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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problem<br />
⎧<br />
⎪⎨<br />
⎪⎩<br />
∂tv − da ∗ (∆xv + ∂2 yv) − (db + 1<br />
∂tw − da ∗ ∆xw − (db + 4<br />
3da) ∗ ∂2 yw − (db + 1<br />
3da) ∗ (∇x∇x · v + ∂y∇xw) = fv (J × R n+1<br />
+ )<br />
3da) ∗ ∂y∇x · v = fw (J × R n+1<br />
+ )<br />
−da ∗ γ∂yv − da ∗ γ∇xw = gv (J × Rn )<br />
−(db − 2<br />
3 da) ∗ γ∇x · v − (db + 4<br />
3 da) ∗ γ∂yw = gw (J × R n )<br />
v|t=0 = v0 (R n+1<br />
+ )<br />
w|t=0 = w0 (R n+1<br />
+ ),<br />
(5.12)<br />
where γ denotes the trace operator at y = 0. We seek a unique solution (v, w) of (5.12)<br />
in the regularity class<br />
Z := (H δa<br />
p (J; Lp(R n+1<br />
+ )) ∩ Lp(J; H 2 p(R n+1<br />
+ )))n+1 .<br />
5.3.1 The case δa ≤ δb: necessary <strong>conditions</strong><br />
In this and the following subsection, we assume that δa ≤ δb. On the basis of the results<br />
in Section 3.5, we first derive necessary <strong>conditions</strong> for the existence of a solution (v, w)<br />
of (5.12) in the space Z.<br />
Suppose that we are given such a solution. By Corollary 2.8.1, it then follows imme-<br />
diately that<br />
(fv, fw) ∈ (H δa−1<br />
p (J; Lp(R n+1<br />
+ )))n+1 . (5.13)<br />
Taking the temporal trace of (v, w) and (∂tv, ∂tw), respectively, at t = 0 gives according<br />
to Theorem 3.5.2 (see also the results from Chapter 4)<br />
and<br />
in case δa > 1 + 1/p. Putting<br />
(v0, w0) ∈ (B<br />
(fv, fw)|t=0 ∈ (B<br />
δa (1− 2<br />
Y = B<br />
1<br />
p )<br />
pp<br />
1<br />
2(1− pδa )<br />
pp<br />
(R n+1<br />
1 1<br />
2(1− − δa pδa )<br />
pp<br />
+ ))n+1 , (5.14)<br />
(R n+1<br />
(J; Lp(R n )) ∩ Lp(J; B<br />
+ ))n+1<br />
1<br />
1− p<br />
pp (R n ))<br />
Theorem 3.5.2 further yields (γ∂yv, γ∇xw, γ∂yw, γ∇x · v) ∈ Y 2n+2 . So if we set<br />
φ = −γ∂yv − γ∇xw,<br />
then it follows from the first <strong>boundary</strong> condition in (5.12) that gv is of the form<br />
(5.15)<br />
gv = da ∗ φ, <strong>with</strong> φ ∈ Y n . (5.16)<br />
δa (1− 2<br />
As, in case p > 1 + 2/δa, we have the embedding B<br />
1<br />
p )<br />
pp (J; Lp(Rn )) ↩→ C(J; Lp(Rn )),<br />
we see that φ satisfies in addition the compatibility condition<br />
φ|t=0 = −γ∂yv0 − γ∇xw0, if p > 1 + 2 . (5.17)<br />
δa<br />
Turning to the second <strong>boundary</strong> condition in (5.12), we put<br />
ψ1 = 2<br />
3 γ∇x · v − 4<br />
3 γ∂yw, ψ2 = −γ∇x · v − γ∂yw.<br />
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