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\headline={\ifnum\pageno=1 \hfill\else%
{\tenrm\ifodd\pageno\rightheadline \else
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\def\rightheadline{EJDE--1995/02\hfil Quasilinear Integro-differential
Equations \hfil\folio}
\def\leftheadline{\folio\hfil Hans Engler
 \hfil EJDE--1995/02}

\def\pretitle{\vbox{\eightrm\noindent\baselineskip 9pt %
 Electronic Journal of Differential Equations\hfil\break
Vol. {\eightbf 1995}(1995), No. 02, pp. 1-16. Published February 24, 1995.
\hfil\break
ISSN 1072-6691. URL: http://ejde.math.swt.edu or http://ejde.math.unt.edu
\hfil\break ftp (login: ftp) 147.26.103.110 or 129.120.3.113 
\bigskip} }


\topmatter
\title
Strong Solutions of Quasilinear Integro-differential Equations
with Singular Kernels in Several Space Dimensions
\endtitle

\thanks \noindent
{\it 1991 Mathematics Subject Classifications:} 45K05.\hfil\break
{\it Key words and phrases:} Integro-differential equation, 
strong solution, singular kernel, quasilinear
\hfil\break
\copyright 1995 Southwest Texas State University  and
University of North Texas.\hfil\break
Submitted: December 15, 1994.\hfil\break
Supported by the National Science Foundation under grant \# DMS - 9003543
\endthanks
\author  Hans Engler  \endauthor
\address 
 Department of Mathematics \newline\indent
 Georgetown University \newline\indent
Washington, D.C. 20057
\endaddress
\email engler\@guvax.acc.georgetown.edu
\endemail
\abstract
For quasilinear integro-differential equations of the form
$ u_t - a*A(u) = f$, where $a$ is a scalar singular integral kernel that
behaves like $t^{-\alpha}$, $\frac{1}{2} \le \alpha < 1$ and $A$ is a 
second order quasilinear elliptic operator in divergence form, 
solutions are found for which $A(u)$ is integrable over space and time.  
\endabstract
\endtopmatter

\document
\head
1. Introduction
\endhead
The purpose of this note is a study of quasilinear integro-differential
equations of the form
$$
\frac{\partial}{\partial t} u(x,t) - 
\int_0^t a(t-s)\, \text{div}\, \tilde g(\nabla u(x,s)) 
 \, ds = f(x,t) \tag 1.1
$$
in cylindrical domains $\Omega \times [0,T] \subset \Bbb R^{N+1}$,
together with zero boundary data for $u$ on $\partial \Omega \times [0,T]$ and
initial data on $\Omega \times \{ 0\}$. Here $a(\cdot)$ is a scalar integral
kernel that behaves like $t^{-\alpha}, \, 0 < \alpha < 1$ for $t$ near zero.
The equation occurs in the description of simple shear motions ($N = 1$)
and of antiplane shear ($N = 2$) of certain idealized viscoelastic materials
(\cite{14}), and ``power law'' kernels $a(t) = t^{-\alpha}$ have been
proposed elsewhere for such models (\cite{13}). We are interested in large 
time solutions without restrictions on the size of the data.

 
Recently, for $\Omega = [0,1] \subset 
\Bbb R$, ``strong solutions'' with $u_{xx}^2$ integrable over
$\Omega \times [0,T]$ have been found under two different sets of assumptions,
namely when $\alpha \ge \frac{1}{2}$ and $0 < c \le \tilde g'(r) \le c' <
\infty$ (\cite{9}) and when the Laplace transform $\hat a$ maps the right 
half plane into a sector in the right half plane, under a restriction
for $\frac{c}{c'}$ that depends on the angle of aperture of this sector 
(\cite{8}). Also, weaker solutions with only $u^2_x$ integrable
can be found without restrictions for $\alpha, \, c, \, c'$ (\cite{11}),
and smooth solutions (as smooth as the data permit) can be found if
$\frac{2}{3} < \alpha < 1$ and only $ 0 < \tilde g'(r) \le C < \infty$
(\cite{3}). In other work, large time solutions for small smooth data
have been constructed, weak solutions for
more regular kernels have been found, and
the break-down of smooth solutions for regular kernels has been established;
see the references in \cite{8} and \cite{9}.

 
We want to extend the results of \cite{9} in several ways, namely by 
treating also higher space dimensions and by allowing also nonlinear
terms $\tilde g$ that grow polynomially in their arguments, corresponding
to ``shear-thickening'' behavior for viscoelastic materials. 
The function $\tilde g : \Bbb R^N  
\, \to \, \Bbb R^N$ will be assumed to be ``isotropic'', i.e. to have the 
form $\tilde g(\xi) = g(|\xi|^2)\xi$. We also use a slightly different class 
of integral kernels and modified assumptions for the data. The main restriction,
namely $\frac{1}{2} \le \alpha < 1$, however is not weakened in the present paper. 
We also give
linear examples that show that more must be assumed for the data of the
problem if strong solutions are to be found for smaller values of $\alpha$.

 
Throughout, $\Omega \subset \Bbb R^N$ is a bounded domain with a 
$C^2$ - smooth boundary $\partial \Omega$, with exterior unit normal
vector field $\nu: \partial \Omega \, \to \, S^{N-1}$.
Subscripts $,i$ denote partial differentiation with respect to 
$x_i, \, 1 \le i \le N$, and a subscript $t$ is used to denote partial 
differentiation with respect to $t$.
We shall use the common symbols $\nabla$ for the gradient of a scalar
function and for the derivative matrix of a vector field and the symbol
$\text{div} \, $ for the divergence of a vector field: If $\phi = 
(\phi_i)_{1 \le i \le M}$ and $\psi = (\psi_i)_{1 \le i \le N}$ are
vector fields, then
$$
\nabla \phi = (\phi_{i,j}) \Sb 1 \le i \le M \\ 1 \le j \le N \endSb \, ,
\quad 
\text{div} \,  \psi = \sum_i \psi_{i,i} \, . 
$$
Also, $\Delta u = \text{dvi}\,  \nabla u$ is the Laplacian of a scalar 
function $u$, and $\nabla^2 u$ is its Hessian  matrix.

 
The common notation for 
Sobolev spaces will be employed, and we write $H^k$ for $W^{k,2}$ and 
$H^k_0$ for $W^{k,2}_0$.  We also use spaces of vector-valued $H^s([0,T],V)$, 
for non-integer  $s = k+ \gamma> 0, \, 0 < \gamma < 1$,
with a separable Hilbert space $V$.   Such spaces can be defined
as complex interpolation spaces between $H^k([0,T],V)$ and
$H^{k+1}([0,T],V)$ and  can alternatively be characterized by the
conditions that $v \in H^s([0,T],V)$ if and only if $v^{(k)} \in L^2(0,T;V)$ 
and 
$$
\int_0^T \, \int_0^T \dfrac{\|v^{(k)}(t) - v^{(k)}(\tau) \|_V^2}
{|t - \tau|^{1 + 2 \gamma}} \, d \tau \, d t < \infty \,, 
$$
see \cite{1}. The norms of $\L^2(\Omega, \Bbb R)$ and 
$L^2(\Omega, \Bbb R^N)$ are denoted by $\| \cdot \|$, and the scalar
products on these spaces are denoted by $\langle \cdot, \cdot \rangle$.
Other norms on function spaces are identified by subscripts. Euclidean norms 
of vectors and matrices  are denoted by $|\cdot|$. 

 
The convolution of two functions $u, \, v$
that are supported on the positive half axis is written as  $u*v(t) = 
\int_0^tu(t-s)v(s) \, ds$. The letter $C$ is used for constants whose 
values may be different in each occurrence and which can in principle be 
estimated explicitly in terms of known quantities.

 

\head
2. Main Result
\endhead

Consider the quasilinear integro-differential equation
$$
u_t(x,t) - \int_0^t a(t-s)\, \text{div} \left(g(|\nabla u(x,s)|^2) 
\nabla u(x,s)\right) \, ds = f(x,t) \tag 2.1
$$
in $\Omega \times [0,T]$, with initial and boundary data
$$
u(\cdot ,0) = u_0, \quad u_{\big| \partial \Omega \times [0,T]} = 0 \, .
\tag 2.2
$$
The kernel $a:[0,T] \to \Bbb R$ is assumed to be 
of the form
$$
a(t) = a_\alpha(t) + c*a_\alpha(t) \tag 2.3
$$
with
$$
a_\alpha(t) = \frac{t^{-\alpha}}{\Gamma(1-\alpha)} \,, \quad c \in W^{1,1}([0,T];\Bbb R) 
\tag 2.4
$$ 
and 
$$
\frac{1}{2} < \alpha < 1\, .  \tag 2.5
$$
The case $\alpha = \frac{1}{2}$ will be discussed in section 3.
We assume that the function $g: [0,\infty) \to \Bbb R$ is continuously
differentiable and satisfies
$$
g(r) + (2 + \epsilon) rg'(r) \ge \epsilon > 0, \quad rg'(r) \le \beta
g(r) \tag 2.6
$$
for some $\epsilon, \, \beta$, for all  $r \ge 0$. Note that (2.6) implies 
that
$$
\epsilon \le g(r) \le g(1)r^\beta \tag 2.7
$$
for all $r \ge 1$. We define
$$
G(r) = \frac{1}{2} \int_0^r g(s) \, ds  \, ;\tag 2.8
$$
then  the function $r \to G(r^2)$ is strictly convex on $\Bbb R$
by (2.6). For the data, we assume that
$$
\align
&\| f(\cdot,0)\| + \int_0^T \| f_t(\cdot,t)\| \, dt < \infty \\
&\int_\Omega G(|\nabla u_0(x)|^2)  < \infty \\
&\int_{\Omega} | \nabla (g(|\nabla u_0|^2) \nabla u_0)|^2  < \infty\, .  
\tag 2.9
\endalign
$$
The main result of this note is the following.

 
\proclaim{Theorem 1}
Under these assumptions, there exists a function $u$ in 
$$W^{1,\infty}([0,T],L^2(\Omega)) \cap L^2(0,T;H^2(\Omega)) \cap
H^{\frac{1+\alpha}{2}}([0,T],H^1_0(\Omega))$$
 that satisfies (2.1)
in the sense of distributions and for which $\lim_{t \to 0} u(\cdot ,t) =
u_0$ in $H^1(\Omega)$. Moreover, for some $q > 1$, $\nabla \left(
g(|\nabla u|^2) \nabla  u\right) \in L^q(\Omega \times [0,T])$, and thus
(2.1) holds in this space.

\endproclaim

 

\demo{Proof}
We construct Galerkin approximations, establish  suitable
\sl a priori \rm estimates,  and pass to the limit. This will yield 
a solution in the desired solution class. Thus let
$$
\{ \varphi_i \, \big| \, i \ge 1 \, \} \subset L^2(\Omega)
$$
be a complete orthonormal system in $L^2(\Omega)$ of eigenfunctions of the
negative Laplacian with zero boundary data. These functions are known to be
in $W^{2,p}(\Omega) \cap C^\infty(\Omega)$ for all $p <\infty$. Let 
$V_n = span( \varphi_1, \dots, \varphi_n)$ for $n = 1,\, 2, \, 3, \dots$. For
technical reasons, we shall construct solutions on $\Omega \times [0, T+1]$.
Thus let ${T'} = T+1$; we can extend $f$ and $a$ 
such that all their properties still hold on the larger interval. Let $f^n$
be a sequence in $C^1([0,{T'}],L^2(\Omega))$ that converges to $f$ in
$W^{1,1}[0,{T'}],L^2(\Omega))$, and let $u^n \in C^1([0,t_n),V_n)$ be the unique
maximal solution of the system
$$
\langle u^n_t, v \rangle + \langle a*g(|\nabla u^n|^2) \nabla u^n,
\nabla v\rangle = \langle f^n, v\rangle \tag 2.10
$$
for all $v \in V_n$, with initial data defined by
$$
\langle u^n(0) - u_0 , v \rangle = 0
$$
for all $v \in V_n$. 
It follows from standard results on functional differential equations 
(\cite{10}) that
$u^n$ exists and is unique for each $n$; possibly, $t_n < {T'}$, in which case
$$
\| u^n(t) \| \, \to \, \infty \quad \text{as} \quad t \,  \to  \,
t_n \, .
$$
It is also easy to see (by differentiating the equation) that in fact 
$u^n \in C^2((0,t_n),V_n)$. 

 
{\it
A Priori Estimate I.}
Let $d \in W^{1,1}([0,{T'}],\Bbb R)$ be the resolvent kernel of $c$ 
(\cite{7}), i.e. the function satisfying
$$
c + d + c*d = 0 \, . \tag 2.11
$$
We use the notation
$$
g^n(t) = g(|\nabla u^n(\cdot ,t)|^2)\nabla u^n(\cdot ,t) \, , 
\quad g^n(0) = g^n_0 \, . \tag 2.12
$$
Then (2.10) is equivalent to 
$$
\langle u^n_t + d*u^n_t, v \rangle + \langle a_\alpha * g^n,
\nabla v \rangle = \langle f^n + d*f^n,v\rangle  \tag 2.13
$$
for all $v \in V_n$. We differentiate with respect to $t$; after some
manipulations, the result is the equation
$$
\gathered
\langle u^n_{tt} + d(0) u^n_t + d'*u^n_t, v \rangle  +
\langle a_\alpha (g^n - g^n_0) , \nabla v \rangle  \\
 \quad  + \langle \int_{0}^t (-a_\alpha'(t-s))(g^n(t) - g^n(s))\, ds , 
\nabla v\rangle 
= \langle F^n(\cdot ,t), v\rangle  \, , \endgathered\tag 2.14
$$
where
$$
F^n(\cdot ,t) = f_t^n(\cdot ,t) + d(0)f^n(\cdot ,t) + d'*f^n(\cdot ,t)
- a_\alpha(t) \text{dvi}\,  g^n_0 \, .
$$
Note that the integral involving $a_\alpha'$ is defined for all $t$,
since $|g^n(t) - g^n(s)| = O(|t-s|)$, due to the differentiability of $u^n$.
We now use the $t$-dependent test function $v = u^n_t(\cdot ,t) \in V_n$. The
result is the identity
$$
\gathered
\frac{1}{2} \frac{d}{dt} \|u^n_t(\cdot ,t) \|^2 + 
d(0) \|u^n_t(\cdot ,t)\|^2 
+ \langle d'*u^n_t(\cdot ,t), \, u^n_t(\cdot ,t) \rangle \\
+ a_\alpha(t) \langle g^n(t) - g^n_0, \nabla u^n_t(\cdot ,t)
\rangle 
 + \int_{0}^t (-a_\alpha'(t-s)) \langle g^n(t) - g^n(s), \nabla u^n_t(\cdot ,t)
\rangle \, ds \\
 = \langle F^n(\cdot ,t), \, u^n_t(\cdot ,t) \rangle \, .
\endgathered \tag 2.15
$$
Now 
$$
\langle g^n(t) - g^n(s), \nabla u^n_t(\cdot ,t)\rangle  =
\frac{d}{dt} \Phi^n (t,s) \tag 2.16
$$
where
$$ \aligned
\Phi^n(t,s) &= \int_\Omega H(\nabla u^n(\cdot,t), \nabla u^n(\cdot,s)) \, , 
\\ H(\xi, \zeta) &= G(|\xi|^2) - G(|\zeta|^2)  
- (\xi - \zeta)^T g(|\zeta|^2) \zeta \, .\endaligned
\tag 2.17
$$
Thus
$$
\gathered
\int_{0}^t (-a_\alpha'(t-s)) \langle g^n(t) - g^n(s), \nabla u^n_t(\cdot ,t)
\rangle \, ds \\
 = \frac{d}{dt} \int_{0}^t (-a_\alpha'(t-s)) \Phi^n(t,s) \, ds
+ \int_{0}^t a_\alpha''(t-s) \Phi^n(t,s) \, ds
\endgathered \tag 2.18
$$
and
$$
a_\alpha(t) \langle g^n(t) - g^n_0, \nabla u^n_t(\cdot ,t)
\rangle = \frac{d}{dt} \left( a_\alpha(t) \Phi^n(t,0) \right) -
a_\alpha'(t) \Phi^n(t,0) \, . \tag 2.19
$$
Note that $|\Phi^n(t,s)| = O(|t-s|^2)$; thus the integral
involving $a_\alpha''(t) = \frac{t^{-\alpha-2}}{\Gamma(-\alpha-1)} $ converges.
We insert these formulae into (2.15) and integrate with respect to $t$.
After a trivial estimate, the result is
$$
\gathered
\frac{1}{2} \| u^n_t(\cdot ,t)\|^2  - \frac{1}{2} \|u^n_t(\cdot ,0) \|^2
 + \int_{0}^t (-a_\alpha'(t-s))
\Phi^n(t,s) \, ds   + a_\alpha(t) \Phi^n(t,0) \\
\quad  + \int_{0}^t \big( \int_{0}^s a_\alpha''(s- \tau) 
\Phi^n(s, \tau) \, d \tau 
-a_\alpha'(s) \Phi^n(s,0) \big) \, ds \\
\leq  \int_{0}^t \big(
(\|F^n(\cdot ,s)\| + \|d'*u^n_t(\cdot ,s)\| 
+ |d(0)|\|u^n_t(\cdot ,s)\|)
\|u^n_t(\cdot ,s)\| \big) \, ds \, .
\endgathered \tag 2.20
$$
Next we note that for any $\xi, \zeta \in \Bbb R^n$
$$
H(\xi, \zeta) = \int_{0}^1 (1-s) (\xi - \zeta)^T 
K(\zeta + s(\xi- \zeta))(\xi - \zeta) \, ds
$$
where
$$
K(\lambda) = g(|\lambda|^2) \bold I + 2g'(|\lambda|^2) \lambda \lambda^T $$
is the derivative matrix of the function $\lambda \, \to \, g(|\lambda|^2)
\lambda$. By assumption (2.6),
$$
\mu^T K(\lambda) \mu \ge \epsilon |\mu|^2
$$
for all $\mu \in \Bbb R^n$, and thus for all $\xi, \zeta$
$$
H(\xi,\zeta) \geq \frac{\epsilon}{2} |\xi - \zeta|^2  \, . \tag 2.21
$$
In particular, 
$$
\Phi^n(t,s) \geq \frac{\epsilon}{2}\|\nabla u^n(\cdot ,t) - 
\nabla u^n(\cdot ,s)\|^2 \geq  0  \tag 2.22
$$
for all $0 \le s,t \le {T'}$.
Dropping now first all terms involving $\Phi^n$ on the left hand side 
of (2.20) and applying Gronwall's inequality shows that
$$
\sup_{0 \le t \le t_n} \|u^n_t(\cdot ,t)\| \le C \tag 2.23
$$
for some constant $C$ that does not depend on $n$.  Consequently, $t_n = {T'}$
for all $n$. 
Next we return to (2.20) and infer that also
$$
\gathered
\sup_{0 \le t \le {T'}} \left( \int_{0}^t (-a_\alpha'(t-s))
\Phi^n(t,s) \, ds  +  a_\alpha(t) \Phi^n(t,0) \right) \le C
\, , \\ 
 \int_{0}^{T'} \left( \int_{0}^s a_\alpha''(s-\tau) \Phi^n(s, \tau) \, d \tau
+ (-a_\alpha'(s)) \Phi^n(s,0) \right) \, ds  \le C \endgathered\tag 2.24
$$
and therefore in particular 
$$
\int_{0}^{T'}  \int_{0}^s (s-\tau)^{-\alpha-2}
\|\nabla u^n(\cdot ,s) - \nabla u^n(\cdot ,\tau) \|^2 \, d \tau
\, ds + \sup_{0 \le t \le {T'}} \, \| \nabla u^n(\cdot,t)\|\le C \, .
 \tag 2.25
$$
The first estimate in (2.25) is equivalent to an {\sl a priori} estimate
in $H^{\frac{1+\alpha}{2}}([0,{T'}], H^1(\Omega))$ for the approximate solutions
$u^n$.  
Finally, from (2.25), (2.24), and (2.9) we deduce that
$$
\sup_{0 \le t \le {T'}} \int_{\Omega} G(|\nabla u^n(\cdot ,t)|^2) \le C \, . 
\tag 2.26
$$

 
{\it A Priori Estimate II.}
 As in (2.11), let $d$ be the resolvent kernel
of $c$, and set
$$
b = b_\alpha + d*b_\alpha \quad \text{with} \quad b_\alpha (t) = 
\frac{t^{\alpha-1}}{\Gamma(\alpha)} \, .
$$
Then $a_\alpha * b_\alpha(t) = 1$ and therefore also $a*b(t) = 1$ for all $t > 0$.
We form the convolution of (2.10) with $b$ and differentiate with respect to $t$. 
The result is the identity
$$
\frac{d}{dt} \langle b*u^n_t(\cdot ,t),v\rangle  + 
\langle g^n(t),\nabla v\rangle  = \langle b(t)f^n(\cdot ,0) + b*f^n_t(\cdot ,t),
v\rangle  \tag 2.27
$$
for all $v \in V_n$. We now use the test function $v = (t-{T'}) \Delta u^n(\cdot ,t)
\in V_n$ (recall that $\Delta $ maps $V_n$ into itself) and integrate from 
0 to ${T'}$. After some integrations by parts, we obtain
$$
\gather
\int_{0}^{T'} \langle b*\nabla u^n_t(\cdot ,t),(t-{T'})\nabla u^n_t(\cdot ,t)+
\nabla u^n(\cdot ,t) \rangle  \, dt + \int_{0}^{T'} (t-{T'}) 
\langle  g^n(t), \nabla \Delta u^n(\cdot ,t) \rangle  \, dt \\
= \int_0^{T'} \langle b(t) f^n(\cdot,0) + b*f^n_t(\cdot,t), (t-{T'}) 
\Delta u^n(\cdot,t) \rangle \, dt \, .
\tag 2.28 \endgather
$$
The absolute value of the integral on the right hand side of this identity can be 
estimated from above by 
$$
\gather
\int_{0}^{T'} \left( |b(t)|\|f^n(\cdot ,0)\| + \|b*f^n_t(\cdot ,t)\| \right)
({T'}-t)\|\Delta u^n(\cdot ,t)\| \, dt  \tag 2.29 \\
 \quad \le C(\epsilon,{T'}) \|b\|_{L^2(0,{T'})} \big( \|f^n(\cdot ,0)\|^2 
+ \|f^n_t\|^2_{L^1(0,{T'};L^2)}\big)  
+ \epsilon \int_{0}^{T'}({T'}-t)\|\Delta u^n(\cdot ,t)\|^2 \, dt 
\endgather
$$
for any $\epsilon >0$, since $b \in L^2(0,{T'})$, due to the restriction
$\alpha > \frac{1}{2}$. To estimate the first integral on the left hand side
of (2.28) in absolute value, we define
$$
e_\alpha(t) = \frac{t^{\alpha/2 - 1}}{\Gamma(\frac{\alpha}{2})}
$$
such that $e_\alpha*e_\alpha = b_\alpha$ and thus $b = e_\alpha*e_\alpha
+ d*e_\alpha*e_\alpha$. Then the integral can be rewritten as
$$
\dots = \int_{0}^{T'} \langle  (e_\alpha + d*e_\alpha)* \nabla u^n(\cdot ,t),
\int_{t}^{T'} e_\alpha(\tau - t) \left( (\tau-{T'})
\nabla u^n(\cdot ,\tau) + \nabla u^n(\cdot ,\tau) \right) \rangle d \tau 
\, dt \, .
$$
Now 
$$
\left( e_\alpha + d*e_\alpha\right)*\nabla u^n_t(\cdot ,t) =
\frac{d}{dt}  (e_\alpha + d*e_\alpha)* w^n (\cdot, t)
 \tag 2.30
$$
with $w^n(\cdot, t) = \nabla u^n(\cdot ,t) - \nabla u^n(\cdot ,0)$, 
and since $\nabla u^n \in H^{\frac{1+\alpha}{2}}([0,{T'}],L^2(\Omega))$ due
to (2.25), with an estimate in this space that does not depend on $n$, 
it follows that $ (e_\alpha + d*e_\alpha)* w^n (\cdot, t)$ is in 
$H^{\alpha + \frac{1}{2}}([0,{T'}], L^2(\Omega))$. Its derivative is therefore
in 
$H^{\alpha - \frac{1}{2}}([0,{T'}],L^2(\Omega))$, with an 
estimate that does not depend on $n$ (\cite{6}). Similarly,
$$
\align
& \int_{t}^{T'} e_\alpha(\tau - t) \left( (\tau-{T'}) \nabla u^n_t(\cdot ,\tau) 
+ \nabla u^n(\cdot ,\tau) \right) \, d \tau \\
 &= \frac{d}{dt} \left( \int_{0}^{{T'}-t} e_\alpha(\sigma)((t-{T'}+\sigma) 
\nabla u^n(\cdot ,t+\sigma)) \, d \sigma \right)   \tag 2.31 \\
& = \frac{d}{dt} \left((t-{T'}) \int_{0}^{{T'}-t} e_\alpha(\sigma) 
\nabla u^n(\cdot ,t+\sigma) \, d \sigma \right)   + 
\frac{d}{dt} \int_{0}^{{T'}-t} \sigma e_\alpha(\sigma) \nabla u^n(\cdot ,t+\sigma)
\, d \sigma \, .
\endalign 
$$
As above, both integrals are in 
$H^{\alpha + \frac{1}{2}}([0,{T'}], L^2(\Omega))$ as function of $t$, and the 
entire expression is therefore bounded \sl a priori \rm 
in $H^{\alpha - \frac{1}{2}}([0,{T'}],L^2(\Omega))$. The first 
integral on the left hand side of (2.28) can now be bounded 
independently of $n$. 

 
Finally consider the second integral on the left hand side of (2.28). Fix $t$ 
and set $w = u^n(\cdot ,t)$, then we want to estimate
$$\int_\Omega g(|\nabla w|^2)\nabla w \cdot \nabla(\Delta w) =
\int_\Omega \sum_{i,j} g(|\nabla w|^2) w_{,i} w_{,i,j,j} \, .
$$
The following arguments are taken from \cite{2}, where more details can be
found. After an integration by parts, the integral equals 
$$ 
-\int_{\Omega} \sum_{i,j} w_{,i,j} (g(|\nabla w|^2)w_{,i})_{,j} +
\int_{\partial \Omega}  \sum_{i,j} g(|\nabla w|^2)w_{,i} w_{,i,j} \nu_j \, .
\tag 2.32
$$
Since the function $w$ vanishes on the hypersurface $\partial \Omega$, its 
gradient is perpendicular to it and therefore parallel to the unit normal
$\nu$, i.e. $\nabla w = \nu \, \partial_\nu w$, where
$\partial_\nu w =  \nabla w \cdot \nu$. Also, at any point of this
hypersurface, $\Delta w = \Delta_{\partial \Omega} w 
 + (N-1)\bold H \partial_\nu w + \partial^2_\nu w$, where
$\Delta_{\partial \Omega}$ is the induced Laplacian,
$\bold H$ is the mean curvature of $\partial \Omega$ with respect to $\nu$
and $\partial_\nu^2 u = \nu^T \nabla^2 w \nu$ (\cite{15}). Since $w$ vanishes
on $\partial \Omega$, this means that $\Delta w = 
(N-1)\bold H \partial_\nu w + \partial^2_\nu w$.
Since also $\Delta w \in V_n$ vanishes on $\partial \Omega$, we obtain at 
each boundary point 
$$
\sum_{i,j} w_{,i}  w_{,i,j} \nu_j = \partial_\nu w \partial^2_\nu w 
= - (N-1)\bold H |\partial_\nu w|^2 =  -(N-1)\bold H |\nabla w|^2 \, .
$$
Therefore the boundary integral reduces to a term containing only first
derivatives that can be estimated from above by means of a trace theorem:
$$
\align
\int_{\partial \Omega} \sum_{i,j} g(|\nabla w|^2) w_{,i,j} w_{,i} \nu_j
   & = - \int_{\partial \Omega} (N-1) \bold H g(|\nabla w|^2) |\nabla w|^2 \\
   &\le \epsilon \|\nabla\left(\sqrt{g(|\nabla w|^2)}\nabla w\right)\|^2
     +  C \|g(|\nabla w|^2)|\nabla w|^2\|_{L^1} \\
   &\le \epsilon \|\nabla\left(\sqrt{g(|\nabla w|^2)}\nabla w\right)\|^2
     + C_1 (1 + \int_\Omega G(|\nabla w|^2)) \tag 2.33
\endalign
$$
for any $\epsilon > 0$ with suitable $C, C_1 > 0$. Here Lemma 2 was used to 
arrive at the last line.

 
The integral over  $\Omega$ in (2.32) is
$$
\gather
- \int_{\Omega} \sum_{i,j} w_{,i,j} (g(|\nabla w|^2)w_{,i})_{,j} \\ =
 - \int_{\Omega}\sum_{i,j} \left(g(|\nabla w|^2) w_{,i,j}w_{,i,j} + 2
   \sum_k g'(| \nabla w|^2) w_{,i,j}w_{,i}w_{,j,k}w_{,k} \right)  \\
 = -\int_{\Omega}\left( g(r^2) D^2 + 2g'(r^2) d^2 \right) 
\endgather
$$
with the abbreviations $r^2 = |\nabla w|^2, \, D^2 = |\nabla^2 w|^2 = 
\sum_{i,j}w_{,i,j}w_{,i,j}, \, d^2 =  |\nabla^2 w \nabla w|^2 = 
\sum_{i,j,k} w_{,i,j}w_{,i}w_{,j,k} w_{,k}$. On the other hand,
$$
|\nabla\left(\sqrt{g(|\nabla w|^2)}\nabla w\right)|^2 = 
        g(r^2)D^2 + 2g'(r^2)d^2 + \frac{(g'(r^2))^2r^2d^2}{g(r^2)} \, .
$$
Using (2.6), this term can be estimated from above by a constant multiple of
$g(r^2)D^2 + 2g'(r^2)d^2$, and therefore
$$
-\int_{\Omega} \sum_{i,j} (g(|\nabla w|^2)w_{,i})_{,j} 
w_{,i,j} 
\le -\delta \|\nabla\left(\sqrt{g(|\nabla w|^2)}\nabla w\right)\|^2_{L^2} 
$$
with some fixed $\delta > 0$. 
Combining this last estimate and (2.33) with $\epsilon = \delta /2$, 
one finally obtains
$$
\int_\Omega g(|\nabla w|^2) \nabla w \cdot \nabla ( \Delta w)   
\le - \epsilon \int_\Omega |\nabla\left(\sqrt{g(|\nabla w|^2)}\nabla w\right)|^2
+ C(1 + \int_\Omega G(|\nabla w|^2) ) \, , \tag 2.34 
$$
for some $\epsilon, \, C > 0$.
Using estimate (2.26), rearranging terms in (2.28), and combining all 
estimates, we thus deduce that
$$
\int_{0}^{{T'}} ({T'}-t) \|\nabla \left( \sqrt{ g(|\nabla u^n(\cdot ,t)|^2)} 
\nabla u^n(\cdot ,t) \right) \|^2 \, dt \le C \tag 2.35
$$
independent of $n$.  In particular, 
$$
\int_{0}^{T}  \|\nabla^2 u^n(\cdot ,t) \|^2 \, dt \le C \, .
\tag 2.36
$$

 
{\it Passage to the Limit.}
 Estimates (2.23) and (2.36) imply that
the set of all $\nabla u^n $ is in a relatively compact subset of
$L^2(0,T;L^2(\Omega))$ (\cite{12}). We can therefore extract a subsequence
$u^{M(n)} $ such that
$$
\align
\nabla u^{M(n)} \, \to \, \nabla u \quad &\text{strongly in 
$L^2(0,T;L^2(\Omega))$} \\
&\text{and pointwise a.e. on $\Omega \times (0,T)$} \\
\nabla^2 u^{M(n)}  \, \to \, \nabla^2 u \quad &\text{ weakly in $L^2(0,T;
L^2(\Omega))$} \\
u^{M(n)}_t \, \to \, u_t \quad &\text{weakly-* in $L^\infty(0,T;L^2(\Omega))$}
\endalign
$$
Also, $u \in H^{\frac{1+\alpha}{2}}([0,T],H^1(\Omega))$ by (2.25).
Estimate (2.26) and
Lemma 2 below imply that the $g^n = g(|\nabla u^n|^2)\nabla u^n$
are in a bounded subset of $L^\infty(0,T;L^p(\Omega))$ for some $p > 1$.
Therefore the subsequence can be chosen such that also
$$                                          
g(|\nabla u^{M(n)} |^2) \nabla u^{M(n)}  \, \to \, \xi
\quad \text{weakly-* in $L^\infty(0,T;L^p(\Omega))$}
$$ 
for some $\xi \in L^\infty(0,T;L^p(\Omega))$. Since also 
$g(|\nabla u^{M(n)}|^2) \nabla u^{M(n)}  \, \to \, g(|\nabla u|^2)\nabla u$
pointwise a.e., Lemma 3 implies that $\xi = g(|\nabla u|^2)\nabla u$.
Passing now to the limit in equation (2.10), we see that
$$
\langle u_t,v\rangle + \langle a* g(|\nabla u|^2)\nabla u, \nabla v\rangle 
= \langle f,v \rangle 
$$
for all $v \in \cup_n V_n$ and therefore by density for all $v \in
C^\infty_0(\Omega)$. Therefore, $u$ is a distributional solution of (1.1)
on $\Omega \times [0,T]$.

 
{\it Additional Regularity. }
For any differentiable function $h: [0,\infty) \, \to \, \Bbb R$
and any sufficiently smooth function $w: \bar \Omega \, \to \, \Bbb R$,
we compute
$$
\nabla \left(h(|\nabla w|^2)\nabla w \right)  = \left(h(|\nabla w|^2)
w_{,i,j} + 2 h'(|\nabla w|^2) \sum_k w_{,k,j} w_{,i} \right)_{i,j} 
$$
Using again the notation  $r^2 = |\nabla w|^2, \, D^2 = |\nabla^2w|^2, \,  
d^2 = |\nabla^2 w \nabla w|^2$ and setting $g = h$ we obtain after estimating 
$$
|\nabla \left( g(|\nabla w^2) \nabla w \right) | \le C g(r^2)D \, .
\tag 2.37
$$
With $h = \sqrt{g}$, we obtain at points where $g'(|\nabla w|^2) < 0$ 
$$
\align
|\nabla \left( \sqrt{ g(|\nabla u|^2)} 
\nabla u) \right)|^2 &= g(|r^2) D^2 + 2 g'(r^2)d^2 + 
\frac{(g'(r^2))^2}{g(r^2)} r^2 d^2 \\
&\ge  g(r^2) D^2 + 2 g'(r^2)d^2  \\
&\ge g(r^2)D^2 + 2 g'(r^2) D^2 r^2 \\
&\ge \frac{\epsilon}{2+\epsilon} g(r^2)D^2  \tag 2.38
\endalign
$$
from (2.6).
The same estimate holds trivially at points where $g'(|\nabla w|^2) \ge 0$. 
Now let $1 < q < 2$, to be fixed later. Then by (2.37), (2.38),
and H\"older's inequality
$$
\align
\|\nabla \left(g(|\nabla w|^2)\nabla w \right)\|^q_{L^q} & \le
C \int_\Omega \left( g(r^2) D \right)^q  \\
& = C \int_\Omega  g(r^2)^{q/2}D^q g(r^2)^{q/2}  \\
&\le C \left(\int_\Omega  g(r^2)D^2 \right)^{q/2}
\left( \int_\Omega g(r^2)^{q/(2-q)} \right)^{1-q/2} \\
&\le   C \left(\int_\Omega  |\nabla \left( \sqrt{g(|\nabla w|^2)}
\nabla w \right)|^2 \right)^{q/2}
\left( \int_\Omega g(r^2)^{q/(2-q)}\right)^{1 - q/2}  \, . \tag 2.39
\endalign
$$
If $q = 1 + \frac{\delta}{1 + 2\delta} \in (1,2)$ with $\delta$ as in Lemma 2,
we can estimate further
$$
\int_\Omega g(r^2)^{q/(2-q)} \le 
C \left( 1 + \int_\Omega G(r^2) \right) \, .
$$ 
We use these estimates for $w = u(\cdot,t)$ for any fixed $t$
and infer that
$$
\|\nabla \left(g(|\nabla u(\cdot,t)|^2)\nabla u(\cdot,t) \right)\|_{L^q}^2 
\le C \|\nabla \left( \sqrt{g(|\nabla u(\cdot,t)|^2)}
\nabla u(\cdot,t)\right)\|^2   
$$
The right hand side is integrable over $[0,T]$, and therefore
$\nabla\left( g(|\nabla u|^2)\nabla u \right) \in 
L^2(0,T;L^q(\Omega))$ with this $q$.
\enddemo


\proclaim{Lemma 2}
If $g:[0,\infty) \, \to \, \Bbb R$ satisfies (2.6), then there exist
$\delta , C > 0$ such that for all $r \ge 0$
$$
\align
|g(r^2)r|^{1+\delta } &\le C(1 + G(r^2)) \, , \\
g(r^2) r^2 & \le C(1 + G(r^2)) \, .
\endalign
$$
\endproclaim

 
\demo{Proof}
A constant $C$ can be found such that both inequalities are true for all
$r \le 1$. For $r \ge 1$, we have with $\beta$ as in (2.6) and 
$\delta = \dfrac{1}{2\beta + 1}$
$$
\align
\frac{d}{dr} \left(g(r^2)r \right)^{1 + \delta } & =
(1 + \delta ) g^\delta (r^2)r^\delta (g(r^2) + 2r^2g'(r^2)) \\
& \le Cg^{1+\delta }(r^2)r^\delta  \\
&\le Cg(r^2) r^{2\delta \beta + \delta }\\
&\le Cg(r^2)r = C \frac{d}{dr}G(r^2) \, .
\endalign
$$
An integration implies the first estimate. The second estimate follows 
from (2.6) in the form
$$
g'(r^2)r^3 + g(r^2)r \le (\beta + 1)g(r^2)r
$$
by integrating.
\enddemo

 

\proclaim{Lemma 3}
Let $\Omega \subset \Bbb R^N$ be measurable and bounded 
and let $z_n$ be a sequence in $L^1(\Omega)$ satisfying
$$
\align
z_n(x) \, \to \, \xi(x) \quad &\text{for a.e. $x \in \Omega$ } \\
z_n \, \to \, \zeta \quad &\text{weakly in $L^1(\Omega)$.} 
\endalign
$$
Then $ \zeta = \xi $ almost everywhere.
\endproclaim

 
\demo{Proof} The function $\xi$ must be finite almost everywhere,
otherwise  the $z_n$ cannot converge weakly. 
Let $\epsilon > 0$. By Egorov's Theorem, there exists a
subset $\Omega_\epsilon \subset \Omega$ such that $z_n \, \to \,
\xi$ uniformly on $\Omega_\epsilon$, $|\xi| \le \epsilon^{-1}$ on
$\Omega_\epsilon$,  and 
$meas(\Omega \,  - \,  \Omega_\epsilon) < \epsilon$ . 
Set $\varphi(x) =
sign(\xi(x) - \zeta(x)) \cdot I_{\Omega_\epsilon}(x)$, then
$$
\int_{\Omega_\epsilon} |\xi-\zeta| =
\int_{\Omega_\epsilon} (\xi - z_n) \varphi_M - \int_{\Omega_\epsilon} 
(\zeta - z_n) \varphi_M \, .
$$
As $n \, \to \, \infty$, both terms go to zero by assumption and because
of the Dominated Convergence Theorem. Therefore $\xi = \zeta$ a.e. on
$\Omega_\epsilon$. As $\epsilon \, \to \, 0$,  the conclusion follows.
\enddemo

  

\head
3. Extensions and Counterexamples
\endhead

The question arises whether a result like Theorem 1 is still true if 
$0 < \alpha \le \frac{1}{2}$. The short answer is that the theorem 
is no longer correct for this range of $\alpha$'s. Below, we give some 
counterexamples to show this. However, these counterexamples are essentially 
related to regularity properties for linear equations. A suitable 
modification can still be expected to hold for $0 < \alpha \le \frac{1}{2}$. 
For $\alpha = \frac{1}{2}$, this is the content of 
the next corollary. For nonlinear problems with $0 < \alpha <
\frac{1}{2}$, the question of existence of solutions $u$ for which
$u(\cdot,t) \in H^2(\Omega)$ for $ t > 0$ remains open, except for the
result in \cite{8}.

 
\proclaim{Corollary 4} Let $\alpha = \dfrac{1}{2}$, let the assumptions
of Theorem 1 hold, and assume that for some $r > 1$
$$
\int_{0}^T \|f_t(\cdot,t)\|^r \, dt < \infty \, . \tag 3.1
$$
\item{a)} If $f(\cdot,0) \in H^1_0(\Omega)$, then the statement of Theorem 1 
remains true.
\item{b)} If $f(\cdot,0) \in L^2(\Omega)$, then a solution $u$ of 
(2.1) exists for which
$$
\int_{0}^T t \| u (\cdot,t)\|^2_{H^2} \, dt < \infty \tag 3.2
$$
and $u \in W^{1,\infty}([0,T],L^2(\Omega)) \cap
H^\frac{3}{4}([0,T],H^1_0(\Omega))$.
\endproclaim

 
\demo{Outline of Proof}
We use the same approximation as in the proof of Theorem 1 and derive
estimates (2.23) -- (2.26) in the same way. In case a), we can assume 
that the $f^n(\cdot,0)$ are all in $H^1_0(\Omega)$. 
We can then carry out {\sl a priori estimate II}  by integrating by parts in 
the right hand side of (2.28), obtaining
$$
 \int_0^{T'} \big( \langle -b(t)  \nabla f^n(\cdot,0), (t-T') 
\nabla u^n(\cdot,t)   \rangle + \langle b*f^n_t(\cdot,t), (t-T') 
\Delta u^n(\cdot,t) \rangle \big) \, dt \, .
$$
Since $b \in L^q(0,T')$ for all $q < 2$ and due to (2.25), this can be 
estimated  by
$$
C(b, \|\nabla f^n(\cdot,0) \|) +  
C(\epsilon, T') \|b\|_{L^q(0,T')} \|f^n_t\|^2_{L^r(0,T';L^2)}
+ \epsilon \int_{0}^{T'}(T'-t)\|\Delta u^n(\cdot ,t)\|^2 \, dt 
$$
with $q = \dfrac{2r}{3r-2}$. No change is required for the remaining 
arguments, and the conclusion follows as before.

\smallskip
In case b), we proceed as before and obtain approximating solutions that
satisfy (2.23) -- (2.26). We then use the test function $v = t(t-T')\Delta
u^n(\cdot,t)$ in the arguments that follow (2.27). Instead of (2.29),  
we then obtain an estimate with the right hand side
$$\gather
C_0(\epsilon,T',b) \|f^n(\cdot,0)\|^2 + 
C_1(\epsilon,T') \|b\|_{L^q(0,T')} \|f^n_t\|^2_{L^r(0,T';L^2)}\\
+ \epsilon \int_{0}^{T'} t(T'-t)\|\Delta u^n(\cdot ,t)\|^2 \, dt \, . 
\endgather
$$
The other terms in the identity that is analogous to (2.28)
can be treated as before. The additional factor $t$ in the test 
function $v$ leads to some longer version of (2.31); we leave the details
to the interested reader. In the passage to the limit, we now only
assert that
$$
\nabla^2 u^{M(n)} \, \to \, \nabla^2 u \quad \text{weakly in}
\quad
L^2(\delta,T; L^2(\Omega))
$$
for all $\delta > 0$. This is sufficient to conclude the proof.

\enddemo

 
To construct counterexamples that show that the conditions in these
results are sharp, several facts about scalar integro-differential
equations will be used.

 
\proclaim{Lemma 5} For $ 0 < \alpha < 1$ fixed and for arbitrary
$\lambda > 0$, let $u_\lambda, \, v_\lambda: 
[0,1] \to \Bbb R$ be the solutions of
$$
\align
u'_\lambda(t) + \lambda a_\alpha*u_\lambda = 0 &\quad (0 \le t \le 1) , 
\quad u_\lambda(0) = 1                          \\
v'_\lambda(t) + \lambda a_\alpha*v_\lambda = 1 &\quad (0 \le t \le 1) , 
\quad v_\lambda(0) = 0 
\endalign
$$
where $a_\alpha$ is as in (2.4). Then
$$
\align
\sup_\lambda \int_0^1 \lambda^2 t^\gamma u_\lambda^2(t) \, dt
< \infty \quad &\text{iff} \quad  2\alpha +  \gamma > 3  \,  \tag 3.3\\
\sup_{\lambda} \int_0^1 \lambda^2 t^\gamma v_\lambda^2(t) \, dt
< \infty \quad &\text{iff} \quad  2\alpha + \gamma > 1  \, .  \tag 3.4
\endalign
$$
\endproclaim

 
\demo{Proof}
It is known that
$$
u_\lambda(t) = E_{2-\alpha}(- \lambda t^{2-\alpha}) \, , \quad
v_\lambda(t) = \int_0^t E_{2-\alpha}(-\lambda s^{2 - \alpha}) \, ds
$$
where
$$
E_\sigma(z) = \sum_{k=0}^\infty \frac{z^k}{\Gamma(1 + \sigma k)}
$$    
is the \smc Mittag-Leffler \rm function (\cite{4}, \cite{5}). 
Therefore the estimates (3.3) and (3.4) follow immediately for, say,
$0 \le \lambda \le K$, where $K$ is any fixed finite value, and we only
have to prove them for large values of $\lambda$. 
If $0 < \sigma < 2$, then
$$
E_\sigma(-z) = \frac{z^{-1}}{\Gamma(1-\sigma)} + O(z^{-2}) 
$$
as $z \, \to \,  \infty$ (\cite{4}).
Therefore there exist constants $c_1, \, c_2, \, c_3, \, c_4 > 0$
such that 
$$
\align
&|u_\lambda(t)| \le c_1 \quad \qquad \qquad (\lambda t^{2-\alpha} \le c_2) \\
c_3 \lambda^{-1} t^{\alpha-2} \le &|u_\lambda(t)| \le 
c_4 \lambda^{-1} t^{\alpha-2} \quad (\lambda t^{2-\alpha} \ge c_2) \, .
\tag 3.5
\endalign
$$
The equation for $u_\lambda$  shows that the Laplace transform of
$u_\lambda$ is given by
$$
\hat{u_\lambda}(s) = \frac{1}{s + \lambda s^{\alpha-1}}
$$
which implies $\int_{0}^\infty u_\lambda(t) \, dt = 0$. Therefore, with 
the same constants $c_1, \dots, c_4$ we can also assume that
$$
\align
&|v_\lambda(t)| \le c_1 \quad \qquad \qquad (\lambda t^{2-\alpha} \le c_2) \\
c_3 \lambda^{-1} t^{\alpha-1} \le &|v_\lambda(t)| \le 
c_4 \lambda^{-1} t^{\alpha-1} \quad (\lambda t^{2-\alpha} \ge c_2) \, .
\tag 3.6
\endalign
$$
Suppose now that $2\alpha + \gamma > 3$. Then
$$
\align
\int_0^1 \lambda^2 t^\gamma u_\lambda^2(t) \, dt &= 
\int_0^{(c_2/ \lambda)^{1/(2-\alpha)}} 
\lambda^2 t^\gamma u_\lambda^2(t) \, dt + 
\int_{(c_2/\lambda)^{1/(2-\alpha)}}^1 
\lambda^2 t^\gamma u_\lambda^2(t) \, dt \\
&  \le 
\int_0^{(c_2/ \lambda)^{1/(2-\alpha)}} \lambda^2 c_1^2 t^\gamma  dt + 
\int_0^1  t^\gamma c_4^2 t^{2\alpha-4} \, dt \\
& \le C \lambda^{2 - \frac{\gamma + 1}{2 - \alpha}} + C \\
& \le C < \infty
\endalign
$$
independently of $\lambda$. The same argument, using (3.6) instead of
(3.5), shows that 
$$
\sup_{\lambda} \int_0^1 \lambda^2 t^\gamma v_\lambda^2(t) \, dt
< \infty 
$$
if  $ 2 \alpha + \gamma > 1$. Suppose next that
$2 \alpha + \gamma \le 3$. Then
$$
\int_0^1 \lambda^2 t^\gamma u_\lambda^2(t) \, dt \ge 
\int_{(c_2/ \lambda)^{1/(2-\alpha)}}^1 \lambda^2 t^\gamma u_\lambda^2(t) 
\, dt \ge 
\int_{(c_2/ \lambda)^{1/(2-\alpha)}}^1 c_3^2 t^{\gamma + 2 \alpha - 4} \, dt
$$
and the last integral does not remain bounded as $\lambda \, \to \, \infty$.
Thus the supremum in (3.3) is infinite if $2 \alpha + \gamma \le 3$.
Using (3.6), it follows that the supremum in (3.4) is infinite
if $2 \alpha + \gamma \le 1$.
\enddemo

 
It is also possible to show that
$$
\sup_{\lambda} \int_0^1 \lambda^{2\delta} t^\gamma u_\lambda^2(t) \, dt
= \infty 
$$
if $\delta > 1$ and that this supremum is finite for $ \delta < 1$ iff in 
addition $2 \delta (2-\alpha) \le \gamma + 1$. Similar statements hold
for the supremum that can be formed with the $ v_\lambda$. Note that the 
supremum is finite if $2 \delta(2 - \alpha) = \gamma + 1$ for 
$\delta < 1$, but infinite in the case $ \delta = 1$.

 
{\bf Counterexamples. }
 Consider the problems
$$
u_t(x,t) - \int_0^t a_\alpha(t-s) \Delta u(x,s) \, ds = F(x,t)
\quad (0 < t \le 1, \, x \in \Omega)      \tag 3.7
$$
with
$$
F(x,t) = f_0(x) + \int_0^t f_1(x,s) \, ds 
$$
and initial data  $u(x,0) = 0$ in $\Omega$. As before, let $(\varphi_i)_i$ be
the set of eigenfunctions of $-\Delta$ with zero Dirichlet boundary
conditions, with eigenvalues $0 < \lambda_1 < \lambda_2 \le \lambda_3 \le 
\dots$.  

 
Suppose first that $ f_0 = \sum_i c_i \varphi_i \in L^2(\Omega)$ and
$f_1 = 0$. The solution of (3.7) then is given by
$$
u(\cdot,t) = \sum_{i=1}^\infty c_i v_{\lambda_i}(t) \varphi_i
$$
and thus
$$
\align
\|u(\cdot,t)\|_{H^2}^2 &\ge C \|\Delta u(\cdot,t)\|^2 \\
& = C\sum_{i=1}^\infty  c_i^2 \lambda_i^2 |v_{\lambda_i}(t)|^2 \, .
\tag 3.8
\endalign
$$
If $\alpha \le \frac{1}{2}$, then there exist $c_i$ such that
$f_0 \in L^2(\Omega)$ but 
$\int_{0}^1 \|u(\cdot,t)\|_{H^2}^2 dt = \infty$,
according to Lemma 5. However, if $\gamma > 1 - 2\alpha \ge 0$, then
$\int_{0}^1 t^\gamma\|u(\cdot,t)\|_{H^2}^2 dt < \infty$ for any such 
$f_0$. 

 
Suppose next that $f_0 = 0$ and $f_1(\cdot,t) =
h_i(t)\varphi_i$. Then $ u(\cdot,t) = \int_0^t h_i(t-s)v_{\lambda_i}(s) \, ds 
\cdot \varphi_i$. Pick $h_i(t) = k_i h(k_it)$, where $h \ge 0$ is smooth, supported 
on $[0,1]$, $\int_{0}^1 h(t) \, dt = 1$, and $k_i> 1$ is so large that 
$$
\int_{0}^1| v_{\lambda_i}*h_i(t)|^2 \, dt \ge \frac{1}{2} 
\int_{0}^1| v_{\lambda_i}(t)|^2 \, dt \, .
$$
It follows that
$$
\|u(\cdot,t)\|_{H^2}^2 \ge C \|\Delta u(\cdot,t)\|^2 
= C \lambda_i^2 \int_{0}^1|v_{\lambda_i}* h_i(t)|^2 \, dt 
 \ge C \lambda_i^2 \int_{0}^1 |v_{\lambda_i}(t)|^2 \, dt = M_i 
\, .
\tag 3.9
$$
If $\alpha \le \frac{1}{2}$, then $ \lim \, \sup M_i = \infty$.
On the other hand,
$$
\int_{0}^1 \|f_1(\cdot,t)\| \, dt = \int_{0}^1 h_i(t) \, dt = 1 \, .
$$
Choose $c_i$ such that $\sum_{i=1}^\infty |c_i| < \infty$ and
$\sum_{i=1}^\infty c_i^2 M_i = \infty$ and set \newline
$ f_1(\cdot,t) = \sum_{i=1}^\infty c_i h_i(t) \varphi_i$,
then 
$$
\int_{0}^1 \|f_1(\cdot,t)\| \, dt < \infty \quad
\text{and} \quad \int_{0}^T \|u(\cdot,t)\|_{H^2}^2 \, dt = \infty \, .
\tag 3.10
$$
These arguments show that Theorem 1 does not extend to the case $\alpha 
\le \frac{1}{2}$ without strengthening some assumptions or weakening some
conclusions, as in Corollary 4. Similar
constructions can be used to show that the assumption
$u_0 \in H^2(\Omega)$ can only be weakened slightly if solutions are 
still to belong to $L^2(0,T; H^2(\Omega))$.

 
\subhead Acknowledgment \endsubhead
 The author would like to thank the referee for several useful
comments.
 

\Refs

\ref \no 1 
\by R. A. Adams 
\book Sobolev Spaces 
\publ Academic Press \publaddr New York \yr 1975
\endref

\ref \no 2
\by H. Engler
\paper Strong solutions for strongly damped quasilinear wave
equations
\inbook Contemporary Mathematics \vol 64 \yr 1987
\procinfo Symposium on the Legacy of Sonya Kovalevskaya,
October 1985 \pages  219 -- 237
\endref 

\ref \no 3
\bysame  
\paper  Global smooth solutions for a class of 
parabolic integro-differential equations
\jour Trans. Amer. Math. Soc. \miscnote submitted
\endref

\ref \no 4
\by A. Erdelyi
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\by A. Friedman
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equations in Banach spaces
\jour Trans. Amer. Math. Soc. \vol 198 \yr 1969 \pages 129 -- 148
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\ref \no 6
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\yr 1991
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\by G. Gripenberg, S.-O. Londen, \& O. Staffans
\book Volterra Integral and Functional Equations
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\ref \no 8
\by G. Gripenberg
\paper Global existence of solutions of Volterra 
integro-differential equations of parabolic type 
\jour J. Differential Eq. \vol 102 \yr 1993 \pages  382 -- 390
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\ref \no 9
\by G. Gripenberg
\paper Nonlinear Volterra equations of parabolic type due to 
singular kernels
\jour J. Differential Eq. \vol 112 \yr 1994 \pages  154 -- 169
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\bookinfo Applied Math. Sciences Vol. 3
\publ Springer \publaddr Berlin, Heidelberg, New York \yr 1977
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\by J. Heikonen
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Parabolic Integro-differential Equation
\bookinfo Licentiate Thesis
\publ Helsinki Univ. of Technology \publaddr Espoo, Finland \yr  1993
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\by J.-L. Lions
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Non-Lin\'eaires
\publ Dunod \publaddr  Paris \yr  1969
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\by A. C. Pipkin
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\ref \no 14
\by M. Renardy, W.E. Hrusa \& J.A. Nohel
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\by R. P. Sperb
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\publ Academic Press \publaddr New York \yr 1981
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\endRefs

\enddocument 
\bye 



