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122    3. Finite Element Methods for Linear Elliptic Problems


                     27λ i λ j λ k ,   i,j,k =1,...,d +1 ,i < j < k .
        Thus for d = 2 the value at the barycentre arises as a degree of freedom.
        This, and in general the a i,j,k , i<j <k, can be dropped if the ansatz
        space P is reduced (see [9, p. 70]).
          All finite elements discussed so far have degrees of freedom that are
        defined in convex combinations of the vertices. On the other hand, two
        regular d-simplices can be mapped bijectively onto each other by a unique
        affine-linear F,that is, F ∈P 1 such that as defining condition, the vertices
        of the simplices should be mapped onto each other. If we choose, besides
                                                        ˆ
        the general simplex K, the standard reference element K defined by (3.47),
                      ˆ
        then F = F K : K → K is defined by
                                 F(ˆx)= Bˆx + a 1 ,                 (3.57)

        where B =(a 2 − a 1 ,... ,a d+1 − a 1 ).
          Since for F we have

                    d+1        d+1                     d+1

                 F     λ i ˆa i  =  λ i F(ˆa i )for λ i ≥ 0 ,  λ i =1 ,
                    i=1        i=1                     i=1
        F is indeed a bijection that maps the degrees of freedom onto each other as
                                                                 ˆ
        well as the faces of the simplices. Since the ansatz spaces P and P remain
        invariant under the transformation F K , the finite elements introduced so
        far are (in their respective classes) affine equivalent to each other and to
        the reference element.
                                                        ˆ ˆ ˆ
        Definition 3.22 Two Lagrange elements (K, P, Σ), (K, P, Σ) are called
                                           ˆ
        equivalent if there exists a bijective F : K → K such that
            *                                           +

                                                       ˆ
                       ˆ
             F(ˆa) ˆa ∈ K generates a degree of freedom on K


                  =    a a ∈ K generates a degree of freedom on K

                                                                    (3.58)
             and
                     *                    +

              P   =    p : K → R p ◦ F ∈ P ˆ  .

        They are called affine equivalent if F is affine-linear.
          Here we have formulated the definition in a more general way, since in
        Section 3.8 elements with more general F will be introduced: For isopara-
        metric elements the same functions F as in the ansatz space are admissible
        for the transformation. From the elements discussed so far only the simplex
        with linear ansatz is thus isoparametric. Hence, in the (affine) equivalent
        case a transformation not only of the points is defined by
                                   ˆ x = F −1 (x) ,
                                                                     ˆ
                                                ˆ
        but also of the mappings, defined on K and K, (not only of P and P)is
        given by
                               ˆ
                           ˆ v : K → R ,  ˆ v(ˆx):= v(F(ˆx))
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