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Universität Konstanz

On a contact problem in thermoelasticity with second sound

Jan Sprenger

Konstanzer Schriften in Mathematik und Informatik Nr. 245, März 2008

ISSN 1430-3558

© Fachbereich Mathematik und Statistik

© Fachbereich Informatik und Informationswissenschaft Universität Konstanz

Fach D 188, 78457 Konstanz, Germany E-Mail: preprints@informatik.uni-konstanz.de

WWW: http://www.informatik.uni-konstanz.de/Schriften/

Konstanzer Online-Publikations-System (KOPS) URL: http://www.ub.uni-konstanz.de/kops/volltexte/2008/5159/

URN: http://nbn-resolving.de/urn:nbn:de:bsz:352-opus-51592

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ON A CONTACT PROBLEM IN THERMOELASTICITY WITH SECOND SOUND

JAN SPRENGER

Abstract. We investigate the existence and stability of a thermoelastic con- tact problem with second sound. Previous results established the existence and stability of a solution of the corresponding classical system in the case of radial symmetry. However, recent works have shown that sometimes stability can be lost when the classical Fourier heat conduction is substituted by Cattaneo’s Law. We show that also in this case this substitution does indeed lead to a loss in regularity that proves to be a major problem prohibiting the transfer of the existence proof for the classical problem to the problem with second sound, leaving the existence of a solution an open question. We then prove that, if a viscoelastic term is added to the equations providing additional regularity, existence and exponential stability - the second, as can be expected, only in the case of radial symmetry - follow.

1. Introduction

We consider a thermoelastic system that can come into contact with a rigid foun- dation. In particular, consider the equations of thermoelasticity with second sound on a bounded set Ω⊂Rn with smooth boundary∂Ω = ΓC∪ΓN∪ΓD. On ΓD, the body is held fix, while on ΓN tractions are zero. On ΓC, the body is free, albeit its extension is limited by a rigid foundation. The temperature is held fixed at the en- tire boundary. If u=u(t, x),θ=θ(t, x) andq=q(t, x) describe the displacement, relative temperature and heat flow respectively, our equations take the form

t2ui−(Cijkluk,l),j−µ∂tui,jj+mijθ,j = 0 (1)

tθ+ div q+mijtui,j = 0 (2) τ0tqi+qi+Kijθ,j = 0 (3) On [0, T]×Ω, with initial values

u(0,·) =u0; ut(0,·) =u1; θ(0,·) =θ0; q(0,·) =q0 (4) satisfying

u0∈(HΓ1D(Ω))n; u1∈(L2(Ω))n; θ0∈L2(Ω); q0∈(L2(Ω))n (5) and boundary conditions

θ|∂Ω= 0 (6)

u|ΓD = 0; σT|ΓN = 0;

σν≤0; uν≤0; σν(uν−g) = 0; σT = 0 on ΓC (7) Where

σij =Cijkluk,l+µui,j−mijθ

is the stress tensor and (withν being the exterior normal vector) σνijνiνj; σT =σν−σνν

The author would like to thank Prof. Dr. Racke for the opportunity to work on this interesting topic and helpful suggestions.

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its normal and tangential components. We assume the elasticity module C = (Cijkl)i,j,k,l, the thermal expansion tensormand the heat conduction tensorK to satisfy

Cijkl∈L(Ω); ∃dC>0∀η∈Rn×nijCijklηkl ≥dC|η|2; Cijkl=Cjikl=Cklij

kij∈L(Ω); ∃dk >0∀ξ∈Rnikijξj ≥dk|ξ|2; kij =kji

mij ∈L(Ω); mij ≥0; mij=mji

wherek=K−1in the sense of matrix inversion andµ≥0 is (for now) an arbitrary constant.

A few remarks on notation: We denote ∂ju=u,j, || · || :=|| · ||(L2)m, where mis either 1, n or n2, which will be clear from the context. In addition, L(H1) :=

L([0, T], H1(Ω)) and likewise. HΓ1

C(Ω) denotes the space of weakly differentiable functions satisfying u|ΓC = 0 in a weak sense. The technical problem in the han- dling of these equations lies in the boundary conditions for uon ΓC, which do not allow the well-known semi-group theoretic approach. Problems of this form arise naturally in the manufacturing of casts and pistons, cf. [8].

On the classical problem, i.eτ0=µ= 0, there are a number of papers available. In particular, Mun˜oz-Rivera and Racke [6] studied the corresponding classical prob- lem and derived existence and stability under the condition of radial symmetry. In the case of one space dimension, there are several results: Elliot and Tang [2] gave an existence result for more general boundary conditions; Mu˜noz Rivera and Jiang [5] gave an existence and stability result for a contact problem of two rods, and Gao and Mu˜noz Rivera [3] gave an existence and stability result for the semilinear case. Dropping the ∂2tuterm in the first equation, one arrives at the quasi-statical case, where Shi and Shillor [8] proved the existence of a solution and Ames and Payne [1] gave a uniqueness result. Mun˜oz-Rivera and Racke [6] also prove the existence of a unique solution to the corresponding classical quasi-static problem and its exponential stability. One would - and, in fact, has for quite some time - expect these results to carry over to the fully hyperbolic problem, especially as the critical equation for the displacementuwhere the difficult boundary conditions arise remains unchanged. However, in a recent work, Racke and Fern´andez Sare [7]

showed that for a damped Timoshenko system, exponential stability is lost when substituting the Fourier Law of heat conduction by Cattaneo’s. In this light, the investigation of the behaviour of this particular system under a transition from clas- sical to hyperbolic heat conduction poses an interesting question. We shall indeed see that this transition leads to a loss in regularity that is not easily compensated, thus requiring the additional viscoelastic term (µ >0).

This paper is organized as follows: In Section 2, we will give a proof for the existence of a weak solution. We will start following the approach of Mu˜noz Rivera and Racke [6] and then show why it can not be extended to this problem. To this end we will approximize the difficult boundary conditions on ΓCand obtain a penalized problem. We will then show that this penalized problem has a solution and give a sufficient condition for the convergence of this solution to a solution of our original problem - this is where the loss of regularity from the changed heat equation leaves its mark, as the conditions derived by Mu˜noz Rivera and Racke will no longer be sufficient. Finally, in section 3, we will prove a stability result in the radially symmetrical case, that is, the solutions to our problem decay to 0 exponentially. We will use a Lyapunov functional, similar to [6], although some changes are required to compensate for the different heat equation.

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2. Existence

We will prove the existence of a solution in the following sense:

Definition 2.1. (u, θ, q)is a solution to (1)-(7) iff

u∈W1,∞((L2)n)∩L((HΓ1D)n), θ∈L(L2), q∈L((L2)n) (8)

tu(T,·), q(T,·)∈(L2(Ω))n; θ(T,·)∈L2(Ω); ∇u(T,·)∈L2(Ω) (9)

∀w∈W1,∞((L2)n)∩L((HΓ1D)n), wν≤g onΓC:

T

Z

0

h∂tu, ∂twidt+hu(T,·), ∂tw(T,·)−∂tu(T,·)i − hu0, ∂tw(0,·)−u1i

T

Z

0

h∂tui,j, wi,jidt+

T

Z

0

hCijkluk,l, wi,jidt−

T

Z

0

hmijθ, wi,jidt

+

T

Z

0

h∂tu, ∂tuidt−

T

Z

0

hCijkluk,l, ui,jidt−µ

2(||∇u(T,·)||2− ||∇u0||2)

+

T

Z

0

hmijθ, uijidt≥0

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∀z∈W1,∞(H01) :

T

Z

0

hθ, zidt+hθ(T,·), z(T,·)i − hθ0, z(0,·)i −

T

Z

0

hqi, z,iidt

T

Z

0

hmijui,j, ∂tzidt+hmijui,j(T,·), z(T,·)i − hmiju0i,j, z(0,·)i= 0

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∀y∈W1,∞((H1)n) :

−τ0

T

Z

0

hkijqi, ∂tyjidt+τ0hkijqi(T,·), yj(T,·)i −τ0hkijq0i, yj(0,·)i

+

T

Z

0

hkijqi, yjidt−

T

Z

0

hθ, yi,iidt= 0

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u|ΓC ≤g a.e. (13)

We remark that all boundary conditions are represented in a weak sense in the above definiton. Also, we need the unusual condition (9) for condition (10) to make sense. This will be seen from the context in section 2.

To better handle the difficult boundary conditions in u, we consider the following penalized problem:

2tui−(Cijkluk,l),j−µui,jj+mijθ,j = 0 (14)

tθ+ div q+mijtui,j = 0 (15) τ0tkijqj+kijqj,i = 0 (16)

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with initial conditions

u(0,·) =u0; ut(0,·) =u1; θ(0,·) =θ0; q(0,·) =q0 (17) and boundary conditions

θ|Ω = 0

u|ΓD = 0; σT|ΓN = 0 σν =−1

(uν−g)+−∂tuν σT = 0 on ΓC (18) Note that only the boundary conditions on ΓChave been changed, everything else is identical to the original problem. We will see that σν is bounded and therefore by (18) (uν−g)+ → 0 as → 0, satisfying (13). Next, we give a definition of a solution to the penalized problem. Letwpp, ypp⊂H1(Ω) be bases of (L2(Ω))nand zpp⊂H01(Ω) be a basis ofL2(Ω).

Definition 2.2. Let

uε0, uε1 ∈ (H2,2(Ω)∩H01(Ω))n q0ε ∈ (H1(Ω))n

θ0 ∈ H01(Ω) Then(u, θ, q)is a solution to (14)-(18) iff

uε∈W2,∞((L2)n)∩W1,∞((HΓ1D)n); θε∈W1,∞(L2)∩L(H01);

qε∈W1,∞((L2)n)∩L(D1) (19)

uε(0,·) =uε0; ∂tuε(0,·) =uε1; θε(0,·) =θ0ε; qε(0,·) =q0ε (20) and for allmost all t∈[0, T]

∀p∈N: h∂t2uε(t,·), wpi+µh∂tuεi,j(t,·), wi,jp i+hCijkluεk,l(t,·), wi,jp i

− hmijθε(t,·), wpi,ji=−1 ε

Z

ΓC

(uεν(t,·)−g)+wpdΓ−ε Z

ΓC

tuεν(t,·)wpdΓ (21)

∀p∈N: h∂tθε(t,·), zpi+hdiv qε(t,·), zpi+hmijtuεi,j(t,·), zpi= 0 (22)

∀p∈N: τ0hkijtqiε(t,·), yjpi+hkijqiε(t,·), yjpi+h∇θε(t,·), yipi= 0 (23) To construct a solution to the penalized problem, we will use a Faedo-Galerkin- method. Note that, if (v, ψ, h) satisfy

v(0,·) =∂tv(0,·) =ψ(0,·) =h(0,·) = 0

h∂t2v, wpi+h(Cijklvk,l), wpi,ji+µh∂tvi,j, wpi,ji − hmijψ, wpi,ji

=hf, wpi −1 ε

Z

ΓC

(vν−g)+wpνdΓ−ε Z

ΓC

(∂tvν)wpνdΓ (24) h∂tψ, zpi+hdivh, zpi+hmijtvi,j, zpi=hb, zpi (25) hτ0kijthj, yii+hkijhj, yii+h∇ψ, yi=he, ypi (26) with

fi := Cijkl(uε0k,l−tuε1k,l)),j+µuε1i,jj−(mijθε0),j; (i= 1, . . . , n) b := −qε0i,i+mijuε1i,j

e := −kijq0jε −θε0,j

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thenu:=v+u0+tu1,θ:=ψ+θ0andq:=h+q0 are a solution to the penalized problem. To find such (v, ψ, h), consider the following set of equations on [0, T]

h∂t2vm, wpin+hCijklvk,lm, wpi,ji+µh∂tvi,jm, wi,jp i − hmijψ, wpi,ji

=hf, wpin−1 ε

Z

ΓC

(vmν −g)+wνpdΓ−ε Z

ΓC

tvνmwpνdΓ (p= 1, ..., m) (27)

h∂tψm, zpi+hdivhm, zpi+hmijtvi,jm, zpi=hb, zpi(p= 1, ..., m) (28) τ0hkijthmi , yjpi+hkijhmi , ypji+h∇ψm, ypin =he, ypin (p= 1, ..., m) (29) v(0,·) =∂tv(0,·) =ψ(0,·) =h(0,·) = 0 (30) where vm(t, x) = amp (t)wp(x), ψm(t, x) = bmp(t)zp(x) and hm(t, x) = cmp(t)yp(x) with unknown coefficents (amp, bmp, cmp). Then (27)-(30) is a set of ordinary differ- ential equations for (amp, bmp , cmp), thus possessing a solution with the regularity

vm∈W3,∞((HΓ1

D)n), ψm∈W2,∞(H01), hm∈W2,∞((H1)n)

Note that the initial conditions are arbitrarily smooth and f, g, e are polynomial in t, allowing for a solution with the required smoothness.

Proposition 2.1. There exist(v, ψ, h)such that

(vm)m

* v in W2,∞((L2)n)∩W1,∞((HΓ1C)n) (ψm)m

* ψ inW1,∞(L2) (hm)m * hin W1,∞((L2)n)

Proof: Multiplying (27) by dtdamp , (28) by bmp and (29) by cmp respectively, we obtain after summarizing from 1 tom:

1 2

d dt

||∂tvm||2+hCijklvk,lm, vmi,ji+1 ε

Z

ΓC

|(umν −g)+|2dΓ +||ψm||20||hm||2

+µ||∂t∇vm||2+ε Z

ΓC

|∂tvmν |2dΓ +hkijhmi , hmj i+hdivhm, ψmi+h∇ψm, hmi

=hf, ∂tvmi+hb, ψmi+he, hmi

(31) where we used that

Z

ΓC

(vmν −g)+tvmdΓ = d dt

Z

ΓC

|(vmν −g)+|2

As one easily checks by partial integration,

hdivhm, ψmi+h∇ψm, hmi= 0

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and therefore, after integrating (31) on (0, t), we obtain by Gronwall’s inequality

||∂tvm(t,·)||n ≤ C hCijklvk,lm(t,·), vmi,j(t,·)i ≤ C

1 ε

Z

ΓC

|(vνm(t,·)−g)+|2dΓ ≤ C

||hm(t,·)||n ≤ C ε

t

Z

0

Z

ΓC

|∂tvνm(t,·)|2dΓdt ≤ C (32)

t

Z

0

hkijhmi (t,·), hmj (t,·)idt ≤ C (33)

Using the smoothness of the functions (vm, ψm, hm), we see that they satisfy the time-derivated system

h∂t3vm, wpin+hCijkltvk,lm, wi,jp i+µh∂t2vi,jm, wi,jp i − hmijtψ, wpi,ji

= −1 ε

Z

ΓC

t(vmν −g)+wpνdΓ−ε Z

ΓC

t2vνmwpνdΓ +h∂tf, wpin (34)

h∂t2ψm, zpi+h∂tdiv hm, zpi+hmijt2vi,jm, zpi= 0 (35)

τ0hkijt2hmi , ypji+hkijthmi , ypji+h∂t∇ψm, ypin = 0 (36) Multiplying (34) by dtd22amp , (35) by dtdbmp and (36) by dtdcmp respectively, we obtain similar to (31)

1 2

d dt

||∂t2vm||2n+hCijkltvk,lm, ∂tvi,jmi+||∂tψm||20||∂thm||2n +µ||∂t2∇vm||2n×n+hkijhmi , hmj i

= h∂tf, ∂t2vmi −1 ε

Z

ΓC

t(vνm−g)+t2vmdΓ−ε Z

ΓC

t2vνmt2vmν

Observe that in general it is not

t |∂t(vmν −g)+|2= 2∂t(vνm−g)+t2vma.e.

since the distributional second derivative of (vνm−g)+need not be regular. However, using (32),

1 2

d dt

||∂t2vm||2n+hCijkltvk,lm, ∂tvi,jmi+||∂tψm||20||∂thm||2n +µ||∂t2∇vm||2n×n+hkijhmi , hmj i

≤ h∂tf, ∂t2vmin+ 1 2ε3

Z

ΓC

|∂tvmν|2dΓ−ε 2

Z

ΓC

|∂t2vνm|2

≤ h∂tf, ∂t2vmin+Cε

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6

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where C→ ∞ as→0. For constant we conclude, using Gronwall’s inequality again, that

(vm)m is bounded in W2,∞((L2)n)∩W1,∞((HΓ1D)n) (ψm)m is bounded in W1,∞(L2)

(hm)m is bounded in W1,∞((L2)n)

from which the claimed convergence follows.

We can now show

Theorem 2.1. There is a solution to the penalized problem.

Proof: Take (v, ψ, h) as in Proposition 2.1. Define u:=v+u0+tu1

θ:=ψ+θ0

q:=h+q0

Then it is clear that (u, θ, q) have the desired regularity (19) and fulfill the initial conditions (20). Using Lemma 1.4 from [4], we obtain the convergence

uε→uinC1([0, T],(L2C))n)

It then follows from the convergence proved in Theorem 2.1 that (u, θ, q) satisfy

(21)-(23).

Now we will prove the convergence of solutions to the penalized problem. As we can see in the proof of Proposition (2.1), we can not use the second energy level to gain estimates on the convergence of (u, θ, q), asis now no longer constant.

Therefore, we lose one level of regularity in time. This loss is grave, since we will no longer have convergence of some terms in the equations, i.e. it is generally unknown if the limits (u, ψ, q) are solutions to the original problem. However, ifµ > 0, the viscoelastic term will provide us with the missing regularity and an existence proof is possible. This will be shown in detail in the proof of Theorem 2.2.

Proposition 2.2. There exist(u, θ, q)such that

uε* u in W1,∞((L2)n)∩L(HΓ1C) θε* θ in L(L2)

qε* q in L((L2)() If µ >0, then

uε* uinW1,2((HΓ1C))

Proof: By the regularity of (uε, θ, q), we can subsitute them for (wp, zp, yp) in (21), (22) and (23) respectively and obtain

d dt

||∂tuε||2+hCijkluεk,l, uεi,ji+||θε||2+hkijqiε, qjεi+1 ε

Z

ΓC

|(uεν−g)+|2

+µ||∂t∇uε||2+hkijqiε, qεji+ε Z

ΓC

|∂tuεν|2dΓ = 0

(38) where we again used that

<divq, θ >+<∇θ, q >= 0

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Integrating from 0 tot and using Gronwall’s inequality, we conclude the existence of a constantC=C(||uε0||,||θ0ε||,||q0ε||) such that for allt >0

||∂tuε(t,·)||n ≤ C hCijkluεk,l(t,·), uεi,j(t,·)i ≤ C

||θε(t,·)|| ≤ C hkijqεi(t,·), qεj(t,·)i ≤ C 1

ε Z

ΓC

|(uεν(t,·)−g(·))+|2dΓ ≤ C

µ

t

Z

0

||∂t∇uε(s,·)||2nds ≤ C

t

Z

0

hkijqiε(s,·), qεj(s,·)ids ≤ C

ε

t

Z

0

Z

ΓC

|∂tuεν(s,·)|2dΓds ≤ C

This implies the desired convergence.

Proposition 2.3. Let(u, θ, q)be the functions from Proposition 2.2. Then uε(T,·)* u(T, ·) in L(HΓ1

C) uεt(T,·)* u t(T,·) in L(L2)

θε(T,·)* θ(T, ·) in L(L2) qε(T,·)* q(T, ·) in L(L2)

Proof: Note that due to the regularity of the solutions to the penalized problem, u, ut, θandqare continuous in time by Sobolev’s Imbedding Theorem. Therefore, the asserted convergence holds by the estimates gained in the proof for Theorem

2.2.

Theorem 2.2. Let µ >0. Let (u0, u1, θ0, q0)∈(HΓ1D(Ω))n×(L2(Ω))2n+1. Then there exists a solution to (1)-(7).

Proof: Let

(uε0)ε, (uε1)ε ⊂ (H01(Ω)∩H2,2(Ω))n (q0ε)ε ⊂ (H1(Ω))n

0ε)ε ⊂ H1(Ω) with

uε0−→u0 in (HΓ1D)n (39)

uε1−→u1 in (L2(Ω))n (40)

θ0ε−→θ0 in L2(Ω) (41)

qε0−→q0 in (L2(Ω))n (42) Let (u, θ, q) be the solutions to the penalized problem for each >0 and (u, θ, q) be the limits from Proposition 2.2. Then (u, θ, q) will satisfy (8).

8

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We can substitute zp in (22) for anyz∈W1,∞(H01) and obtain h∂tθε, zi+hdivqε, zi+hmijtuεi,j, zi= 0

Integrating from 0 to T we arrive at

hθ(T,·)ε, z(T,·)i − hθε0, z(0,·i −

T

Z

0

ε, ∂tzidt−

T

Z

0

hqεi, z,iidt

+hmijuεi,j(T,·), z(T,·)i − hmijuε0i,j, z(0,·)i −

T

Z

0

hmijuεi,j, zidt= 0

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Using Propositions 2.2 and 2.3, we conclude by taking the limit→0 that (u, θ, q) fulfill (11).

Similarly, substitutingyp in (23) for anyy∈W1,∞(H1) and integrating yields

hkijqiε(T,·), y(T,·)i − hkijq0iε, y(0,·)i −

T

Z

0

hkijqεi(t,·), ∂tyj(t,·)idt

+

T

Z

0

hkijqεi(t,·), yj(t,·)i+

T

Z

0

ε(t,·), yi,i(t,·)idt= 0

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Again, taking the limit→0 and using Propositions 2.2 and 2.3 we conclude that (u, θ, q) fulfill (12).

From Proposition 2.3, it is immediately clear that (u, θ, q) satisfy (9). Using Lemma 1.4 from [4] again, it follows from Proposition 2.2 that

uε−→u inC0([0, T],(L2C))n) therefore, since

1 ε

Z

ΓC

|(uεν(t,·)−g(·))+|2dΓ ≤C,

we conclude that

Z

ΓC

|(uν(t,·)−g(·))+|2dΓ = 0

and therefore (13) is satisfied.

Note that we did not useµ >0 yet, therefore everything we proved so far will also hold if µ= 0. The critical part is in fact the convergence of quadratic terms that appear in (10), as we will see in the following calculations.

For any w∈L(HΓ1

D)∩W1,∞(L2) we substitutewp in (23) byw−uand obtain h∂t2uε, w−uεi+hCijkluεk,l, wi,j−uεi,ji

+µh∂tuεi,j, wi,j−uεi,ji+hmijθε, wi,j−uεi,ji

= −1 ε

Z

ΓC

(uεν−g)+(wν−uεν)dΓ−ε Z

ΓC

tuεν(wν−uεν)dΓ

9

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Integrating from 0 to T we arrive at

h∂tuε(T,·), w(T,·)i − h∂tuε(T,·), uε(T,·)i − huε1, w(0,·)−uε0i

T

Z

0

h∂tuε(t,·), ∂tw(t,·)idt+

T

Z

0

hCijkluεk,l(t,·), wi,j(t,·)idt

+

T

Z

0

h∂tuε(t,·), ∂tuε(t,·)idt−

T

Z

0

hCijkluεk,l(t,·), uεi,j(t,·)idt

T

Z

0

h∂tuεi,j(t,·), wi,j(t,·)idt−µ

2 ||∇uε(T,·)||2− ||∇uε0||2

+

T

Z

0

hmijθε(t,·), wi,j(t,·)idt−

T

Z

0

hmijθε(t,·), uεi,j(t,·)idt

= 1 ε

T

Z

0

Z

ΓC

(uεν(t,·)−g)+(uεν(t,·)−g)−(uεν(t,·)−g)+(wν(t,·)−g)dΓdt

−ε

T

Z

0

Z

ΓC

tuεν(t,·)wν(t,·)dΓdt+ε 2

Z

ΓC

|uεν(T,·)|2− |uε|2

≥ − ε

T

Z

0

Z

ΓC

tuεν(t,·)wν(t,·)dΓdt+1 2

Z

ΓC

|uεν(T,·)|2− |uε|2

(45)

Using Propositions 2.2 and 2.3, we see that the right hand side of (45) will converge to 0 as→0, since weak-* convergent series are bounded in norm. For the left hand side we can again conlude the convergence of all terms that are linear in (u, θ, q).

However, the convergence of the quadratic terms, namely the L2(0, T)-Norms of

||ut||,hCijklui,j, uk,li andhmijθ, ui,ji remains an issue. While we know the terms will be bounded, we can not conclude their convergence to the respective terms for u, as weak-* convergence does not imply norm convergence.

Note that it is not possible to circumvent this problem by simply taking estimates for the second order energy and giving a strong solution, since the second order energy is not (trivially) bounded in . We remark that Mun˜oz Rivera and Racke [6] encountered a similar problem, which could be circumvented by reducing the problem to the radially symmetrical case and using an estimate obtained via com- pensated compactness. However, it is not possible to utilize this for our problem, since we do not have a bound on∇θ, which is a necessary component of the proof in [6].

Therefore, we shall useµ >0, which will yield uε* uin W1,2((HΓ1C))

by Proposition 2.2. From this we can conclude the uniform convergence of ut as well as ∇u. It is then possible to take the limit→ 0 in (45) and conclude that

(u, θ, q) will satisfy (10).

10

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3. Stability

In general, one can not expect the exponential stability of a thermoelastic problem that is not radially symmetric. Therefore, we shall restrict our problem to the ra- dially symmetric, isotropic and homogenous case, i.e. we assume that the following conditions hold:

The domain Ω is radially symmetric, in this case annular:

Ω =B(0,1)\B(0, r0), 1> r0>0; ΓD=∂B(0, r0); ΓC=∂B(0,1); ΓN =∅ The coefficients satisfy the following symmetry conditions:

Cijkl=λδijδkl+ν(δikδjljkδil)

mij =mδij, Kij =κδij, g(x) =g≥0 f.a. x∈ΓC

Additionally, we shall assume that the solution to the problem as derived in the previous section is unique in this case, which implies that with radially symmetric initial data and the above assumptions on the coefficients, the solution itself will be radially symmetric. We shall first investigate the stability of the penalized problem, which will transfer to the original problem by a simple continuity argument.

With our assumptions, the equations take the form

t2uε−µ∂t4uε−λ14uε−(λ12)∇divuε+m∇θε= 0 (46)

tθε+ divqε+mdiv∂tuε= 0 (47) τ0tqε+qε+κθε= 0 (48) with Lame-Moduliλ12satisfying 2λ1+nλ2>0 and constantsκ >0 andm6= 0.

The boundary conditions to the penalized problem then read θε|∂Ω= 0, uε|ΓD = 0 µ∂t∂uε

∂ν ·ν+λ1∂uε

∂ν ·ν+ (λ12)divuε=−1

ε(uεν−g)+−ε∂tuεν on ΓC (49) As mentioned above, solutions to this problem will also be radially symmetric, so we can write

uε(t, x) =xw(t,|x|), θε(t, x) =ψ(t,|x|), qε(t, x) =xh(t,|x|) Writingr:=|x|, (w, ψ, h) will then satisfy the equations

t2w−µ∂twrr−µ∂t

1

rwr−ν1wrr−ν2

r wr+m

r= 0 (50)

tψ+nh+rhr+mn∂tw+mr∂twr= 0 (51) τ0th+h+κ

r= 0 (52)

We will now show that the energy of the penalized problem, defined by Eε(t) :=||∂tuε||21||∇uε||2+κ||θε||2+||qε||2+1

ε Z

ΓC

|(uεν−g)+|2

11

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decays exponentially as time goes to infinity, i.e.

Eε(t)≤αE0εe−βt

We will use the technique of a Lyapunov functional, constructing the negative terms of the energy and combining the respective functionals in a final estimate. First, one easily sees by multiplying (46) with ∂tu, (47) with κθ and (48) with q and integrating over Ω, that the energy satisfies

d

dtEε(t)≤ −C2 (µ||∂tuε||2n+||qε||2n) (53) Proposition 3.1. Let

F1(t) :=h∂tuε, uεin+ε Z

ΓC

|uεν|2dΓ−µ||∇uε||2n×n then for any δ1>0

d

dtF1(t)≤ −(C3−δ1)||∇uε||2n×n−1 ε

Z

ΓC

|(uεν−g)+|2dΓ +||∂tuε||2n+C4

δ1||θε||2 (54) Proof:

d

dth∂tuε, uεi

=||∂tuε||2+h∂t2uε, uεi

=||∂tuε||2−λ1||∇uε||2−µh∂t∇uε,∇uεi − hmθε,div uεi

−(λ12)||divuε||2−1 ε

Z

ΓC

(uεν−g)+uνdΓ−ε Z

ΓC

tuενuεν

(55)

Estimating

|hmθε,divuεi| ≤C4

δ1||∇uε||2+1 δ1

||θε||2

for any δ1>0 and

−1 ε

Z

ΓC

(uεν−g)+uεν

≤ −1 ε

Z

ΓC

|(uεν−g)+|2

we obtain the desired result.

Proposition 3.2. Let

Ψ(t, r) :=

r

Z

r0

ψ(t, s)ds and

F2(t) :=−τ0 1

Z

r0

Ψ(t, r)h(t, r)dr Then for any δ2, δ3>0

d

dtF2(t)≤ C δ23

1

Z

r0

|h(t, r)|2dr−κ−δ2

r0 1

Z

r0

|ψ(t, r)|2dr+δ3 1

Z

r0

|∂tw(t, r)|2dr (56)

12

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Proof: By (51), Ψ satisfies

tΨ +

r

Z

r0

nhds+

r

Z

r0

shds+

r

Z

r0

mn∂twds+

r

Z

r0

ms∂twsds= 0 (57)

Multiplying (57) withhr and integrating, we obtain for anyδ3>0

1

Z

r0

(∂tΨ)hrdr=n

1

Z

r0

hr

r

Z

r0

hdsdr+

1

Z

r0

hr

r

Z

r0

shsdsdr

+mn

1

Z

r0

hr

r

Z

r0

tw(t, s)dsdr+m

1

Z

r0

h

r

Z

r0

s∂twsdsdr

≤ C δ3

1

Z

r0

|h(t, r)|2dr+δ3 1

Z

r0

|w(t, r)|2dr

(58)

Multiplying (52) by Ψrand integrating, we obtain

τ0

1

Z

r0

Ψ(∂th)rdr+

1

Z

r0

Ψhrdr+

1

Z

r0

κΨrrΨdr= 0

We have, by definition of Ψ,

1

Z

r0

κΨrr(t, r)Ψ(t, r)dr=−κ

1

Z

r0

r(t, r)|2dr=−κ

1

Z

r0

|ψ(t, r)|2dr

Using Poincar´e’s Inequalitiy for Ψ, this implies for any δ2>0

1

Z

r0

Ψ(∂th)rdr≤ C δ2

1

Z

r0

|h|2dr−(κ−δ2)

1

Z

r0

|ψ|2dr (59)

Combining (58) and (59), we obtain the desired result.

Defining

L(t) :=N Eε(t) +F1(t) +δ4F2(t)

whereδ4 will be chosen later, we easily see that for large enoughN there existC1, C2>0 such that

C1E(t)≤L(t)≤C2E(t) (60)

Now, we can prove the essential theorem of this section.

Theorem 3.1. Let µ >0. Then the system is exponentially stable, i.e. there is a β >0such that

Eε(t)≤αE0εe−βt

13

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Proof: Using (53), (54) and (56), we conclude that d

dtL(t)≤ −N C2(µ||∂tuε||2n+||qε||2n)−(C3−δ1)||∇uε||2n×n

−1 ε

Z

ΓC

|(uεν−g)+|2dΓ +||∂tuε||2n+C4 δ1

||θε||2

4

 C5 δ23

1

Z

r0

|h(t, r)|2dr−κ−δ2 r0

1

Z

r0

|ψ|2dr+δ3

1

Z

r0

|∂tw|2dr

≤(1 +C6δ3δ4−N C2µ)||∂tuε||2n+ ( δ4C7

δ23

−N C2)||qε||2n+ (δ1−C3)||∇uε||2n×n

−1 ε

Z

ΓC

|(uεν−g)+|2dΓ + (C4

δ1

−δ4

κ−δ2

r0

)||θε||2

Choosing δ1 < C3 and δ2 < κ, then δ4 > δ r0C4

1(κ−δ2) and (arbitrarily) δ3 = 1 we conclude that, for sufficiently large N, there is aC >0 such that

d

dtL(t)≤ −CEε(t)

Using (60), this proves our theorem.

Note that δ3 is not really needed for the construction of the Lyapunov functional and could have been left as 1. However, we want to point out that the positive ut term arising from F2is not a problem; the problem requiring µ >0 is the positive utterm arising fromF1, which can not be made arbitrarily small without losing the negative terms for the derivatives of u. For the classical problem, Mun˜oz-Rivera and Racke [6] showed that this term can be handled by adding additional functions to the Lyapunov functional; however, this gives rise to a positive ∇θterm. While

∇θis given as a negative term from the energy itself in the classical case, this does not hold forτ0 >0; in fact we do not know anything about derivatives ofθ. It is therefore necessary to gain the negativeutterm by other means, one of them being the viscoelastic term. If we define the energy of the original problem as

E(t) :=||∂tu||2+||∇u||2+||θ||2+||q||2

we see by the lower semicontinuity of the norms of weak*-convergent series, using Proposition 2.2, that

lim inf

ε→0 Eε(t)≥E(t) Using the strong convergence of initial data, we obtain

E(t)≤Eε(t)≤αEε(0) exp(−βt)→αE(0) exp(−βt) This proves our final theorem:

Theorem 3.2. Letµ >0. Then there areα,β >0such that E(t) ≤ αE(0) exp(−βt)

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References

[1] K.A. Ames and L.E. Payne. Uniqueness and continuous dependence of solutions to a multidi- mensional thermoelastic contact problem.J. Elasticity, 34:139–148, 1994.

[2] C.M. Elliot and Q. Tang. A dynamic contact problem in thermoelasticity.Nonlinear Analysis, 23:884–898, 1994.

[3] H. Gao and J. Mu˜noz Rivera. Global existence and decay for the semilinear thermoelastic contact problem.J. Differential Equations, 186:52–68, 2002.

[4] J.U. Kim. A boundary thin obstacle problem for a wave equation.Comm. Partial Differential Equations, 14:1011–1026, 1989.

[5] J. Mu˜noz Rivera and S. Jiang. The thermoelastic and viscoelastic contact of two rods.J. Math.

Anal. Appl., 217:423–458, 1998.

[6] J. Mu˜noz Rivera and R. Racke. Multidimensional contact problems in thermoelasticity.SIAM J. Appl. Math, 58:1307–1337, 1998.

[7] H. Fern´andez Sare and R. Racke. On the stability of damped timoshenko systems - cattaneo versus fourier law.Archive Rational Mech. Anal. (to appear), 2007.

[8] P. Shi and M. Shillor. Existence of a solution to the n dimensional problem of thermoelastic contact.Comm. Partial Differential Equations, 17:1597–1618, 1992.

Jan Sprenger, Institute for Analysis and Scientific Computing, Vienna University of Technology, Wiedner Hauptstraße 8-10, 1040 Wien, Austria

E-Mail: jsprenger@asc.tuwien.ac.at

15

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