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3.9 Direct Boundary Integral Equations  147

                           Definition 3.9.1. The boundary value problem is called a regular elliptic
                            boundary value problem if P in (3.9.1) is elliptic and the boundary con-
                           ditions in (3.9.2) are normal and satisfy the Lopatinski–Shapiro conditions.
                           In order to have a regular elliptic boundary value problem (see H¨ormander
                           [130], Wloka [322]) we require in addition to the fundamental assumption,
                           i.e. normal boundary conditions, that the Lopatinski–Shapiro condition is
                           fulfilled (see [322, Chap.11]). This condition reads as follows:
                           Definition 3.9.2. The boundary conditions (3.9.3) for the differential op-
                           erator in (3.9.1) are said to satisfy the Lopatinski–Shapiro conditions if the
                           initial value problem defined by the constant coefficient ordinary differential
                           equations
                                         2m
                                                              k
                                             (2m)
                                                         d

                                            P    (x, iξ )     χ(σ n )=0 for 0 <σ n      (3.9.6)
                                             k
                                                        dσ n
                                        k=0
                           together with the initial conditions
                                                          k−1
                                                   λ  d
                                        r jkλ (x)(iξ )       χ | σ n =0  =0 for j =1,...,m  (3.9.7)
                                                     dσ n
                               |λ|=µ j −k−1
                           and the radiation condition χ(σ n )= o(1) as σ n →∞ admits only the trivial


                           solution χ(σ n )=0 for every fixed x ∈ Γ and every ξ ∈ IR n−1  with |ξ | =1.
                           Here, the coefficients in (3.9.6) are given by the principal part of P in local
                           coordinates via (3.4.50) as
                                      (2m)                                         γ


                                     P    (x, ξ ):=             a α (x)c α,γ,k (σ , 0)(iξ ) ;
                                      k
                                                  |γ|≤2m−k |α|=2m
                           and the coefficients in (3.9.7), from the tangential boundary operators in
                           (3.9.2) in local coordinates are given by
                                                                          λ
                                                                      ∂
                                              R jk =         r jkλ (x)     .
                                                                     ∂σ
                                                    |λ|≤µ j −k−1
                              The case of more general boundary conditions in which the orders µ j
                           for the different components u   of u are different, with corresponding given
                           components ϕ jt of ϕ j , was treated by Grubb in [109]. Here the boundary
                           conditions have the form
                                        p  µ j  +1
                                                            t        λ
                                                           r jkλ (x)(iξ ) γ k−1 u   = ϕ jt ,  (3.9.8)
                                        =1  k=1  |λ|=µ j  −k−1
                                                                        m

                                      t =1,...,q j ≤ p, j =1,...,m and    q j = m · p.
                                                                       j=1
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