Page 43 - Determinants and Their Applications in Mathematical Physics
P. 43

28   3. Intermediate Determinant Theory

          Substituting the first line of (3.3.9 and the second line of (3.3.8),
                        n   n              2
                                          ∂ A
                  A =         a i 1 j 1 i 2 j 2
                                  a
                                      ∂a i 1 j 1  ∂a i 2 j 2
                      i 1 =1 i 2 =1
                        n   n

                                  a
                    =         a i 1 j 1 i 2 j 2  A i 1 i 2 ;j 1 j 2 ,  i 1 <i 2 and j 1 <j 2 .  (3.3.10)
                      i 1 =1 i 2 =1
          Continuing in this way and applying (3.3.7) in reverse,
                     n   n      n
                                                          r
                                                         ∂ A
                A =         ···   a i 1 j 1 i 2 j 2  ··· a i r j r
                                      a
                                                 ∂a i 1 j 1  ∂a i 2 j 2  ··· ∂a i r j r
                    i 1 =1 i 2 =1  i r =1
                     n   n     n

                  =         ···   a i 1 j 1 i 2 j 2  ··· a i r j r  A i 1 i 2 ...i r ;j 1 j 2 ...j r ,  (3.3.11)
                                      a
                    i 1 =1 i 2 =1  i r =1
          subject to the inequalities associated with (3.3.7) which require that the i s
          and j s shall be in ascending order of magnitude.
            In this multiple sum, those rth cofactors in which the dummy variables
          are not distinct are zero so that the corresponding terms in the sum are
          zero. The remaining terms can be divided into a number of groups according
          to the relative magnitudes of the dummies. Since r distinct dummies can
          be arranged in a linear sequence in r! ways, the number of groups is r!.
          Hence,
                                    (r! terms)

                                A =        G k 1 k 2 ...,k r  ,
          where

                               =
                       G k 1 k 2 ...k r          a i k 1 k 1  a i k 2 k 2
                                                     j     j
                                 i≤i k 1  <i k 2  <···<i k r  ≤n
                                                            .       (3.3.12)
                                       j A i k 1 k 2
                                 ··· a i k r k r  i  ···i k r  ;j k 1 k 2  ...j k r
                                                      j
          In one of these r! terms, the dummies i 1 ,i 2 ,...,i r are in ascending order
          of magnitude, that is, i s <i s+1 ,1 ≤ s ≤ r − 1. However, the dummies
          in the other (r! − 1) terms can be interchanged in such a way that the
          inequalities are valid for those terms too. Hence, applying those properties
          of rth cofactors which concern changes in sign,


                                           a
               A =                   σ r a i 1 j 1 i 2 j 2  ··· a i r j r  A i 1 i 2 ...i r ;j 1 j 2 ...j r ,
                   1≤i 1 <i 2 <···<i r ≤n
          where

                                     1   2   3  ···  r
                           σ r = sgn                    .           (3.3.13)
                                     i 1  i 2  i 3  ··· i r
          (Appendix A.2). But,

                                 a                          .
                           σ r a i 1 j 1 i 2 j 2  ··· a i r j r  = N i 1 i 2 ...i r ;j 1 j 2 ...j r
   38   39   40   41   42   43   44   45   46   47   48