Uniform decay rates for parabolic conservation laws

Uniform decay rates for parabolic conservation laws

UNIFORIM DECAY RATES FOR PARABOLIC MARIA Department of Mathematics. Duke (Received in reoised form 17 ,Vouember Key words and phrases: Paraboli...

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UNIFORIM

DECAY

RATES

FOR PARABOLIC MARIA

Department

of Mathematics.

Duke

(Received in reoised form 17 ,Vouember Key words and phrases: Parabolic

conservation

E.

CONSERVATION

LAWS

SCHONBEK

University.

Durham,

NC 27706.

U.S.A.

1983; received for publication 21 October 1985) laws, decay

rates.

1. INTRODUCTION

paper we establish optimal uniform rates of decay for solutions of the Cauchy problem with large data to scalar parabolic conservation laws in several space dimensions, IN THIS

where the II,, are constants, and to parabolic systems of conservation

laws

$ + divf(L1) = Au,

(1.2)

where u = U(X, t) E RP, x E R” and f, = (f’, . . . ,fp) with f: RF- R”. Equations of this type arise in continuum mechanics where they serve as models for elastic solids and ideal gases. In an earlier paper [j], we have shown that solutions of the scalar equation (1.1) decay in L’ and L’ with a rate of ten”. It is not difficult to verify that t -n:’ is the optimal rate in L’. On the other hand, one can expect the faster rate of ten,’ m ’ L” based on an analysis of the heat equation. In Section 2, we shall show that solutions of the scalar equation (1.1) decay at the optimal rates t -n “‘-‘;P) in LP for 1 < p < x and at the optimal rate of t-“/I in L”. In order to establish the decay rate we derive an entropy inequality for the function up. Applying Fourier analysis yields an inequality for the Fourier transform of an appropriate power depending on p. A subdivision of the frequency domain into two time dependent subspaces leads to the desired decay rate. In Sections 3 and 4 we show that periodic solutions of system (1.2) decay exponentially in H” and L” for a class of general flux functionsfi With regard to background we recall that decay without a rate of solutions of (1.2) in one spatial dimension was established in [5]. In the present paper we first obtain the exponential decay in the L?-norm. We derive an entropy inequality which expresses the dissipative mechanism present in (1.2). The combination of Poincare’s inequality with this entropy inequality gives rise to a linear differential inequality from which the rate of decay is established. To obtain the H” decay a family of generalized entropy inequalities for higher order spatial derivatives will be derived and combined with Poincare’s inequality. This process leads to a differential inequality in a weighted H” norm from which the exponential decay will follow. The H” decay together with a standard Sobolev inequality yields the L” decay. 2.

DECAY

RATES

FOR

SOLUTIONS

OF THE

SCALAR

EQUATIOS

In this section. we show that the solutions of the Cauchy problem for the consemation 943

law

94-t

M. E. SCHONBEK

(1.1) decay at the optimal rate of f-” I”- ’ pi m Lp and at the optimal rate of r-n’z in Lx. We will first consider the decay rate of the solutions in Lp with 1


j

i j=l In order solutions of order

to obtain the desired in a special sequence

=

p!

!

and hence

lim CJP = x. P-r

rate of decay in L”, we need to establish the decay rate for the of Lp norms with p = 2’. In this case the coefficients C, will be

that is the growth of the coefficients C, is slow enough. We now state two theorems, the first one establishes the decay rate of the solutions of (1.1) in LP for all p 2 1, the second one establishes the decay rate in LP for p = 2’ with s 2 1. The techniques used in the proof of both theorems are similar. Since the arguments for the second proof contain those needed for the first proof we shall only present the proof of the second theorem. For existence of solutions of (1.1) we refer the reader to [3]. THEOREM 2.1. Let F’ E C’, ug E L’ n C’ fl H’(R”).

u,) then for 1 6p

If u is a solution

of (1.1) with initial

data

If u is a solution

of (1.1) with initial

data

< 3~

where

THEOREM 2.2. Let F’ E Cl, u(, E L’ f7 C1 f? /ii(

u,, then for all p = 2’ with s 2 1 lL’(4LP

c A;‘” (r + 1) -n/2(1 - i/PI.

(2.1)

Here A, defined

= 2’rBhs ,:pzp (1 + ~L&~)

with

and

B

by s-l h, = 2 2i = 2’ - 1, ri = 0, rs = (s - l)(n/2

+ 1) i 2r,_, , B = 4 coo nni2,

j=O

where

h,, rr

o0 is the measure

of the n dimensional

unit sphere.

945

Uniform decay rates for parabolic conservation laws

Proof.

we let iVp = ,ma: (1 + ju Olt,). By using a linear change - -P of independent variables, one can reduce the general constant coefficient elliptic operator on the right-hand side of (1.1) to the Laplacian while preserving the general divergence structure of the equation. Therefore we shall work with the equation For notational

convenience,

u, + jt $(4 where the p will be in C’. The proof of (2.1) follows the one presented in [5].

by induction.

= Au

The first step corresponding

(2.2)

to s = 1 is similar

to

Step 1. By energy methods, we derive an equation which connects the L’ norm of the solution with the L2 norm of its gradient. An application of Plancherel’s theorem and a decomposition of the frequency domain into two time dependent subspaces yields a first order differential inequality for the L’ norm of the Fourier transform of the solution. The time dependent subspaces are an n-sphere S of radius R=

2-In 12 i t+ 11

and its complement. This decomposition allows us to bound the inhomogeneous term of the differential inequality by the volume of S yielding a new differential inequality from which the desired L’ rate of decay follows. To begin with, we multiply equation (2.2) by u and integrate by parts to obtain

(2.3) The second

integral

can be rewritten

as 2

where infinity,

qj(u)

=

Jo"

it follows

j Rn

Zd

q'(u)

dx,

axj

f’(s) ds. Recalling that u vanishes at infinity since the initial data vanishes that the second integral is equal to zero. Hence (2.3) is equal to

at

(2.4) Plancherel’s

where

theorem

yields

916

.Ll.E. SCHONBEK

Hence

Reordering

the terms

hIultiplying

both sides of the last inequality

Recalling

yields

that the solutions

by the integrating

of (1.1) satisfy an L’ contraction ILlILl c

it follows

that iris, s ‘I~,);~L. Therefore.

and integrating

the right side it follo\vs

C

:LLo I,l(f

+

1)”

Plancherel’s

theorem

j R” Recalling

yields

sphere

of radius

one.

Integrating

the last

that

jl1012dyi (t + 1))” + ~L~&co,,~“~‘(~ + l)-”

that

that

[2], i.e.

ln 1 n(r + l)_’ - -n C2r+l [

A , = Bl\’ 3 = &,&’ it follows

principle

that

again it follows

ll/’ du d (j

(t + I)” gives

IAL1

the last inequality

lvhere wO is the measure of the n-dimensional inequality kvith respect to time yields

Using

factor

max (1 + 1~~12~) lSrS2

2

(2.5)

Uniform

decay

rates for parabolic

conservation

laws

947

so that (2.5) yields

Step 2. Suppose

now that inequality

i R”

(2.1) holds for q = T1. ILL/~dx c A&

that is

+ l)-” 2(‘J-1).

(2.6)

To show that (2.1) holds with p = 2’ we need to derive an equation similar to (2.3). This equation will connect the L’ norm of the pth power of the solution with the L’ norm of the qth power of the gradient of the solution. By Plancherel’s theorem and some manipulations similar to the ones used in the case p = 2 we obtain a differential inequality for the L’ norm of the qth power of the Fourier transform of the solution. Here again the frequency domain will be divided into two time dependent subspaces: the n-sphere S, with radius I 2

and its complement S;. As in the L2 case, the inhomogeneous term will be bounded by the volume of S, in order to derive a new differential inequality from where the desired rate of decay will be obtained. We start by multiplying equation (2.2) by up-’ and integrating in space and time to obtain

dJ- lujp dx = -p zf R”

J”~4$~w~-P

j

R"

up- ’ au cl\.

R"

The same reasoning as in step one shows that the first integral on the right-hand hence after an integration by parts on the second integral. vve have

dj zf

lulpdx =

-(P

- l)P i I=1

R”

Noting

j

ll?-211;,

side vanishes,

dx.

R”

that

It follows

that

where the last inequality follows sincep(p to the last inequality yields

- l)q-’

3 1 fors > 2. Applying

Plancherel’s

theorem

hi. E. SCHONBEK

948

where

we have let w = tiq. Let S, = [g: ,s”, < ($)I’:].

We now split the integral on the right-hand side of (2.7) into an integral S; and we bound iei on S; by the radius of S, obtaining

The last inequality

is now multiplied

-$+lPjR”

/WI?

by the integrating d;‘s(t+

factor

over S, and one over

(I + 1)“q

1)"9

Hence

Integrating

the right-hand

The inductive

hypothesis

side yields

(2.6) yields the following

bound

for iwl$:

1~14dx)‘sA;(t+

Iwit < (j

I)-“(q-‘1

R” where

Ai

the bound

where

=

2?rJ-1B?h

S--I

Ni.

Noting

that 2h,_,

= h, - 1 and IV: < 4N,, it follows

by (2.8) and

for /WI: that

(Y= 2r,_ 1 + (n/2 + 1) (s - 1). Since 4n”‘* o. = B and 2/(n + 2) G 2/3 it follows

;[(i+ We now integrate

1)“q

jRn IU’112dj]

in time and use Plancherel’s

(2 + 1)"q j

theorem

1)“/2-1. to obtain

juIpdx s j juolP dx + ;A,([

R”

Since A,/3

=+A&+

- 1) it follows

(uIP d_xs A, (t + 1) -“%j R”

+ l)“?

R”

> ju o1ALPand n/2 - nq = -n/2(p

that

from (2.9) that l)

(2.9)

Uniform

This last inequality

completes

decay

rates for parabolic

the proof of theorem

conservation

laws

9-19

2.2.

COROLLARY 2.1.Let fj E C’, u. E L’ fl H’ n C’(P).

If u is a solution

of (1.1) with initial

data u. then

where A = 2”‘2C’BN,, with N, = ,mryz (1 + IuoI,_,). Proof. By theorem

2.2, we have for p = 2’ lu(t)lx

Hence

=

!i~:

(1

lulP

dx)

‘If

s

(A,)‘/P(t

!Lir

+ l)-““.

to show that lim (Ap)“p = A. For this we note that J-+X

it suffices

r, = [(s - 1) + 2(q - s)]O = [p - (s + l)]O where

q = s’-l

and 8 = n/2 + 1. Hence (AP)r/P c 2(‘-(S+ i)k’)eBr-i/P

,Tra2. (1 +

I~oM

so that lim (AP)ljP x-+x

= 2e BN,

= A.

In the next corollary we establish optimal decay rates for the solutions p 2 1. The estimate that will be obtained is of the type

of (1.1) in LP for all

s c,v,(1+ f)-n.‘311‘PI. ILl(f)lLP This result differs from the one obtained in theorem 2.1 since here the coefficient c is independent of p and the estimate depends on all the L’ norms of the initial data. not only on the ones with r sp.

COROLLARY 2.2.Let fj and u. be as in theorem

2.1. If u is a solution

of (1.1) with initial

data

uo, then

l4)l LPs 2”BN,(l + 4-“/2(‘-‘lP). Proof. The proof is a consequence of theorem 2.2, corollary 2.1 and the following Sobolev interpolation inequality for Lp spaces: Let p E (2, x) then

standard

I(P,-?),lP. I4 LPz=lui’/“l L’ uL

Applying

this inequality

in our case yields

(1w where that

p = -n/2(1

- 1/2)2/p

q’” < /#P&P-?)iP(f

+ (p - 2)/2 = -n/2(1

+

- l/p).

1)s

A simple

calculation

will show

950

E.

hl.

SCHONBEK

3. L’ RATES OF DECAY

In this section of the form

we consider

the Cauchy

problem

11, + divf((u)

FOR SYSTEMS

for systems

of parabolic

conservation

laws

= Au (3.1)

n(x, 0) = un(x) where u = U(X. t) f RP, x E R”. u. is smooth and f = (f’, . show that periodic solutions of (3.1) decay at an exponential supposed that the associated system u, + divf(u)

,fp) with?:

RP-+ R” smooth. We rate in the L’ norm. It will be

= 0

(3.2)

is hyperbolic and admits a uniformly convex entropy in the sense of Lax [4]. We recall that a pair of functions 7, q where 7: RP, q = (ql, . . , q,J and q,: RP- R is an entropy flux pair if all smooth solutions of (3.2) satisfy the additional conservation law q(u), + div q(u) = 0. The last equation

is equivalent

to the compatibility Vq .

where fl = (f; _ff, . ,f;). Condition and multiplying (3.1) by Vr],

(3.3)

condition

Tf, = vqi,

(3.4) follows by carrying

(3.3) out the differentiation

in (3.3)

n cqu,

+ c, Oq’u,, = 0

V~U,

+ C

]=I n

V17VfjU.,.

/=1

We note that if ‘I, q is an entropy flux pair for the hyperbolic of (3.1) satisfy the additional equation n qr + divq

= Aq - 2 i=

In this section satisfy

the systems

under consideration

system

(3.5)

V?qu:,. 1

will admit uniformly

V’@

(3.2) then all solutions

convex

entropies,

i.e. they

2 Si;“i?

for some S > 0. This class of systems include symmetric systems, that is systems for which the flux function f arises from a gradient of a scalar potential @, and f = V@. Here r](u) = Xuj/2 serves as an entropy [4]. The proof of the decay rate uses energy estimates in conjunction with Poincare’s inequality. Specifically, we show that if system (3.1) admits an entropy ‘I, then all smooth periodic solutions satisfy an integral inequality of the form

IK

q(u),&<

-&

(3.6) IK

Uniform

where ff > 0. The set K is defined of 11, i.e.

decay

rates for parabolic

conssrvarion

laws

by ={x: 0 c x, < L,}, L, is the period

u(x + L,e,, t) = u(x, t)

951

of the ith component

i=l.....n

(3.7)

with e, the ith element of the canonical basis of R”. e.g. ez = (0, 1, 0, .. ,0). In vvhat follows we will say that u is L-periodic if L = (L.,, . , L,) and 11satisfies (3.7). The exponential decay of solutions for systems (3.1), admitting a uniformly convex entropy rl which satisfies n(u) 3 c(u)‘, c > 0, will follow by (3.6) and Poincare’s inequality. We first establish a theorem on the decay for functions satisfying the integral inequality (3.6). We then show that solutions of (3.1) satisfy (3.6) and therefore decay. THEOREM 3.1. Let 17:RP--, R be an arbitrary uniformly convex function satisfying V(U) 5 cjc~1’, c > 0. Let x E R”. t E R,. Suppose that u = u(x, I) E RP is a smooth L-periodic function with vanishing average ti, that is

fi=h i K Ll(x, r) dx = 0. where k = {x:x = (x1.. ..,x,), 0
where

M and y depend

/KI = II;=,

L,. If u satisfies

the

integral

only on ‘7, n, L and u(x, 0).

Proof. From (3.6) and the uniform

convexity

of 17it follows that

(3.8) side of (3.7), Poincare’s inequality will be used. For completeness To bound the right-hand we recall Poincare’s inequality: Let u E R” be a L-periodic Ci function with average

then

(3.9) only on n and L. Let u = u and combine

where

p depends

where

N = p&S. By hypothesis

n 2 c[uI’, hence

(3.8) with (3.9) to obtain

if we let y = c-*N it follows

that

952

An integration

M.

E. SCHOXBEK

in time yields

I

q(u) dx C ewyr iK

K

Hence using the hypothesis

rp(“, 0) dx.

‘I 2 c/1112again yields IK

Iu/’ dr G M exp( - yt).

In the remainder of the paper we suppose that U,,(X)andfsatisfy general conditions insuring the existence of smooth solutions u of (3.1) with initial data uO(x). The next theorem and corollary show that periodic solutions of (3.1) satisfy (3.6) and hence decay exponentially. THEOREM3.2. Let PJ:RP+ R be an entropy corresponding to the system (3.1) and let u be an L-periodic smooth solution, then u satisfies inequality (3.6). Proof. Integrating

equation (3.5) in space yields

d r](u) du + divg(u)dr=j~A~d~-j~~~~~iiidr dr i K iK where K is defined as in theorem 3.1. The periodicity d V(U) du = dr i K

i

of 11yields C’~U;~ du.

i K 1=i

COROLL.&RY3.1. Let Us be a smooth L-periodic function. Let k be defined as in theorem 3.1. Suppose (3.1) admits a uniformly convex entropy q which satisfies q(u) b c/l~:~.c > 0. If u is a smooth solution of (3.1) with initial data uo(x). then [u(r) - ti/L’(Ic) 4 M exp( - yt). where 12=

& I K U(X, f) dr

and M and y depend only on llo, 17,L, and n. Proof. The uniqueness of solutions for system (3.1) and the L-periodicity of 14;)imply the L-periodicity of u. We first show that U is constant. Integrating (3.1) in space yields

%~K~~d~=j~L~,,=-~Kdivfdr+~KA~dr. The right-hand side vanishes by the periodicity of u and hence 12is constant. Without loss of generality we suppose ti = 0. If not, let u = LL - ti,then u satisfies u, + divg(u) = Au, where g(u) = f(u + ~2). Hence corollary 3.1 follows from theorems 3.1 and 3.2.

Uniform decay rates for parabolic conservation laws

953

Remark. The decay results obtained for periodic solutions of (3.1) are also valid for solutions in a bounded domain with zero boundary data. Example 1. In [4], Lax constructs strictly convex entropies for 2 x 2 systems. Hence corollary 3.1 can be applied to 2 x 2 systems which have solutions with a known L” a priori bound. Example 2. Navier-Stokes

equations. div I( = 0 u, + (u . V)u = -VP + vhu

v>o

(3.10)

u(x, 0) = &l(x) where u = u(x, t) E R” , x E R”, t E R,. The functions Us and p(x, t) are smooth and Lperiodic. In the case n = 2, it is known that system (3.10) has smooth solutions. It is well known that such solutions satisfy the integral inequality (3.6) with

specifically they satisfy [ Iu/2 dx = -2v An easy computation

/ jVul’ dw

(3.11)

shows that

li=&

J

K u(x, t) dx = constant.

Hence from theorem 3.1 and (3.11) the exponential

decay follows, that is

lu(x, t) - ~21~2C M exp( - yt) where M, y depend only on uo. We note finally that under sufficient assumptions of smoothness for solutions of (3.10) in higher dimension, theorem (3.1) will give their exponential decay. 4. H” AND L’ RATES OF DECAY

In this section we show that periodic solutions of the system (3.1) decay exponentially in H” and in L”. The H” decay is obtained by combining certain generalized entropy inequalities for the higher order spatial derivatives of the solutions and Poincare’s inequality. This leads to a linear differential inequality connecting a weighted H”’ norm of the solution with an m + 1 weighted norm from where the exponential decay follows. The L” decay is obtained from the H”’ decay and a standard Sobolev inequality. Letf= (f’,. . .,f’),fj: R” + R. The following notation will be used.

where lfilz and If’l%are the usual L2 and L” norms. Let r E N and CY= (cY,, . . . , an), q E N,

954

&I.

E.

SCHONBEK

then we let

where INi = i: cr, 1=1

D”=D,;=fiD;;.

and

I=1

THEOREM 4.1. LetfE C+‘(IC’, R”). Let ll0 E C(RP) be a L-periodic function. Suppose (3.2) admits a uniformly convex entropy ‘I. satisfying q(u) 2 cu’, c > 0. If 11is a solution of (3.1) with initial data u. then

and if m > [n/2] then

x

r
where

M and y depend

Proof.

We introduce

lJD’u(l,

c Mexp(-yt),

I]

only on n, m. f and uo. the following

weighted

H’ norms

(u(t)); = i. k,,, JID'ull;s 2 0.

(-1.1)

quantities where k. o = 0, /c,,~ = 0 and the weights k,,, with s 2 1, 1 s r < s are nonnegative defined below by induction. The main step in the proof is to establish a differential inequality of the type (3.6) for the norms (4.1). Specifically we obtain an inequality connecting the rate of change in time of the s-norm with the negative of an s -I- 1 norm, that is we show (4.2) where c indicates here and below a positive constant depending only on ‘I, n, f.IL,) and the L” norm of ~1. Once (4.2) is established the H” decay will follow by Poincare’s inequality. To establish (4.2) we proceed by induction on s. For s = 0 the equality is reduced to

and was established in theorem 3.1 with k,, = CYSand c = 1. We now suppose that (4.2) holds for all integers less than s and show that it holds for s. Taking the D” derivative of (3.1) with INI = s and multiplying by D”u it follows that DLudDnuj

+ D”dD”

div f (u) = D”dD”Aul

Uniform

forj=

1,. . . . p. An integration

decay

rates for parabolic

955

laws

in space yields

Integrating by parts in the second hand side gives

integral

& = - i I=1

where Schwarz’s inequality with 1cy\ = s yields

conservation

on the left-hand

j

side and in the integral

of the right-

jDn+e,l(‘j2 K

was used in the last step. Hence

adding

all derivatives

of order

N,

of the Sobolev

embedding

Hence

We will need the following theorem, [2].

lemma which is a well known consequence

LEMMA 4.1. Let u = (u’, f(0) = 0. Then ifs 2 1

. , up), uJ E Cs(R,),

; = 1,

. . , p. Suppose

f= f(rt) f C’(RP. R”),

(4.4)

IlD”f(~)ll~ s c]]Ds~& 3 where

c depends

only on s.

f

and the L” norm

Remark 1. We note that lemma in R” and dR is in C’[l].

of

K.

4.1 is also valid if the U! E C(Q)

Remark 2. Without loss of generality we can suppose f(0) = 0 otherwise we replace f by g = f - f(0). Combining inequalities (4.3) and (4.4) yields

with R a bounded

that the flux function

$‘sull; 6 - +llDscl~+ + cIID~KI~;.

domain

f in (4.1) satisfies

(4.5)

M. E. SCHONBEK

956

By inductive

hypothesis

we have that

(4.6) Now we define the k,,,. 0 < r < s and k,,,,, inequality (4.2). That is let

so that

the result

k,., = k,,,-i

O
k,,,

k J-f I.3 = &k,,,.

= $k,,,_,

of adding

(4.5)

and (1.6)

is

Hence adding (4.5) and (4.6) gives inequality (4.2). Since u is periodic and satisfies (3.1). the average

vanishes

Combining

for all N. Hence

this inequality

By hypothesis

Poincare’s

inequality

yields

with (1.2) will give

we had V(U) 2 CU?, thus

where &,I = Ik,,,, k,

= k+ 1.5

O
The constant ? can be chosen positive since the k,,,, 1 S r S s are positive. Integrating inequality (4.7) yields the exponential decay of the (I), and hence the exponential decay of the W norms follows. The L” decay is obtained from the decay in W’ and the Sobolev inequality for r < m - [n/2].

REFERENCES 1. FRIEDMAS A.. Parrial Differenrial Equations, Robert E. Krieger, Huntington, New York (1976). 2. KLMSERMW S.. Global existence for nonlinear wave equations, CPA.M XxX111, 43-101 (1980). 3. KOTLAW D. B.. Quasilinear parabolic equations and first order quasilinear conservation laws with bad Cauchy data. J. math. Analysis Applic. 35, 563-576 (1971). 4. LAX P., Shock waves and entropy, in Contributions to Nonlinear Function Analysis, (Edited by Z.ARA_\TOSELLO), Academic Press. New York (1971). 5. SCHOXBEK M., Decay of solutions to parabolic conservation laws, Communs parrial dif” Eqns 7, 449173 (1980).