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HAL Id: hal-00159729

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Preprint submitted on 21 Jul 2007

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Two Results concerning the Small Viscosity Solution of Linear Scalar Conservation Laws with Discontinuous

Coefficients.

Bruno Fornet

To cite this version:

Bruno Fornet. Two Results concerning the Small Viscosity Solution of Linear Scalar Conservation

Laws with Discontinuous Coefficients.. 2007. �hal-00159729v6�

(2)

Two results concerning the small viscosity solution of linear

conservation laws with discontinuous coefficients.

B. Fornet [fornet@cmi.univ-mrs.fr]

∗†

July 21, 2007

Abstract

In this paper, we consider the vanishing viscosity approach of the linear hyperbolic Cauchy problem in 1-D

(∂tu+∂x(au) =f, {t >0, x∈R}, u|t=0=h,

when the coefficient a(t, x) is discontinuous across the line {x = 0}

and smooth on {x 6= 0}. Two cases are treated: the expansive (or completely outgoing) case where sign(xa(t, x)) > 0, for all (t, x) in a neighborhood of{x= 0}, and the compressive case (or completely ingoing) case wheresign(xa(t, x))<0,for all (t, x) in a neighborhood of {x = 0}. In both cases, we show that the solution of the viscous problem converges and selects a well defined ”generalized solution”.

In the expansive case, our first result answers the open question of selecting a unique solution to the hyperbolic problem, answering a question raised in paper [9]. In the compressive case, we show the formation of a Dirac measure in the small viscosity limit. Moreover, the considered problem does not need to be the linearized of a shockwave on a shock front. For both results, a detailed asymptotic analysis is made via the construction of approximate solutions at any order, including a boundary layer analysis. Moreover, both results state not only existence and uniqueness of the solution but its stability, and are new.

LATP, Universit´e de Provence,39 rue Joliot-Curie, 13453 Marseille cedex 13, France.

LMRS, Universit´e de Rouen,Avenue de l’Universit´e, BP.12, 76801 Saint Etienne du Rouvray, France.

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1 Introduction.

Consider the conservative 1-D Cauchy problem:

(1.1)

(

t

u + ∂

x

(a(t, x)u) = f, x ∈

R,

u|

t=0

= h .

If a is discontinuous through {x = 0}, problem (1.1) has no classical sense and a new notion of solution has to be introduced. Several approaches have already been proposed. Among them, renormalized solutions for this sort of problems have been introduced by Diperna and Lions in [3]. In [1] and [2], Bouchut, James and Mancini defines a notion of solution around the parallel study of the conservative problem (1.1) and the associated nonconservative problem:

(1.2)

(

t

u + a(t, x)∂

x

u = g, x ∈

R

, u|

t=0

= l .

In [9], Poupaud and Rascle proposes a notion of solution based on generalized characteristics in the sense of Filippov.

In this short paper, we will consider the vanishing viscosity approach in the case where a(t, x) is a piecewise smooth function. Let us describe our assumptions. Let T > 0 be fixed once for all. We will assume that the coefficient a belongs to the space of infinitely differentiable functions, bounded with all their derivatives: C

b

([0, T ] ×

R

), with

R

=

R

− {0}.

Furthermore, we assume that f belongs to C

0

([0, T ] ×

R) and

h belongs to C

0

(

R

). As a first step, let us take a(x) := a

R

1

x>0

+ a

L

1

x<0

, where a

L

and a

R

denote two constants in

R

. Different cases have to be considered depending on the sign of a

L

and a

R

. Among those cases, the most interesting ones are when a

L

and a

R

are of opposite sign. If a

L

> 0 and a

R

< 0 [resp a

L

< 0 and a

R

> 0], the associated problem will fall into what we call the ”ingoing case” [resp ”outgoing case” or ”expansive case”]. Our two results state existence, uniqueness and stability of the solution obtained by vanishing viscous perturbation of (1.1). The first result deals with the expansive case where uniqueness is the main concern whereas the second result deals with the ingoing case where existence is the main concern. Let ε denote a positive real number. Having in mind to make ε tends towards zero, we consider the following viscous perturbation of (1.1):

(1.3)

(

t

u

ε

+ ∂

x

(a(t, x)u

ε

) − ε∂

x2

u

ε

= f, x ∈

R

,

u

ε

|

t=0

= h .

(4)

We prove then a convergence result stating that the solution u

ε

of (1.3) tends towards u deduced from an asymptotic analysis of the problem. Naturally, u is then what could be called the small viscosity solution of (1.1). In the ingoing case, u is a measure-valued solution which coincides with the gener- alized solution introduced in the already cited papers. But the interesting point is the asymptotic expansion which gives a very precise description of the solution. In the expansive case, the result seems to be completely new, since the main difficulty was to ”select” a solution among all possible weak solutions.

2 Viscous treatment of the expansive case.

For our first result, let us consider equation (1.3) in the case where the coefficient a satisfies, for all t ∈ [0, T ],

a(t, 0

+

) > 0, a(t, 0

) < 0.

We will denote by a

R

the restriction of a to {x > 0} and by a

L

the restriction of a to {x < 0}.

Remark 2.1. The value of a|

x=0

is of no concern here. Moreover, by taking f = 0, a

L

= −1 and a

R

= 1, we recover the singular expansive case given by Poupaud and Rascle as an example in [9].

Let us define u by u := u

R

1

x≥0

+ u

L

1

x<0

, where (u

R

, u

L

) is the unique solution of the following problem:

(2.1)









t

u

R

+ ∂

x

(a

R

u

R

) = f

R

, {x > 0},

t

u

L

+ ∂

x

(a

L

u

L

) = f

L

, {x < 0}, u

R

|

x=0

= u

L

|

x=0

= 0, ∀t ∈ (0, T ], u

R

|

t=0

= h

R

, u

L

|

t=0

= h

L

,

where f

R

[resp h

R

] denotes the restriction of f [resp h] to {x > 0}, and f

L

[resp h

L

] denotes the restriction of f [resp h] to {x < 0}. Note well that this problem has a unique solution in L

2

([0, T ] ×

R

), which is given on the side {x < 0} by:





t

u

L

+ ∂

x

(a

L

u

L

) = f

L

, {x < 0}, u

L

|

x=0

= 0, ∀t ∈ (0, T ],

u

L

|

t=0

= h

L

,

(5)

and on the side {x > 0} by:





t

u

R

+ ∂

x

(a

R

u

R

) = f

R

, {x > 0}, u

R

|

x=0

= 0, ∀t ∈ (0, T ],

u

R

|

t=0

= h

R

.

Remark that, in general, h

R

(0) = h

L

(0) 6= 0, and thus the corner compati- bilities are not satisfied. Let us compute u in the case where f = 0. We will first introduce some notations. Let Ω

R

be (0, T ) ×

R∗+

. Consider now the vector field defined through: (t, x) 7→ ∂

t

+ a

R

(t, x)∂

x

. We will denote by Γ

R

the characteristic curve passing through t = 0, x = 0 and tangent to this vec- tor field. A parametrization of Γ

R

is given by: Γ

R

= {(t, x

R

(t)), t ∈ (0, T )}, where x

R

is the solution of the equation:

dx

R

dt (t) = a

R

(t, x

R

(t)), t ∈ (0, T ), x

R

(0) = 0 .

Let us denote by ˜ a

R

an arbitrary smooth extension of a

R

to {x < 0}. We define then ϕ

R

as the solution of:

(

(∂

t

+ ˜ a

R

(t, x)∂

x

R

= 0, (t, x) ∈ (0, T ) ×

R

, ϕ

R

|

t=0

= x .

The obtained ϕ

R

is in C

((0, T ) ×

R

). Moreover, we have:

Γ

R

= {(t, x) ∈ Ω

R

: ϕ

R

(t, x) = 0}.

L

, Γ

L

and ϕ

L

are defined in a symmetric way and there holds:

Γ

L

= {(t, x) ∈ Ω

L

: ϕ

L

(t, x) = 0}.

Note well that, by construction of ϕ

L

and ϕ

R

, we have:

Lemma 2.2. There is c such that, for all (t, x) ∈ Γ

R

, there holds:

|∂

x

ϕ

R

(t, x)| ≥ c > 0, |∂

x

ϕ

L

(t, x)| ≥ c > 0.

Proof.

Differentiating the equation with respect to x, we obtain that v := ∂

x

ϕ

R

is the solution of the following transport equation:

(

(∂

t

+ ˜ a

R

x

)v + (∂

x

˜ a

R

)v = 0, (t, x) ∈ (0, T ) ×

R,

v|

t=0

= 1 .

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v is solution of a linear homogeneous equation thus, it cannot cancel without being identically equal to zero along the characteristic curve and in particular for t = 0, which achieves to prove our Lemma for ϕ

R

. The proof for ϕ

L

is

identical.

2

We note for instance:

+L

= {(t, x) ∈ Ω

L

: ϕ

L

(t, x) > 0},

where the ”L” stands for ”on left hand side of Γ

L

” and the + is related to the sign of ϕ

L

(t, x). We define in the same manner: Ω

L

, Ω

+R

and Ω

R

.

+R

R

L

+L

t

x

Let us consider, as an example, the case where the coefficient is piecewise constant and f = 0. Solving the limiting hyperbolic problem, we get that, for all (t, x) ∈ Ω

+LS

RS

{x = 0},

u(t, x) = 0, for all (t, x) ∈ Ω

+R

,

u(t, x) = h

R

(x − a

R

t), and for all (t, x) ∈ Ω

L

,

u(t, x) = h

L

(x − a

L

t).

Observe that, in this case, the mass of u remains constant for all t ∈ [0, T ].

Moreover, this example shows clearly the discontinuity of u through the lines {x − a

R

t = 0} and {x − a

L

t = 0}.

Although equation (1.1) trivially admits an infinite number of solutions,

we prove the following result:

(7)

Theorem 2.3. There is C > 0 such that, for all 0 < ε < 1, there holds:

ku

ε

− uk

L([0,T]:L2(R))

≤ Cε

14

, where u

ε

is the solution of (1.3).

Proof.

We will begin by constructing an approximate solution of problem (1.3).

As a first step, we will reformulate problem (1.3) in an equivalent manner.

The restrictions of u

ε

to {x > 0} and {x < 0}, denoted respectively by u

εL

and u

εR

satisfy the following transmission problem:

(2.2)





















t

u

εR

+ ∂

x

(a

R

u

εR

) − ε∂

x2

u

εR

= f

R

, {x > 0}, t ∈ [0, T ],

t

u

εL

+ ∂

x

(a

L

u

εL

) − ε∂

x2

u

εL

= f

L

, {x < 0}, t ∈ [0, T ], [u

ε

]

x=0

= 0,

[a(x)u

ε

− ε∂

x

u

ε

]

x=0

= 0, u

εR

|

t=0

= h

R

,

u

εL

|

t=0

= h

L

.

Let us introduce L

εR

= ∂

t

+ ∂

x

(a

R

.) − ε

2

x2

and L

εL

= ∂

t

+ ∂

x

(a

L

.) − ε

2

x2

. We perform the construction of the approximate solution separately on the four domains Ω

L

, Ω

+L

, Ω

+R

and Ω

R

. . We will denote by u

εapp,L,+

the restriction of u

εapp

to Ω

+L

and so on. Let us present the different profiles and their ansatz:

u

εapp,L,+

(t, x) =

M

X

n=0

U

L,n,+

(t, x) + U

cL,n,+

t, ϕ

L

(t, x)

√ ε

ε

n2

,

where the profiles U

n,L,+

belongs to H

(Ω

+L

) and the characteristic bound- ary layer profiles U

cn,L,+

(t, x, θ

L

) belongs to e

−δ|θL|

H

((0, T ) ×

R∗+

), for some δ > 0. We will take a similar ansatz for u

εapp,L,−

, u

εapp,R,−

and u

εapp,R,+

over their respective domains. Let us explain the different steps of the construction of the approximate solution. We begin by constructing the underlined profiles U

n

in cascade, the boundary layer profiles U

cn

are then computed as a last step. We construct our profiles such that, for all fixed ε > 0, u

εapp

belongs to C

1

([0, T ] ×

R).

In what follows, we will note:

U

R,j

(t, x) := U

R,j,+

(t, x)1

(t,x)∈Ω+

R

+ U

R,j,−

(t, x)1

(t,x)∈Ω

R

. Moreover, we will note:

U

cR,j

t, x, ϕ

R

(t, x)

√ ε

:= U

cR,j,+

t, ϕ

R

(t, x)

√ ε

1

(t,x)∈Ω+

R

+U

cR,j,−

t, ϕ

R

(t, x)

√ ε

1

(t,x)∈Ω

R

.

(8)

Note well that the dependence of U

cR,j

in x is a bit subtle. Actually, U

cR,j

is piecewise constant with respect to x on each side of Γ

R

, which explains that U

cn,L,+

and U

cn,L,−

have no direct dependency in x. Due to their particular meaning, we prefer denoting the profiles U

R,0

and U

L,0

by u

R

and u

L

. Let us note H

R

the differential operator

H

R

:= ∂

t

+ ∂

x

(a

R

.) and P

R

the differential operator

P

R

:= ∂

t

+ a

R

x

− (∂

x

ϕ)

2

2θ

R

+ ∂

x

a

R

. We have

L

εR

u

εR,app

t, x, ϕ

R

(t, x)

√ ε

=

M+1

X

j=0

L

R,j

t, x, ϕ

R

(t, x)

√ ε

ε

j2

where

L

R,0

= H

R

u

R

+ P

R

U

R,0c

,

L

R,1

= H

R

U

R,1

+ P

R

U

R,1c

− 2(∂

x

ϕ)∂

x

θR

+ (∂

x2

ϕ)∂

θR

U

R,0c

, and, for 2 ≤ j ≤ M − 1, we get:

L

R,j

= H

R

U

R,j

+P

R

U

R,jc

− 2(∂

x

ϕ)∂

x

θR

+ (∂

x2

ϕ)∂

θR

U

R,j−1c

−∂

x2

U

R,j−2

−∂

x2

U

R,j−2c

, L

R,M

= P

R

U

R,Mc

− 2(∂

x

ϕ)∂

x

θR

+ (∂

x2

ϕ)∂

θR

U

R,M−1c

−∂

x2

U

R,M−2

−∂

x2

U

R,Mc −2

, L

R,M+1

= − 2(∂

x

ϕ)∂

x

θR

+ (∂

x2

ϕ)∂

θR

U

R,Mc

− ∂

x2

U

R,M−1

− ∂

x2

U

R,Mc −1

. Symmetrically, there holds:

L

εL

u

εL,app

t, x, ϕ

L

(t, x)

√ ε

=

M+1

X

j=0

L

L,j

t, x, ϕ

L

(t, x)

√ ε

ε

j2

where, for instance, L

L,2

is given by:

L

L,2

= H

L

U

L,2

+P

L

U

L,2c

− 2(∂

x

ϕ

L

)∂

x

θL

+ (∂

x2

ϕ

L

)∂

θL

U

L,1c

−∂

x2

u

L

−∂

x2

U

L,0c

, where H

L

is defined by:

H

L

:= ∂

t

+ ∂

x

(a

L

.) and P

L

is given by:

P

L

:= ∂

t

+ a

L

x

− (∂

x

ϕ

L

)

2

θ2

L

+ ∂

x

a

L

.

(9)

Plugging u

εL,app

and u

εR,app

in the problem (2.2) and identifying the terms with the same scale in ε, making then |θ

L

| and |θ

R

| tend to infinity, we obtain the profiles equations satisfied by the underlined profiles. Let us begin by writing the equations satisfied by U

L,j

and U

R,j

for all 0 ≤ j ≤ M − 1.

Thanks to the transmission conditions we had on the viscous problem, we get:

(

u

L,+

|

x=0

− u

R,−

|

x=0

= 0, a

L

u

L,+

|

x=0

− a

R

u

R,−

|

x=0

= 0.

This linear system being invertible, we get then the homogeneous Dirichlet boundary condition:

u

L

|

x=0

= u

R

|

x=0

= 0.

We can split these equations into three well-posed problems:





t

u

R,−

+ ∂

x

(a

R

u

R,−

) = f

R,−

, (t, x) ∈ Ω

R

,

t

u

L,+

+ ∂

x

(a

L

u

L,+

) = f

L,+

, (t, x) ∈ Ω

+L

, u

L,+

|

x=0

= u

R,−

|

x=0

= 0,

(

t

u

R,+

+ ∂

x

(a

R

u

R,+

) = f

R,+

, (t, x) ∈ Ω

+R

, u

R

|

t=0

= h

R

,

(

t

u

L,−

+ ∂

x

(a

L

u

L,−

) = f

L,−

, (t, x) ∈ Ω

L

, u

L

|

t=0

= h

L

.

Since these equations are well-posed, the function u is now perfectly defined.

Let us go on with the construction of the next profiles. U

R,1

and U

L,1

are defined by:





t

U

1,R,−

+ ∂

x

(a

R

U

1,R,−

) = 0, (t, x) ∈ Ω

R

,

t

U

1,L,+

+ ∂

x

(a

L

U

1,L,+

) = 0, (t, x) ∈ Ω

+L

, U

1,L,+

|

x=0

= U

1,R,−

|

x=0

= 0 .

Thus U

1,R,−

= 0 and U

1,L,+

= 0.

(

t

U

1,R,+

+ ∂

x

(a

R

U

1,R,+

) = 0, (t, x) ∈ Ω

+R

, U

1,R,+

|

t=0

= 0 ,

(

t

U

1,L,−

+ ∂

x

(a

L

U

1,L,−

) = 0, (t, x) ∈ Ω

T,L

,

U

1,L,−

|

t=0

= 0 .

(10)

Hence U

1,R,+

= 0 and U

1,L,−

= 0. Actually, we see by induction that for all n ∈

N,

we have U

±2n+1,R,±

= 0 and U

2n+1,L,±

= 0. On the other hand for n ∈

N

, the profiles U

2n,L,±

and U

2n,R,±

are given by the following well-posed hyperbolic problems.









t

U

2n,R,−

+ ∂

x

(a

R

U

2n,R,−

) = ∂

x2

U

2n−2,R,−

, (t, x) ∈ Ω

T,R

,

t

U

2n,L,+

+ ∂

x

(a

L

U

2n,L,+

) = ∂

x2

U

2n−2,L,+

, (t, x) ∈ Ω

+T,L

,

U

2n,L,+

|

x=0

U

2n,R,−

|

x=0

= M

−1

0

− ∂

x

U

2n−2,R,−

|

x=0

− ∂

x

U

2n,L,+

|

x=0

where M :=

1 −1 a

L

|

x=0

−a

R

|

x=0

; remark that the matrix M is nonsin- gular since a

L

|

x=0

− a

R

|

x=0

< 0.

(

t

U

2n,R,+

+ ∂

x

(a

R

U

2n,R,+

) = ∂

x2

U

2n−2,R,+

, (t, x) ∈ Ω

+T,R

, U

2n,R,+

|

t=0

= 0 .

(

t

U

2n,L,−

+ ∂

x

(a

L

U

2n,L,−

) = ∂

x2

U

2n−2,L,−

, (t, x) ∈ Ω

T,L

, U

2n,L,−

|

t=0

= 0 .

In conclusion, all the profiles U

n

are constructed by induction.

We turn now to the construction of the boundary layer profiles U

L,j,±c

(t, θ

L

) and U

R,j,±c

(t, θ

R

). We will use the relations imposed on the profiles by the transmission conditions: [u

εapp

]

ΓR

= 0, [∂

x

u

εapp

]

ΓR

= 0, [u

εapp

]

ΓL

= 0, and [∂

x

u

εapp

]

ΓL

= 0; [u

εapp

]

ΓR

stands for the jump of u

εapp

through Γ

R

defined, for all t ∈ [0, T ] by:

[u

εapp

]

ΓR

(t) := lim

x→xR(t),x>xR(t)

u

εapp

t, x, ϕ

R

(t, x)

√ ε

− lim

x→xR(t),x<xR(t)

u

εapp

t, x, ϕ

R

(t, x)

√ ε

,

where we recall that x

R

(t) is the unique x such that (t, x) ∈ Γ

R

. [u

εapp

]

ΓL

(t) is defined the same way. Because u

εapp

belongs to C

1

((0, T ) ×

R

), for all 0 ≤ j ≤ M, we have:

[U

L,jc

]

L

= −[U

L,j

]

ΓL

,

[U

R,jc

]

R

= −[U

R,j

]

ΓR

.

(11)

Let [U

R,j

]

ΓR

be given, for all t ∈ (0, T ), by:

[U

R,j

]

ΓR

(t) = lim

x→xR(t),x>xR(t)

U

R,j,+

(t, x) − lim

x→xR(t),x<xR(t)

U

R,j,−

(t, x) and [U

R,jc

]

R

be defined, for all t ∈ (0, T ), by:

[U

R,jc

]

R

(t) = lim

θR→0+

U

R,j,+c

(t, θ

R

) − lim

θR→0

U

R,j,−c

(t, θ

R

).

To avoid writing the exact symmetric equations on {x > 0} and {x < 0}, let us only proceed with the construction of the boundary layer profiles U

R,j,±c

. Referring to the computations above, for all 1 ≤ j ≤ M + 1, the following quantity must not have any Dirac measure in it:

x

θR

U

R,j−1c

+ 1

2(∂

x

ϕ) ∂

x

(∂

x

(U

R,j−2

+ U

R,j−2c

)),

Our first boundary condition: [U

L,jc

]

L

= −[U

L,j

]

ΓL

, ensures that, even if

x

(U

R,j−2

+ U

R,j−2c

) is, in general, discontinuous on Γ

T

, it has no Dirac Measure. ∂

x

(∂

x

(U

R,j−2

+ U

R,j−2c

)) is the derivative of such a function and thus has a Dirac Measure. Let us describe this singularity: if we fix t = t

0

, the Dirac measure forming is

[∂

x

U

R,j−2

]|

x=xR(t0)

+ [∂

x

U

R,j−2c

]

R

(t

0

)

δ

x=xR(t0)

. Hence the Dirac measure forming in

2(∂1

xϕ)

x

(∂

x

(U

R,j−2

+ U

R,j−2c

)) is 1

2(∂

x

ϕ)|

x=xR(t0)

[∂

x

U

R,j−2

(t

0

)]|

x=xR(t0)

+ [∂

x

U

R,j−2c

(t

0

)]

R

δ

x=xR(t0)

.

where [ω]|

x=x

R(t0)

= lim

x→xR(t0),x>xR(t0)

ω − lim

x→xR(t0),x<xR(t0)

ω.

On the other hand, if ∂

θR

U

R,j−1c

is discontinuous through Γ

R

, ∂

x

θR

U

R,j−1c

has a Dirac measure given, for t = t

0

by:

[∂

θR

U

R,j−1c

]

R

δ

x=xR(t0)

.

The game is to construct the boundary layer profiles such that the sum of the two Dirac measures cancel. As a result, the second boundary condition we get is that, ∀t ∈ (0, T ) :

[∂

θR

U

R,j−1c

]

R

(t) = − 1

2(∂

x

ϕ)|

x=xR(t)

[∂

x

U

R,j−2

]

ΓR

(t) + [∂

x

U

R,j−2c

(t)]

R

.

(12)

The profiles U

R,0,+c

and U

R,0,−c

are solution of the following heat equation:





















t

U

R,0,+c

− (∂

x

ϕ

R

)

2

θ2R

U

R,0,+c

+ (∂

x

a

R

)U

R,0,+c

= 0 t ∈ (0, T ), {θ

R

> 0},

t

U

R,0,−c

− (∂

x

ϕ

R

)

2

θ2R

U

R,0,−c

+ (∂

x

a

R

)U

R,j,−c

= 0 t ∈ (0, T ), {θ

R

< 0}, [U

R,0c

]

R

(t) = −[u

R

]

ΓR

, ∀t ∈ (0, T ),

[∂

θR

U

R,jc

]

R

(t) = 0, ∀t ∈ (0, T ), U

R,j,+c

|

t=0

= 0,

U

R,j,−c

|

t=0

= 0 .

Note well that, since [u

R

]

ΓR

6= 0, the profiles U

R,0c

and U

L,0c

are not equal to zero.

For all 1 ≤ j ≤ M, the profiles U

R,j,+c

and U

R,j,−c

are given by:

























t

U

R,j,+c

− (∂

x

ϕ

R

)

2

θ2R

U

R,j,+c

+ (∂

x

a

R

)U

R,j,+c

= (∂

x2

ϕ

R

)∂

θR

U

R,j−1,+c

t ∈ (0, T ), {θ

R

> 0},

t

U

R,j,−c

− (∂

x

ϕ

R

)

2

θ2R

U

R,j,−c

+ (∂

x

a

R

)U

R,j,−c

= (∂

x2

ϕ

R

)∂

θR

U

R,j−1,−c

t ∈ (0, T ), {θ

R

< 0}, [U

R,jc

]

R

(t) = −[U

R,j

]

ΓR

, ∀t ∈ (0, T ),

[∂

θR

U

R,jc

]

R

(t) = − 1

2(∂

x

ϕ)|

x=xR(t)

[∂

x

U

R,j−1

(t)]

ΓR

(t) + [∂

x

U

R,j−1c

(t)]

R

, ∀t ∈ (0, T ), U

R,j,+c

|

t=0

= 0,

U

R,j,−c

|

t=0

= 0 .

Let us now prove the well-posedness of these problems. We take ψ

R,j

in H

((0, T ) ×

R

) such that

R,j

]

R

= −[U

R,j

]

ΓR

, and

[∂

θR

ψ

R,j

]

R

(t) = − 1

2(∂

x

ϕ)|

x=xR(t)

[∂

x

U

R,j−1

(t)]

ΓR

(t) + [∂

x

U

R,j−1c

(t)]

R

.

We can then compute U

R,jc

:= U

R,j,+c

1

θR>0

+ U

R,j,−c

1

θR<0

by:

U

R,jc

:= ψ

R,j

+ V

R,jc

. V

R,jc

is then the solution of the classical heat equation:

(

t

V

R,jc

− (∂

x

ϕ

R

)

2

θ2R

)V

R,jc

+ (∂

x

a

R

)V

R,jc

= ϕ

R,j

, (t, θ

R

) ∈ (0, T ) ×

R

,

V

R,jc

|

t=0

= 0 .

(13)

and ϕ

R,j

is given by:

ϕ

R,j

:= − ∂

t

ψ

R,j

− (∂

x

ϕ

R

)

2

θ2

R

ψ

R,j

+ (∂

x

a

R

R,j

+ (∂

x2

ϕ

R

)∂

θR

U

R,j−1c

. The profiles can thus be constructed by induction using the scheme just in- troduced.

We will now prove stability estimates.

We define the error w

ε

:= u

εapp

− u

ε

. Let us denote by w

ε±

the restriction of w

ε

to ±x > 0. (w

ε+

, w

ε−

) is then solution of the transmission problem:





















t

w

ε+

+ ∂

x

(a

R

w

ε+

) − ε∂

x2

w

ε+

= ε

M

R

ε+

, x > 0, t ∈ [0, T ],

t

w

ε−

+ ∂

x

(a

L

w

ε−

) − ε∂

x2

w

ε−

= ε

M

R

ε−

, x < 0, t ∈ [0, T ], w

ε+

|

x=0+

− w

ε−

|

x=0

= 0,

a

R

w

ε+

|

x=0+

− ε∂

x

w

ε+

|

x=0+

= a

L

w

ε−

|

x=0

− ε∂

x

w

ε−

|

x=0

, w

ε+

|

t=0

= 0, ∀x > 0,

w

ε−

|

t=0

= 0, ∀x < 0.

By construction of our approximate solution, R

ε

belongs to L

([0, T ] : L

2

(R)). Multiplying by the solution and integrating by parts, we get, for {x > 0} :

1 2

d

dt kw

ε+

k

2L2(R+)

+ εk∂

x

w

ε+

k

2L2(R+)

− a

R

|

x=0

2 w

ε+

|

x=02

+ εw

ε+

x

w

ε+

|

x=0

= ε

M Z

0

R

ε+

w

ε+

dx − 2

Z

0

x

a

R

(w

ε+

)

2

dx.

Note that:

− a

R

|

x=0

2 w

ε+

|

x=02

+ εw

ε+

x

w

ε+

|

x=0

= a

R

|

x=0

2 w

ε+

|

x=02

− w

ε+

|

x=0

a

R

w

ε+

|

x=0

− ε∂

x

w

ε+

|

x=0

. And, for {x < 0}, we have:

1 2

d

dt kw

ε−

k

2L2(R)

+ εk∂

x

w

ε−

k

2L2(R)

+ a

L

|

x=0

2 w

ε−

|

x=02

− εw

ε−

x

w

ε−

|

x=0

= ε

M Z 0

−∞

R

ε−

w

ε−

dx − 2

Z 0

−∞

x

a

L

(w

ε−

)

2

dx.

(14)

Note that:

a

L

|

x=0

2 w

ε−

|

x=02

− εw

ε−

x

w

ε−

|

x=0

= − a

L

|

x=0

2 w

ε−

|

x=02

+ w

ε−

|

x=0

a

L

w

ε−

|

x=0

− ε∂

x

w

ε−

|

x=0

. Thanks to our boundary condition, there holds:

w

ε+

|

x=0

a

R

w

ε+

|

x=0

− ε∂

x

w

ε+

|

x=0

= w

ε−

|

x=0

a

L

w

ε−

|

x=0

− ε∂

x

w

ε−

|

x=0

Thus, by adding our estimates, we obtain:

1 2

d

dt kw

ε

k

2L2(R)

+ εk∂

x

w

ε

k

2L2(R)

+ a

R

|

x=0

− a

L

|

x=0

2 (w

ε

|

x=0

)

2

= ε

M Z

−∞

R

ε

w

ε

dx − 2

Z

0

x

a

R

(w

ε+

)

2

dx − 2

Z 0

−∞

x

a

L

(w

ε−

)

2

dx.

Z

−∞

R

ε

w

ε

dx − 2

Z

0

x

a

R

(w

ε+

)

2

dx − 2

Z 0

−∞

x

a

L

(w

ε−

)

2

dx

≤ 1

2 kR

ε

k

2L2(R)

+Ckw

ε

k

2L2(R)

, where C =

12

+ 2M ax

sup

(t,x)∈ΩL

|∂

x

a

L

|, sup

(t,x)∈ΩR

|∂

x

a

R

| .

Since a

R

|

x=0

> 0 and a

L

|

x=0

< 0, by Gronwall Lemma, we get the simplified estimate:

kw

ε

k

2L2(R)

(t) ≤ 1 2 ε

M

Z T 0

e

C(t−s)

kR

ε

k

2L2(R)

(s) ds.

Constructing the profiles up to order M = 1, we get then that there is c > 0, independent of ε, such that:

kw

ε

k

2L([0,T]:L2(R))

≤ cε, thus achieving our proof.

2

3 Treatment of the ingoing case.

Let us now introduce our second result. Our second result concerns the case where, for all t ∈ [0, T ], the coefficient a satisfies:

a(t, 0

+

) < 0,

a(t, 0

) > 0.

(15)

During the study of a similar problem, Poupaud and Rascle show in [9]

the formation of a Dirac measure on {x = 0} for their solution. We show that a Dirac-measure also forms in the small viscosity limit. We give an asymptotic expansion of the solution u

ε

of (1.3), which shows explicitely the convergence to the generalized measure-valued solution u. The main result is stated in Corollary 3.3 . The problem we consider here appears as one very simple example of the arising of a ” δ-measure” in the vanishing viscosity limit. Note that, by using viscous approaches as well, Joseph ([6]) and Tan, Zhang , Zheng ([10]) describe an analogous phenomenon, called δ-shockwave. We will denote by [θ]|

x=0

the jump of θ through {x = 0} i.e

θ(., 0

+

) − θ(., 0

).

A piecewise smooth u

ε

is solution of (1.3) iff its restrictions to ±x > 0 satisfies the equation on ±x > 0 and

[a(., x)u

ε

− ε∂

x

u

ε

]|

x=0

= 0,

which is the corresponding Rankine-Hugoniot condition. The hyperbolic- parabolic problem (1.3) reformulates then as the following transmission problem:

(3.1)





















t

u

ε+

+ ∂

x

(a

+

u

ε+

) − ε∂

x2

u

ε+

= f

+

, {x > 0}, t ∈ [0; T ],

t

u

ε−

+ ∂

x

(a

u

ε−

) − ε∂

x2

u

ε−

= f

, {x < 0}, t ∈ [0; T ], u

ε+

|

x=0+

− u

ε−

|

x=0

= 0,

a

+

u

ε+

|

x=0+

− ε∂

x

u

ε+

|

x=0+

= a

u

ε−

|

x=0

− ε∂

x

u

ε−

|

x=0

, u

ε+

|

t=0

= h

+

,

u

ε−

|

t=0

= h

,

with u

ε+

= u

ε

|

x>0

, a

+

= a|

x>0

, f

+

= f |

x>0

, h

+

= h|

x>0

and u

ε−

= u

ε

|

x<0

, a

= a|

x<0

, f

= f |

x<0

, h

= h|

x<0

. Problem (3.1) can be reformulated as the doubled problem on a half-space:

(3.2)





t

u ˜

ε

+ ∂

x

( ˜ A˜ u

ε

) − ε∂

x2

u ˜

ε

= ˜ f (t, x), {x > 0}, t ∈ [0; T ], M

c

u ˜

ε

|

x=0

= 0,

˜

u

ε

|

t=0

= ˜ h .

Let us precise how problem (3.2) is deduced from problem (3.1): ˜ u

ε

is a two dimensional vector which first component [resp second component] is u

ε+

(t, x) [resp u

ε−

(t, −x)]. ˜ A is defined by:

A(t, x) = ˜

a

+

(t, x) 0 0 −a

(t, −x)

,

Références

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