Quasilinear parabolic problems with nonlinear boundary conditions

Quasilinear parabolic problems with nonlinear boundary conditions Quasilinear parabolic problems with nonlinear boundary conditions

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which is necessary for v to be a solution of (4.40) on [0, Ti+1]. Let Zi+1 = H α p ([0, Ti+1]; Lp(Ω)) ∩ Lp([0, Ti+1]; H 2 p(Ω)) for i = 0, . . . , M − 1, and set as usual Z1(v 0 ) = {w ∈ Z1 : ∂ m t w|t=0 = ∂ m t f|t=0, if α > m + 1/p, m = 0, 1}, as well as Zi+1(v i ) := {w ∈ Zi+1 : w| [0,Ti] = v i } for i > 0, where v i denotes the unique solution of (4.40) on [0, Ti] determined in the ith time step. In similar fashion as in the proofs of Theorem 4.1.1 and Theorem 4.2.3, one can now show that for each i = 0, . . . , M − 1, the mapping G leaves Zi+1(v i ) invariant and is a strict contraction, provided that δ is small enough. In fact, one uses the estimates derived in the above proofs together with the diffeomorphism property of the coordinate transformations ¯x = ˜ ϑj(x). Observe that we have uniform bounds for |Θj| and |Θ −1 j | w.r.t. i and j, as only the spatial variables are transformed and by compactness of Γ. So for sufficiently small δ, equation (4.52) admits a unique solution v =: Qi+1(f, g, h) in the space Zi+1(v i ). To see that this function indeed solves (4.40) on [0, Ti+1], one can again argue as in the proofs of Theorem 4.1.1 and Theorem 4.2.3. Here one has to consider the linear operators Ki+1 defined by + = N� � N1 Ki+1(f1, f2, f3) = (K (1) i+1 (f1, f2, f3), 0 , K (3) i+1 (f1, f2, f3)) � [A, ψj] h F ij(f1, Qi+1(f1, f2, f3)) + j=0 N2 � j=N1+1 [A, ψj] h j=N2+1 N ij (f1, f3, Qi+1(f1, f2, f3)), 0 , γΓN j=N2+1 [A, ψj] h D ij (f1, f2, Qi+1(f1, f2, f3)) N� [B, ψj] h N � ij (f1, f3, Qi+1(f1, f2, f3)) , for triples (f1, f2, f3) in the product space of the regularity classes of f, g, h whose temporal traces at t = 0 coincide with those of f, g, h (including the first temporal derivative) whenever these traces exist. Since Ki+1 contains only terms of lower order, one can prove existence of a triple (f1, f2, f3) satisfying (f1, f2, f3)+Ki+1(f1, f2, f3) = (f, g, h), provided that δ is sufficiently small. By simple computations, one shows then that Qi+1(f1, f2, f3) solves (4.40) on [0, Ti+1]. Finally, uniqueness implies v = Qi+1(f, g, h) = Qi+1(f1, f2, f3). This establishes the sufficiency part. We turn now to necessity. Suppose that v ∈ Z solves (4.40). Clearly, ϕjv ∈ Z for all j = 0, . . . , N, which in turn implies Θ −1 j (ϕjv) ∈ Hα p (J; Lp(R n+1 + )) ∩ Lp(J; H2 p(R n+1 + )) for all j = N1 + 1, . . . , N. Observe further that all those terms on the right-hand sides of (4.48), (4.50), and the first equation of (4.46) (i = M − 1) which involve the function v have the regularity desired for the corresponding inhomogeneity (f, g resp. h) on J × Rn+1 resp. J × R n+1 + . In view of the Theorems 4.1.1, 4.2.3, 4.2.4, and the diffeomorphism property of the variable transformations ¯x = ˜ ϑj(x), it thus follows that the functions ϕjf, ϕjg, and ϕjh enjoy the desired regularity on J ×Ω, J ×ΓD, and J ×ΓN, respectively, for each j. On account of �N j=0 ϕj(x) ≡ 1 on Ω, we eventually obtain the desired regularity for the data f, g, h themselves. The compatibility conditions can be seen in the same way. � 78

Chapter 5 Linear Viscoelasticity In this chapter we shall study a linear parabolic problem of second order which arises in the theory of viscoelasticity. In comparison to the problems investigated in the previous chapter, it has two new challenging features: (1) it is a vector-valued problem, and (2) it contains two independent kernels. As before we shall characterize unique existence of the solution in a certain class of optimal Lp-regularity in terms of regularity and compatibility conditions on the given data. The chapter is organized as follows. At first we recall the model equations from linear viscoelasticity, here following the presentation given in Prüss [63, Section 5]. In the second part we state the problem and discuss the assumptions on the kernels. The third and main part of this chapter is devoted to the thorough investigation of a half space case of the problem. For a derivation of the fundamental equations of continuum mechanics and of linear viscoelasticity, we further refer to the books by Christensen [12], Gurtin [41], Pipkin [62], and Gripenberg, Londen, Staffans [39]. 5.1 Model equations Let Ω ⊂ R 3 be an open set with boundary ∂Ω of class C 2 . The set Ω shall represent a body, i.e. a solid or fluid material. Acting forces lead to a deformation of the body, displacing every material point x ∈ Ω at time t to the point x + u(t, x). The vector field u : R × Ω → R 3 is called the displacement field, or briefly displacement. The velocity v(t, x) of the material point x ∈ Ω at time t is then given by v(t, x) = ˙u(t, x), the dot indicating partial derivative w.r.t. t. The deformation of the body induces a strain E(t, x), which will depend linearly on the gradient ∇u(t, x), provided that the deformation is small enough. We will put E(t, x) = 1 2 (∇u(t, x) + (∇u(t, x))T ), t ∈ R, x ∈ Ω, (5.1) i.e. E is the symmetric part of the displacement gradient ∇u. The strain in turn causes stress in a way which has to be specified, expressing the properties of the material the body is made of. The stress is described by the symmetric tensor S(t, x). If ρ denotes the mass density and assuming that it is time independent, i.e. ρ(t, x) = ρ0(x), the balance of momentum law implies ρ0(x)ü(t, x) = div S(t, x) + ρ0(x)f(t, x), t ∈ R, x ∈ Ω, (5.2) 79

which is necessary for v to be a solution of (4.40) on [0, Ti+1].<br />

Let Zi+1 = H α p ([0, Ti+1]; Lp(Ω)) ∩ Lp([0, Ti+1]; H 2 p(Ω)) for i = 0, . . . , M − 1, and set<br />

as usual Z1(v 0 ) = {w ∈ Z1 : ∂ m t w|t=0 = ∂ m t f|t=0, if α > m + 1/p, m = 0, 1}, as well as<br />

Zi+1(v i ) := {w ∈ Zi+1 : w| [0,Ti] = v i } for i > 0, where v i denotes the unique solution of<br />

(4.40) on [0, Ti] determined in the ith time step. In similar fashion as in the proofs of<br />

Theorem 4.1.1 and Theorem 4.2.3, one can now show that for each i = 0, . . . , M − 1, the<br />

mapping G leaves Zi+1(v i ) invariant and is a strict contraction, provided that δ is small<br />

enough. In fact, one uses the estimates derived in the above proofs together <strong>with</strong> the<br />

diffeomorphism property of the coordinate transformations ¯x = ˜ ϑj(x). Observe that we<br />

have uniform bounds for |Θj| and |Θ −1<br />

j | w.r.t. i and j, as only the spatial variables are<br />

transformed and by compactness of Γ. So for sufficiently small δ, equation (4.52) admits<br />

a unique solution v =: Qi+1(f, g, h) in the space Zi+1(v i ). To see that this function<br />

indeed solves (4.40) on [0, Ti+1], one can again argue as in the proofs of Theorem 4.1.1<br />

and Theorem 4.2.3. Here one has to consider the linear operators Ki+1 defined by<br />

+<br />

=<br />

N�<br />

� N1<br />

Ki+1(f1, f2, f3) = (K (1)<br />

i+1 (f1, f2, f3), 0 , K (3)<br />

i+1 (f1, f2, f3))<br />

�<br />

[A, ψj] h F ij(f1, Qi+1(f1, f2, f3)) +<br />

j=0<br />

N2 �<br />

j=N1+1<br />

[A, ψj] h<br />

j=N2+1<br />

N ij (f1, f3, Qi+1(f1, f2, f3)), 0 , γΓN<br />

j=N2+1<br />

[A, ψj] h D ij (f1, f2, Qi+1(f1, f2, f3))<br />

N�<br />

[B, ψj] h N �<br />

ij (f1, f3, Qi+1(f1, f2, f3)) ,<br />

for triples (f1, f2, f3) in the product space of the regularity classes of f, g, h whose temporal<br />

traces at t = 0 coincide <strong>with</strong> those of f, g, h (including the first temporal derivative)<br />

whenever these traces exist. Since Ki+1 contains only terms of lower order, one can prove<br />

existence of a triple (f1, f2, f3) satisfying (f1, f2, f3)+Ki+1(f1, f2, f3) = (f, g, h), provided<br />

that δ is sufficiently small. By simple computations, one shows then that Qi+1(f1, f2, f3)<br />

solves (4.40) on [0, Ti+1]. Finally, uniqueness implies v = Qi+1(f, g, h) = Qi+1(f1, f2, f3).<br />

This establishes the sufficiency part.<br />

We turn now to necessity. Suppose that v ∈ Z solves (4.40). Clearly, ϕjv ∈ Z for<br />

all j = 0, . . . , N, which in turn implies Θ −1<br />

j (ϕjv) ∈ Hα p (J; Lp(R n+1<br />

+ )) ∩ Lp(J; H2 p(R n+1<br />

+ ))<br />

for all j = N1 + 1, . . . , N. Observe further that all those terms on the right-hand<br />

sides of (4.48), (4.50), and the first equation of (4.46) (i = M − 1) which involve the<br />

function v have the regularity desired for the corresponding inhomogeneity (f, g resp.<br />

h) on J × Rn+1 resp. J × R n+1<br />

+ . In view of the Theorems 4.1.1, 4.2.3, 4.2.4, and the<br />

diffeomorphism property of the variable transformations ¯x = ˜ ϑj(x), it thus follows that<br />

the functions ϕjf, ϕjg, and ϕjh enjoy the desired regularity on J ×Ω, J ×ΓD, and J ×ΓN,<br />

respectively, for each j. On account of �N j=0 ϕj(x) ≡ 1 on Ω, we eventually obtain the<br />

desired regularity for the data f, g, h themselves. The compatibility <strong>conditions</strong> can be<br />

seen in the same way. �<br />

78

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