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www.elsevier.com/locate/anihpc

A vanishing viscosity approach to a quasistatic evolution problem with nonconvex energy

Alice Fiaschi

SISSA, Via Beirut 2-4, 34014 Trieste, Italy Received 14 January 2008; accepted 22 February 2008

Available online 21 March 2008

Abstract

We study a quasistatic evolution problem for a nonconvex elastic energy functional. Due to lack of convexity, the natural energetic formulation can be obtained only in the framework of Young measures. Since the energy functional may present multiple wells, an evolution driven by global minimizers may exhibit unnatural jumps from one well to another one, which overcome large potential barriers. To avoid this phenomenon, we study a notion of solution based on a viscous regularization. Finally we compare this solution with the one obtained with global minimization.

©2008 Elsevier Masson SAS. All rights reserved.

MSC:74B20; 28A33; 74G65; 49J45

Keywords:Quasistatic evolution; Rate-independent processes; Elastic materials; Incremental problems; Young measures

1. Introduction

In this paper we consider a quasistatic evolution problem for an elastic material described by the deformation variable and by a further parameter which plays the role of internal variable connected to energy dissipation. The energetic formulation of this problem is expressed in terms of the elastic energy functionalW, depending both on the deformation and on the internal variable, and of the dissipation functionalH, depending just on the internal variable (see, e.g. [10,12,13]).

As in [8] we assume thatWandHhave the following integral form W(z, v):=

D

W

z(x),v(x) dx,

H(z):=

D

H z(x)

dx

E-mail address:fiaschi@sissa.it.

0294-1449/$ – see front matter ©2008 Elsevier Masson SAS. All rights reserved.

doi:10.1016/j.anihpc.2008.02.003

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whereD⊆Rdis the reference configuration,v:D→RN the deformation, andz:D→Rmthe internal variable. We also assume that the body is subjected to volume forcesf(t )depending on time, and to a time-dependent prescribed boundary condition (which in this introduction is imposed on the whole boundary for simplicity).

The standard method to attack the problem of the quasistatic evolution is via time-discretization and resolution of incremental minimum problems, which in our case would take the form

min

W(z, v)f(t ), v

+H(zz0)

(1.1) among all functions(z, v)which satisfy the prescribed boundary condition at timet. Herez0is the known value ofz at the previous instant.

For the mechanical applications considered in [8], the convexity ofWwith respect to the internal variablezis not a natural assumption. Thus, as observed in [7], the minimum problem (1.1) may have no solutions; moreover, since the lack of convexity allows the functional to have multiple wells, a quasistatic evolution driven by global minimizers, if they would exist, could prescribe abrupt jumps from one well to another one; therefore it is preferable to follow a path composed by local minimizers rather than global minimizers.

In this spirit, the properties of global minimality (stability) and energy balance characterizing the usual energetic solution (see e.g. [11, Section 3] and references therein) are weakened: they are replaced by a stationarity condition and an energy inequality, i.e.

(1) for everyt∈ [0, T]

−divσ(t )=f(t ), ζ(t )∂H(0)

whereσ(t ):=∂W∂F(z(t ),v(t ))andζ(t ):= −∂W∂θ (z(t ),v(t ));

(2) for everyt∈ [0, T] W

z(t ),v(t )

f(t ),v(t )

+VarH(z;0, t ) W(z0, v0)

f(0), v0

+ t 0

σ(s),∇ ˙ϕ(s) ds

t 0

f˙(s),v(s) +

f(s),ϕ(s)˙ ds,

where VarH is a suitably defined notion of variation (see (3.1)).

Moreover in the spirit of [5,3,15,1,9], we propose a selection criterion among the solutions of (1) and (2), based on a sort of viscous approximation. The underlying idea is that an evolution obtained in this way does not jump over potential barriers. Given a regularizing parameterε >0, we first consider theε-regularized problem:

(a) equilibrium condition: for a.e.t∈ [0, T]

−divσε(t )εv˙ε(t )=f(t ); (1.2)

(b) regularized flow rule: for a.e.t∈ [0, T]

˙

zε(t )=NKε ζε(t )

a.e. inD,

where we look for a solution(zε,vε)inH1([0, T];L2(D;Rm)×H1(D;RN))satisfying the boundary condition, σε(t ):=∂W∂F(zε(t ),vε(t )),ζε(t ):= −∂W∂θ (zε(t ),vε(t )), and NKε(ζ):= 1εPK(ζ)),PK being the projection ontoK:=∂H (0).

In Theorem 4.4 we prove that everyε-regularized problem is equivalent to the following one:

(1)ε equilibrium condition: for a.e.t∈ [0, T]

−divσε(t )εv˙ε(t )=f(t ) (1.3)

relaxed dual constraint: for a.e.t∈ [0, T]

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ζε(t )εz˙ε(t )∂H(0); (2)ε energy equality: for everyt∈ [0, T],

W

zε(t ),vε(t )

f(t ),vε(t ) +

t 0

H

˙ zε(s)

ds+ε t 0

z˙ε(s)2

2ds+ε t 0

∇ ˙vε(s),∇ ˙vε(s)− ∇ ˙ϕ(s) ds

=W(z0, v0)f(0), v0

+ t 0

σε(s),∇ ˙ϕ(s) ds

t 0

f˙(s),vε(s) +

f(s),ϕ(s)˙ ds

where we look for a solution(zε,vε)inH1([0, T];L2(D;Rm)×H1(D;RN))satisfying the boundary condition.

To prove the existence and uniqueness of the solutions to theε-regularized problems we use the analysis of dis- cretized minimum problems. We fix a time discretization of the interval[0, T]

0=t0< t1<· · ·< tn=T ,

and we setτi :=titi1, fori >0. Givenε >0 and an initial value(z0, v0), we define inductively the value of an approximate solution of theε-regularized problem at timeti, fori >0, as a minimizer of the functional

W(z, v)f(ti), v

+H

zz(ti1) + ε

i

zz(ti1)2

2+ εi

v− ∇v(ti1)2

2, (1.4)

among all(z, v)which satisfy the boundary condition at time ti. Under suitable regularity assumptions onW, the functional (1.4) is convex forτi sufficiently small, thanks to the presence of the regularizing terms ε

izz(ti1)22 and ε

iv− ∇v(ti1)22; hence the minimizer exists and is unique. The study of the limit of the approximate solu- tions, when the discretization step tends to 0 and the parameterεis kept fixed, proves the existence (see Theorem 4.6) of a unique solution of theε-regularized problem.

We come back now to the original problem: as in [3], we accept only solutions to (1) and (2) which can be approxi- mated by solutions ofε-regularized problems; nevertheless, due to the nonconvexity of the problem, theε-regularized solutions may develop stronger and stronger oscillations in space asεtends to 0, and this prevents the passage to the limit of(1)εand(2)εin the usual function spaces.

Therefore (1) and (2) need a weaker formulation in terms of Young measures, or equivalently (see [7, Section 3]) in terms of stochastic processes. In the latter formulation the function(z(t, x),v(t, x))is substituted by a stochastic process(Zt(x, ω),Yt(x, ω)), defined on a product probability space(D×Ω, P ), with

πD(P )=Ld, (1.5)

and (1), (2) become

(1) equilibrium condition: for everyt∈ [0, T]

−divσ(t )=f(t ); (1.6)

dual constraint: for everyt∈ [0, T]

ζ(t )∂H(0); (1.7)

(2) energy inequality: for everyt∈ [0, T]we have

D×Ω

W

Zt(x, ω),Yt(x, ω)

dP (x, ω)

f(t ),v(t )

+VarH(Z, P;0, t )

W(z0, v0)f(0), v0

+ t 0

σ(s),∇ ˙ϕ(s) ds

t 0

f(s),ϕ(s)˙

+f˙(s),v(s)

ds, (1.8)

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where(Zt,Yt)tis the stochastic process representing the evolution,v(t )is the unique function satisfying the boundary condition and∇v(t )=bar((πD,Yt)(P )),σ(t ),ζ(t )are the unique elements ofL2(D;RN×d)andL2(D;Rm), such that

D

σ(t, x)g(x) dx=

D×Ω

∂W

∂F

Zt(x, ω),Yt(x, ω)

g(x) dP (x, ω),

D

ζ(t, x)h(x) dx=

D×Ω

∂W

∂θ

Zt(x, ω),Yt(x, ω)

h(x) dP (x, ω),

for everygL2(D;RN×d),hL2(D;Rm), and VarH(Z, P;0, t ):=sup

k i=1

D×Ω

H

Zti(x, ω)Zti1(x, ω)

dP (x, ω),

where the supremum is taken over all finite partitions 0=t0<· · ·< tk=t.

In this formalism ordinary functions can be seen as stochastic processes independent ofω; in this case conditions (1)and(2)are exactly (1) and (2), thanks to (1.5).

In Theorem 7.16 we study the passage to the limit in the space of Young measures of the solutions to the ε-regularized problems, asεtends to 0, while in Theorem 7.13 we show that the stochastic process corresponding to this limit is a solution of the generalized problem(1)and(2).

In the last section, we compare the notion of approximable quasistatic evolution considered in the present paper with the quasistatic evolution based on global minimization defined in [7, Definition 6.12]. More precisely we study an example in which the approximable quasistatic evolution is unique and is a classical function which can be described explicitly. Theorem 8.2 proves that this evolution cannot be a globally stable quasistatic evolution, since it does not satisfy the stability condition.

2. Mathematical preliminaries and notations

For the mathematical preliminaries about functions, measures, and Young measures we refer to [7, Section 2].

The symbol·,· will denote a duality pairing depending on the context.

We refer to [7, Section 3] for a presentation of compatible systems of Young measures with probabilistic language;

here we just recall the statement of the main theorem about the correspondence between compatible systems of Young measures and stochastic processes.

Theorem 2.1.LetT be a set of indices, and let, for everytT,VtandWtbe finite dimensional Hilbert spaces. Given two compatible systemsμSY2(D;(Vt)tT)andνSY2(D;(Vt×Wt)tT), satisfying

πD×Vtt)=μt, for everytT , (2.1)

there exist a probability space of the form(D×Ω,B(D)F, P ), whereB(D)is the Borelσ-algebra onD,(Ω,F) is a measurable space, andP a probability measure withπD(P )=Ld, and a stochastic process(Zt,Yt)tT with

ZtL2(D×Ω;Vt), YtL2(D×Ω;Wt), for everytT, such that

πD, (Zt)tF

(P )=μF, (2.2)

for every nonempty finite subsetF ofT, and

D,Zt,Yt)(P )=νt, (2.3)

for everytT.

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3. Mechanical model

Thereference configurationDis a bounded connected open subset ofRdwith Lipschitz boundary∂D=Γ0Γ1, whereΓ0is assumed to be a nonempty closed subset of∂DwithHd10)=0, andΓ1=∂D\Γ0. Without loss of generality we also assume for simplicity thatLd(D)=1.

We indicate the deformation byvand the internal variable byz.

We denotethe stored energy densitybyW:Rm×RN×d→ [0,+∞)and thedissipation rate densitybyH:Rm→ [0,+∞). For everyθ∈Rmand everyF ∈RN×d, we make the following assumptions:

(W.1) there exist positive constantsc, Csuch that c

|θ|2+ |F|2

CW (θ, F )C

1+ |θ|2+ |F|2

; (W.2) Wis of classC2and there exists a positive constantMsuch that

2W

∂(θ, F )2(θ, F ) M,

where ∂(θ,F )2W2 denotes the matrix of all second derivatives with respect to (the components of)θandF; (H.1) His positively homogeneous of degree one and convex;

(H.2) there exists a positive constantλ, such that 1λ|θ|H (θ )λ|θ|.

LetWbe the functionalW(z, v):=

DW (z(x),v(x)) dx, for everyzL2(D;Rm)and everyvH1(D;RN), andHthe functionalH(z):=

DH (z(x)) dx, for everyzL1(D;Rm).

Given two distinct timess < t, theglobal dissipationof a possibly discontinuous functionz:[0, T] →L2(D;Rm) in the interval[s, t]is

VarH(z;s, t ):=sup k

i=1

H

z(τi)z(τi1)

, (3.1)

where the supremum is taken among all finite partitionss=τ0< τ1<· · ·< τk=t. Note that forzH1([0, T];L2(D;Rm))we have

VarH(z;s, t )= t

s

H

˙ z(τ )

(3.2)

(see, e.g., [2, Theorem 7.1]).

The external load at time t and the prescribed boundary datum on Γ0 at timet are denoted byl(t ) andϕ(t ), respectively; we assume that lH1([0, T];H1(D;RN)), where H1(D;RN) is the dual of H1(D;RN), and ϕH1([0, T];H1(D;RN)).

The kinematically admissible values at timet forzandvare those who make the total energy finite and satisfy the boundary condition, i.e.v=ϕ(t )onΓ0Hd1-a.e. (in the sense of traces). From previous assumptions it follows that the kinematically admissible values at timet are contained inL2(D;Rm)×A(t ), where

A(t )=HΓ1

0

ϕ(t ) :=

vH1 D;RN

such thatv=ϕ(t )Hd1-a.e. onΓ0 .

Before concluding this section, we want to point out some properties of the functionalHand to introduce some new notation.

From the hypotheses onH, it follows thatHis l.s.c. with respect to the weak topology ofL2(D;Rm)and satisfies the triangle inequality, i.e.

H(z1+z2)H(z1)+H(z2).

For everyε >0 we define the functionHε:Rm→Ras Hε(θ ):=H (θ )+ε

2|θ|2, (3.3)

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and the corresponding integral functionalHε:L2(D;Rm)→Ras Hε(z):=

D

Hε z(x)

dx. (3.4)

The convex conjugateHε:Rm→RofHε is Hε(ζ ):= sup

θ∈Rm

ζ θHε(θ ) .

Since the convex conjugateHofHis the indicator function of the convex setK:=∂H (0)(see [14, Theorem 13.2]), using [14, Theorem 16.4], it can be proved that

Hε(ζ )= 1

2εζ−PK(ζ )2, (3.5)

wherePK:RmKis the projection ontoK. ThereforeHεis differentiable with gradient NKε(ζ ):=1

ε

ζPK(ζ )

. (3.6)

In particularNKε is Lipschitz continuous.

Let Hε:L2(D;Rm)→Rbe the convex conjugate of Hε. It can be easily shown (using a general property of integral functionals, see e.g., [6, Proposition IX.2.1]) that

Hε(ζ )=

D

Hε ζ (x)

dx, so that the gradient∂Hε is given by

∂Hε(ζ )(x)=NKε ζ (x)

, for a.e.xD. (3.7)

Therefore∂Hε is Lipschitz continuous.

4. Regularized evolution

In this section we give the definition and an existence result for the solution of theε-regularized evolution problem.

We will assume that the initial condition(z0, v0)L2(D;Rm)×A(0)satisfies the following condition σ0,∇ ˜u =

l(0),u˜

for everyu˜∈HΓ1

0(0), (4.1)

ζ0∂H(0), (4.2)

whereσ0(x):=∂W∂F(z0(x),v0(x)),ζ0(x):= −∂W∂θ (z0(x),v0(x)), for a.e.xD.

Definition 4.1. Let ε >0, lH1([0, T];H1(D;RN)), ϕH1([0, T];H1(D;RN)), (z0, v0)L2(D;Rm)× A(0), and T >0. Assume that (z0, v0) satisfies (4.1) and (4.2). A solution of the ε-regularized problem in the time interval [0, T], with external load l, boundary datum ϕ, and initial condition (z0, v0) is a pair (zε,vε)H1([0, T];L2(D;Rm)×H1(D;RN)), satisfying the following conditions:

(ev0)ε initial condition:(zε(0),vε(0))=(z0, v0);

(ev1)ε kinematic admissibility:vε(t )A(t ), for everyt∈ [0, T];

(ev2)ε equilibrium condition: for a.e.t∈ [0, T]and for everyu˜∈HΓ1

0(0), σε(t )+ε∇ ˙vε(t ),∇ ˜u

= l(t ),u˜

, (4.3)

whereσε(t ):=∂W∂F(zε(t ),∇vε(t ));

(ev3)ˆ ε regularized flow rule: for a.e.t∈ [0, T],

˙

zε(t )=NKε ζε(t )

a.e. inD, (4.4)

whereζε(t ):= −∂W∂θ(zε(t ),∇vε(t )).

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Remark 4.2.Iflcan be written in the form l(t ),v˜

=

D

f (t, x)· ˜v(x) dx+

∂D

g(t, x)· ˜v(x) dHd1(x),

withf (t )L2(D;RN)andg(t )L2(∂D;RN), for everyv˜∈H1(D;RN), then (ev2)εtakes the form

−divσε(t )εv˙ε(t )=f (t ), (4.5)

σε(t )+ε∇ ˙vε(t )

·ν=g(t ), Hd1-a.e. onΓ1, (4.6)

whereνis the outer unit normal to∂D.

Indeed, choosing firstu˜∈H01(D;RN)in (ev2)ε, we obtain (4.5) and this ensures that−divσε(t )εv˙ε(t )L2(D;RN); hence we can apply integration by parts to get (4.6).

Remark 4.3.Let us fixt∈ [0, T]such thatz˙ε(t )andv˙ε(t )exist. Then the following conditions are equivalent

˙

zε(t )=NKε ζε(t )

a.e. inD, (4.7)

ζε(t )∂Hε

z˙ε(t )

, (4.8)

ζε(t )εz˙ε(t )∂H

˙ zε(t )

. (4.9)

Indeed, by (3.7),∂Hεε(t ))=NKεε(t )), so that (4.7) and (4.8) are equivalent by standard property of conjugate functions (see, e.g., [6, Corollary I.5.2]). The equivalence of (4.8) and (4.9) comes from the definition ofHε.

In the following theorem we prove that the modified flow rule (evˆ3)εcan be replaced by a suitable constraint onζε and an energy equality.

Theorem 4.4.Letl,ϕ,z0,v0,ε, andT be as in Definition4.1.

Then(zε,vε)H1([0, T];L2(D;Rm)×H1(D;RN))is a solution of theε-regularized problem in the time interval [0, T], with external loadl, boundary datumϕ, and initial condition (z0, v0) if and only if it satisfies the initial condition(ev0)ε, the kinematic admissibility(ev1)ε, the equilibrium condition(ev2)ε, and the following conditions:

(ev3)ε relaxed dual constraint:ζε(t )εz˙ε(t )∂H(0), for a.e.t∈ [0, T];

(ev4)ε energy equality:for everyt∈ [0, T], W

zε(t ),vε(t )

l(t ),vε(t ) +

t 0

H

˙ zε(s)

ds+ε t 0

z˙ε(s)2

2ds+ε t 0

∇ ˙vε(s),∇ ˙vε(s)− ∇ ˙ϕ(s) ds

=W(z0, v0)l(0), v0

+ t 0

σε(s),∇ ˙ϕ(s) ds

t 0

˙l(s),vε(s) +

l(s),ϕ(s)˙ ds.

Remark 4.5.Since we are dealing with theε-regularized problem, in theenergy equalitythere are two extra terms proportional toεand depending on the time derivatives ofzεand∇vε; they represent a sort of viscous dissipation.

Proof of Theorem 4.4. Suppose that(zε,vε)satisfies (ev0)ε, (ev1)ε, (ev2)ε and (evˆ3)ε. AsHis positively homoge- neous of degree one, by a general property of integral functionals (see, e.g., [6, Proposition IX.2.1])

∂H

˙ zε(t )

∂H(0)= ζL2

D;Rm

: ζ (x)∂H (0)for a.e.xD

, (4.10)

for a.e.t∈ [0, T]. Hence from (4.9) we derive (ev3)ε.

SinceHis positively homogeneous of degree one, we haveζ, z =H(z), for everyzL2(D;Rm)andζ∂H(z).

Therefore, by (4.9), H

˙ zε(t )

=

ζε(t )εz˙ε(t ),z˙ε(t )

, (4.11)

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for a.e.t∈ [0, T].

Choosingu˜= ˙vε(t )− ˙ϕ(t )in (ev2)εand using (4.11) we obtain ∂W

∂θ

zε(t ),vε(t ) ,z˙ε(t )

+

∂W

∂F

zε(t ),vε(t )

,∇ ˙vε(t )− ∇ ˙ϕ(t )

l(t ),v˙ε(t )− ˙ϕ(t ) +H

˙ zε(t ) +εz˙ε(t )2

2+ε

∇ ˙vε(t ),∇ ˙vε(t )− ∇ ˙ϕ(t )

=0, (4.12)

for a.e.t∈ [0, T]. By integration of (4.12) from 0 tot, we obtain (ev4)ε.

Conversely, suppose that(zε,vε)satisfies (ev0)ε, (ev1)ε, (ev2)ε, (ev3)εand (ev4)ε. Then, by derivation with respect tot of (ev4)ε, we obtain (4.12), which gives (4.11), thanks to (ev2)ε. Combining (4.11) with (ev3)ε, it immediately follows (4.9) for a.e.t∈ [0, T], and hence (evˆ3)ε. 2

We conclude by stating the existence theorem for the solutions of theε-regularized problems, which will be proved in the next section.

Theorem 4.6.Letε,l,ϕ,z0,v0, andT as in Definition4.1. Then there exists a unique solution of theε-regularized problem in the time interval[0, T]with external loadl, boundary datumϕand initial condition(z0, v0).

5. Proof of Theorem 4.6

The proof is obtained via time-discretization, resolution of incremental minimum problems, and passing to the limit as the time step tends to 0.

5.1. The incremental minimum problem

In this section we study the incremental minimum problem used in the discrete-time formulation of the evolution problem.

Let us fix a sequence of subdivisions of[0, T], 0=tn0< tn1<· · ·< tnk(n)=T, such thatτn:=supi=1,...,k(n)τni→0, as n→ ∞, whereτni :=tnitni1, for everyi=1, . . . , k(n). We assume thatτn<Mε for everyn, whereM is the constant appearing in (W.2).

For everyi=0,1, . . . , k(n)we setlin:=l(tni)andϕni :=ϕ(tni).

For everyn, we define(zni, vin)L2(D;Rm)×A(tni)by induction oni: set(zn0, v0n):=(z0, v0), and fori >0 we define(zin, vni)as the solution (see Lemma 5.1 below) to the incremental minimum problem

min

W(z, v)lni, v

+H

zzin1 + ε

nizzin12

2+ ε

niv− ∇vni12

2

, (5.1)

among allzL2(D;Rm)and allvA(tni).

Lemma 5.1.Letε >0, then for everynand everyi >0there exists a unique solution to(5.1)inL2(D;Rm)×A(tni).

Proof. Let(zk, vk)L2(D;Rm)×A(tni)be a minimizing sequence. By the bounds onW and the assumption onl, we have

c

zk22+ ∇vk22

C

1+ vkH1

W(zk, vk)lin, vk

C, (5.2)

for suitable positive constants c, C. Since vkA(tni), using Poincaré inequality we can deduce from (5.2) that (zk, vk)kis a bounded sequence inL2(D;Rm)×H1(D;RN).

From the boundedness of the second derivative ofW, guaranteed by (W.2), and sinceτn(0, ε/M)by our assump- tion onτn, it easily follows that the functional in (5.1) is strictly convex, and hence weakly lower semicontinuous on L2(D;Rm)×H1(D;RN). Now the existence of minimizers comes from the direct methods of the Calculus of Varia- tions; the uniqueness is a consequence of the strict convexity of the functional. 2

Now we derive Euler conditions for the minimizers.

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Theorem 5.2.Letε >0, then for everynand everyi >0we have H

˜

z+zinzin1

H

zinzin1

lni,u˜

∂W

∂θ

zin,vin ,z˜

∂W

∂F

zin,vni ,∇ ˜u

ε τni

zinzin1,z˜

ε τni

vni − ∇vin1,∇ ˜u

, (5.3)

for everyz˜∈L2(D;RN)andu˜∈HΓ1

0(0).

Hence we can deduce the following Euler conditions:

∂W

∂θ

zin,vni

ε τni

znizin1

∂H

zinzni1

, (5.4)

∂W

∂F

zin,vni + ε

τni

vni − ∇vin1 ,∇ ˜u

= lni,u˜

for everyu˜∈HΓ1

0(0). (5.5)

Conversely, conditions(5.4)and(5.5)imply that(zin, vni)is a solution of (5.1).

Proof. Since for everyz˜∈L2(D;Rm),u˜∈HΓ1

0(0)ands0,zni +sz˜∈L2(D;Rm)andvin+su˜∈A(tni), the mini- mality property of(zin, vni)leads to

W zin, vin

lni, vin

+H

zinzni1 + ε

nizinzin12

2+ ε

nivni − ∇vin12

2

W

zin+sz, v˜ in+su˜

lin, vin+su˜ +H

zin+sz˜−zin1 + ε

nizin+sz˜−zni12

2+ ε

nivni +s∇ ˜u− ∇vni12

2. (5.6)

Hence from the convexity ofHwe can deduce for everys∈ [0,1]

s H

zin+ ˜zzin1

H

zinzin1

W

zin, vni

W

zin+sz, v˜ in+su˜

lni, vin

+

lni, vni +su˜ + ε

nizinzin12

2ε

nizin+sz˜−zin12

2

+ ε

nivni − ∇vni12

2ε

nivni +s∇ ˜u− ∇vin12

2. (5.7)

Taking the derivative of (5.7) with respect tosats=0 we obtain (5.3). Foru˜=0, (5.3) is H

zin+ ˜zzin1

H

zinzin1

∂W

∂θ

zin,vin

ε τni

zinzin1 ,z˜

, for everyz˜∈L2(D;Rm), i.e. (5.4). Takingz˜=0 in (5.3) we obtain (5.5).

Conversely, (5.4) and (5.5) imply the minimality of(zin, vin), thanks to the strict convexity of the functional. 2 Remark 5.3.(5.4) is equivalent to

1 τni

zinzin1

=∂Hε

∂W

∂θ

zni,vni

. (5.8)

Indeed, since∂His positively homogeneous of degree 0, (5.4) can be rewritten as

∂W

∂θ

zin,vni

ε τni

znizin1

∂H 1

τni

znizni1 , which is equivalent to

∂W

∂θ

zin,vni

∂Hε

1 τni

zinzin1 .

This is equivalent to (5.8), thanks to a general duality formula (see, e.g., [6, Corollary I.5.2]).

(10)

Since A(tni)=ϕni +HΓ1

0(0), for every n and everyi=0,1, . . . , k(n), there exists uinHΓ1

0(0)such that vni = ϕni +uin.

Set, for everynand everyi=0,1, . . . , k(n), ζni:= −∂W

∂θ

zni,uin+ ∇ϕin , σni:=∂W

∂F

zin,uin+ ∇ϕni .

Let define the piecewise constant interpolations (zn,un):[0, T] →L2(D;Rm)×HΓ1

0(0) and n,σn):[0, T] → L2(D;Rm)×L2(D;RN×d)as

zn(t ):=zin, un(t ):=uin, ζn(t ):=ζni, σn(t ):=σni, fortni t < tni+1,

where we settnk(n)+1=T +1n. Setτn(t ):=tni whenevertni t < tni+1. We introduce also the piecewise affine in- terpolationszn :[0, T] →L2(D;Rm),un :[0, T] →HΓ1

0(0),ϕn:[0, T] →H1(D;RN),ln :[0, T] →H1(D;RN), defined by

zn(t ):=zin+

ttnizin+1zin tni+1tni , un(t ):=uin+

ttniuin+1uin tni+1tni , ϕn(t ):=ϕni +

ttniϕin+1ϕin tni+1tni , ln(t ):=lni +

ttnilni+1lni tni+1tni

(5.9)

fortni ttni+1.

Observe that, thanks to Remark 5.3 and to (3.7), we can obtain from (5.4) that zinzin1

tnitni1 =NKε ζni

. (5.10)

Analogously we can deduce from (5.5) that

σni+ε

uin− ∇uin1

tnitni+1 +∇ϕinϕni1 tnitni1

,∇ ˜u

= lin1,u˜

, (5.11)

for everyu˜∈HΓ1

0(0).

5.2. A priori estimates

Now we obtain an a priori bound on the piecewise constant interpolations, from an energy estimate for the solutions of the incremental problems.

Sinceuin1+ϕniA(tni), from the minimum property of(zin, uin+ϕni)we deduce the following inequality:

W

zin, uin+ϕni

lin, uin+ϕin +H

zinzni1 + ε

nizinzin12

2+ ε

niuin− ∇uin1+ ∇ϕni − ∇ϕni12

2

W

zin1, uin1+ϕni1

lni1, uin1+ϕin1 + ε

niϕin− ∇ϕni12

2

tni

tni1

˙l(s), uin1+ϕ(s) ds

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