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106    3. Finite Element Methods for Linear Elliptic Problems


        Indeed, using Theorem 3.13, we have

                     2         2                   2      2            2
         a(u, u) ≥ k 0 |u| + α 0  u dσ ≥ min{k 0 ,α 0 } |u| +  u dσ  ≥ C 5  u
                     1                             1                   1
                            ˜ Γ                         ˜ Γ
        with C 5 := C −2  min{k 0 ,α 0 }. Therefore, we obtain the existence and
                      F
        uniqueness of a solution analogously to Theorem 3.12.
        (III) General Case
        First, we consider the case of a homogeneous Dirichlet boundary
        condition on Γ 3 with |Γ 3 | d−1 > 0. For this, we define
                                   1
                        V := v ∈ H (Ω) : γ 0 (v)=0 on Γ 3 .         (3.30)
                                        1
        Here V is a closed subspace of H (Ω), since the trace mapping γ 0 :
                                                                    2
          1
                  2
                                                           2
        H (Ω) → L (∂Ω) and the restriction of a function from L (∂Ω) to L (Γ 3 )
        are continuous.
          Suppose u is a solution of (3.12), (3.18)–(3.20); that is, in the sense
                                           1 ¯
                                   2
        of classical solutions let u ∈ C (Ω) ∩ C (Ω) and the differential equation
        (3.12) be satisfied pointwise in Ω and the boundary conditions (3.18)–
        (3.20) pointwise on their respective parts of ∂Ω under the assumptions
                                                    2
        (3.13), (3.21). However, the weaker case that u ∈ H (Ω) and the differential
                                          2
        equation is satisfied in the sense of L (Ω) and the boundary conditions
                                               2
        (3.18)–(3.20) are satisfied in the sense of L (Γ j ),j =1, 2, 3, under the
        assumptions (3.14), (3.22) can also be considered here.
          As in (I), according to (3.11),

         a(u, v):=      {K∇u ·∇v + c ·∇uv + ruv} dx +    αuv dσ     (3.31)
                      Ω                                Γ 2

                 =   b(v):=   fv dx +    g 1 vdσ +  g 2 vdσ  for all v ∈ V.
                             Ω         Γ 1        Γ 2
        Under the assumptions (3.15), (3.22) the continuity of a and b, (3.25)) and
        ((3.24) can be proven analogously to (II).
        Conditions for V -Ellipticity of a
        For the verification of the V -ellipticity we again proceed similarly to (II),
        but now the boundary conditions are more complicated. Here we have for
        the convective term

                                1         2     1           2
                   c ·∇uudx = −      ∇· cu dx +         ν · cu dσ ,
                 Ω              2  Ω            2  Γ 1 ∪Γ 2
        and therefore

                                               1       2
               a(u, u)=        K∇u ·∇u + r − ∇· c u       dx
                            Ω                  2

                             1         2              1      2
                           +      ν · cu dσ +     α + ν · c u dσ .
                             2  Γ 1           Γ 2     2
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