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Complex Analysis and Differential Geometry




                    Notes              Usually the valencies of all tensors composing the tensor field are the same. Let them all
                                       be of type (r, s). Then if we choose some basis e , e , e , we can represent any tensor of our
                                                                             1  2  3
                                       tensor field as an array  X  1 i ...i r s   with r + s indices:
                                                            1. j ..j
                                                                        1 i ...i
                                                                X j1 1 i ...i s r   X  1 j ...j r s (P).
                                                                  . ..j
                                       The left hand side is a tensor since the fraction in right hand side is constructed by means
                                       of tensorial operations. Passing to the limit h  0 does not destroy the tensorial nature of
                                       this fraction since the transition matrices S and T are all time-independent.

                                       Differentiation with  respect to  external parameters is a  tensorial operation  producing
                                       new tensors from existing ones.
                                       The tensorial nature of partial derivatives established by theorem is a very useful feature.
                                   
                                       We can apply it to extend the scope of classical operations of vector analysis. Let’s consider
                                       the gradient, grad = . Usually the  gradient operator is applied to scalar fields, i.e. to
                                       functions  = (P) or  = (x , x , x ) in coordinate form:
                                                              1
                                                                 2
                                                                   3
                                                                         
                                                                a       .
                                                                 q
                                                                     q
                                                                          x q
                                       The  Laplace operator  is defined  as the  divergency applied  to a  vectorial gradient  of
                                   
                                       something, it is denoted by the triangle sign:  = div grad. From Laplace operator , we
                                       derive the following formula:
                                                                    3  3
                                                                        ij
                                                                   g   j .
                                                                          i
                                                                   i 1 j 1
                                                                   
                                                                      
                                       Denote by    the following differential operator:
                                                                     1  2
                                                                   =       . 
                                                                     2
                                                                    c  t 2
                                       Above operator is called the d’Alambert operator or wave operator. In general relativity
                                       upon introducing the additional coordinate x  = ct one usually rewrites the d’Alambert
                                                                            0
                                       operator in a form quite similar.
                                       And finally, let’s consider the rotor operator or curl operator (the term “rotor” is derived
                                       from “rotation” so that “rotor” and “curl” have approximately the same meaning). The
                                       rotor  operator is  usually applied  to a vector field  and produces  another vector  field:
                                       Y = rot X. Here is the formula for the r-th coordinate of rot X:

                                                                   3  3  3
                                                                                k
                                                                          ri
                                                           (rot X)r   g   j X .
                                                                            ijk
                                                                   i 1 j 1 k 1
                                                                        
                                                                     
                                                                   
                                   16.6 Keywords
                                                                                                        
                                   Cartesian coordinate system in space and hence can represent P by its radius-vector r  OP  and
                                                                                                      p
                                   by its coordinates x , x , x .
                                                     2
                                                  1
                                                       3
                                                                                   1
                                                                       2
                                                                                       3
                                                                                     2
                                                                          3
                                                                  1
                                                                            
                                                    X  1 i ...i r  X  1 i ...i r  (x  h,x ,x ) X  1 i ...i r (x ,x ,x )
                                   Partial derivatives   1 j ...j s   lim  1 j ...j s  1 j ...j s  ,  taken as a whole, form an
                                                     t   h 0            h
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