\quad Crandall was supported by NSF grant
DMS93-02995 and by an appointment as a Miller Research Professor at the University of 
California, Berkeley. Kocan was supported  by the
Australian Research Council and an Alexander von Humboldt Fellowhip.
Lions was supported by URA CNRS
749 and NSF grant DMS93-02995. \Swiech\ was supported by NSF grants
DMS97-06760, DMS93-02995.



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\bigskip


\noindent M.~G. Crandall \hfill\break
Department of Mathematics, University of California, Santa Barbara \hfill\break
Santa Barbara, CA 93106, USA \hfill\break
E-mail address: crandall@math.ucsb.edu 


\noindent M. Kocan \hfill\break
Mathematics Institute, University of Cologne \hfill\break
50923 Cologne, Germany \hfill\break
E-mail address: mkocan@mi.uni-koeln.de 

\noindent P.~L. Lions \hfill\break
Ceremade,  Universit\'e Paris-Dauphine   \hfill\break
Place de Lattre de Tassigny, 75775 \hfill\break
Paris 16, France  


\noindent A. \Swiech  \hfill\break
School of Mathematics, Georgia Institute of Technology  \hfill\break
Atlanta, GA 30332, USA \hfill\break
E-mail address: swiech@math.gatech.edu


\bye
