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(PDF file: paper9.pdf)
2 Preliminaries
A function is called the weak solution of the
time-periodic problem (1) and
|
(7) |
with period
if the function is bounded measurable in the region
, and there exists a bounded measurable
function such that space-periodic extensions of
, and satisfy
|
(8) |
for any
.
Note that the definition has other equivalent forms.
One is the following:
|
(9) |
for any
,
.
Another is expressed in terms of the space-periodic extension of
and for the
space and time periodic extension of .
That is, it is required to satisfy
|
(10) |
for any
.
The conclusion is that satisfies
(9) if and only if the followings valid
- is solution of (1) in weak sense
- converges in weak sense to as tends to
zero and as tends to
in weak.
-
and
converge in weak sense
to the same value
in weak for some function of
.
It seems that the function which satisfies above conditions
is a solution of the problem (1) satisfying
|
(11) |
instead of (7).
Certainly, both definitions are equivalent for the weak solution.
However, these include different means for the entropy condition.
The boundary condition of the original problem (7)
seems to say that the space-periodic extension satisfies the equation
(1), but the problem (11)
does not seem to require it. Hence in the case that boundary
values of the weak solution and are different,
these should satisfy the entropy condition, that is,
for (7), but should not
for (11).
It remains an open problem whether the boundary condition
(11) is well-posed.
A smooth function pair of
is an entropy pair for the scalar conservation law
|
(12) |
if
for a smooth solution of (12).
This is equivalent that and satisfy
The function called entropy and called entropy flux.
A weak solution satisfies the entropy condition if
|
(13) |
for any smooth entropy pair with convex entropy .
We suppose that the function is smooth,
|
(14) |
and is a time-periodic function with period . The last
relation for is need for the existence of a time periodic
solution.
We also assume that the space-extension of satisfies
|
(15) |
for any and , where is a constant. The condition
is necessary by a technical reason.
It is well-known that the solution of the Riemann problem
for the scalar conservation law
|
(16) |
is each of the two typical waves.
In the case the solution is the rarefaction wave
and in the case the solution is the shock wave
where the shock speed is determined by the
Rankine-Hugoniot relation
and Lax's entropy condition
(cf. [7], [12]).
We note that the average on the line
for the solution of the Riemann problem is equal to the
Lax-Friedrichs difference approximation
provided the Courant-Friedrichs-Lewy (CFL) condition
Next: 3 Approximate Solution
Up: Time-periodic solutions
Previous: 1 Introduction
Shigeharu TAKENO
15 January 2002