We consider an abstract initial value problem
| |
(29) |
To this end, let us first review a few ways of defining the exponential of a matrix.
1. The power series:
| (30) |
2. As a limit:
| (31) |
3. By diagonalization or, more generally, transforming to Jordan canonical form. This is the procedure we followed in the preceding sections.
4. By Laplace transforms: Consider the equation
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(32) |
For unbounded operators, the power series definition is not useful. Consider the example of the heat equation discussed in the last section A=d2/dx2. Then formally, we would have
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(33) |
The definition as a limit seems to suffer from the same defect. However, we can make the following modification to it:
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(34) |
Theorem 3
Assume that A is a linear operator defined on a dense subspace D(A) of
a Hilbert space H. Assume further that there are constants M and
such that
exists (as an operator from H to D(A))
for
and
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(35) |
| |
(36) |
| (37) |
The set of operators
where
is referred to as a semigroup
of operators; it is closed under multiplication since
. It is in general not possible to extend t to negative
values; for instance the heat equation is well posed only for solutions forward
in time, not for solutions backward in time.
We note that
| (38) |
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(39) |
Example 7
To give a simple example, we show how the Hille-Yosida theorem applies to the heat equation, discussed in the previous section. We use the Fourier series representation
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(40) |
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(41) |
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(42) |
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(43) |
and consequently,
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(44) |
In a somewhat simpler fashion, we could argue that
| (45) |
| (46) |
| (47) |
| (48) |
| (49) |
| (50) |
The second argument given in the last example clearly yields a weaker conclusion
than the first. On the other hand, it required no knowledge of eigenvalues
and eigenfunctions. In general,
the representation of
in terms of eigenvalues and eigenfunctions
is very useful for closed form solutions, if such a representation is
available. As a foundation for a general theory, however, such a definition
would be too restrictive, since little is known (except for special cases
such as self-adjoint operators) about spectral representations. Indeed, there
are (physically relevant) examples of operators which do not even have a
spectrum, so any attempt to ``diagonalize"
is doomed from the
start.
Example 8
Consider the equation ut+ux=0, with boundary condition u(0,t)=0
on the interval (0,1). Abstractly, we associate with this the operator
Au=-u' with domain
. The initial
value problem has a well-defined solution, namely, we have
| (51) |
| (52) |
| (53) |
If, however, we consider the problem
, i.e.
| (54) |
| (55) |
In the earlier sections on stability of systems of ODEs, we established
a connection between stability and eigenvalues. For infinite-dimensional
systems, the issues are more complicated. First of all, there is
a more general notion of spectrum. We say that
is in the resolvent
set of A if the ``resolvent"
exists as a bounded operator defined on
all of H, and we say
is in the spectrum if it is not in the
resolvent set. In the finite-dimensional case, the spectrum consists
precisely of the eigenvalues, but in infinite dimensions this is no longer
the case; for instance, there may be what is known as a ``continuous spectrum."
Example 9
Consider, for instance, the operator
| Au[x]=xu[x] | (56) |
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(57) |
For any operator which satisfies the hypotheses of the Hille-Yosida theorem, we can define the following quantities:
We call r(A) the spectral bound, and
the type of the semigroup.
The quantity
measures the rate of exponential growth or decay
of
. The connection between spectrum and stability is established
if
. While it can be shown that
, the
converse inequality is in general not true. There are a
number of known counterexamples in the literature; a very natural
one [13] is the equation
| utt=uxx+uyy+eixuy, | (58) |
The Laplace inversion formula for
(see above) can be exploited
to establish a weaker result. Namely, it turns out that
We note that, if there are no spectral values for
, i.e.
if s>r(A), then the resolvent exists in that half plane. But this does
not necessarily imply that it is uniformly bounded. In the finite-dimensional
case, this is no issue, since
.
For a wide class of problems, including those of Newtonian fluid mechanics,
it is known that
. However, these results do not include
viscoelastic fluids, where the problem is in general still open. Hence we
do not know that the onset of instabilities is always associated with
eigenvalues crossing the imaginary axis. Nevertheless, many of the instabilities
observed clearly show the type of dynamics which is expected from such a
scenario, and we shall analyze them in the appropriate framework.