Page 171 - Intro to Tensor Calculus
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                   For these nonvanishing components only one independent component exists. By convention, the com-
                   ponent R 1212 is selected as the single independent component and all other nonzero components are
                   expressed in terms of this component.
                   Find the nonvanishing independent components R ijkl for i, j, k, l =1, 2, 3, 4and show that


                                                 R 1212  R 3434  R 2142  R 4124
                                                 R 1313  R 1231  R 2342  R 4314

                                                 R 2323  R 1421  R 3213  R 4234
                                                 R 1414  R 1341  R 3243  R 1324
                                                 R 2424  R 2132  R 3143  R 1432

               can be selected as the twenty independent components.
              I 21.
                (a) For N =2 show R 1212 is the only nonzero independent component and
                   R 1212 = R 2121 = −R 1221 = −R 2112 .
                                                                                  2
                                                                               2
                (b) Show that on the surface of a sphere of radius r 0 we have R 1212 = r sin θ.
                                                                               0
              I 22.  Show for N =2 that
                                                                            2
                                                              2          ∂x
                                                 R 1212 = R 1212 J = R 1212
                                                                        ∂x

                                                            i
                                                                    1 i
                                                                                                    i
                                                                 i
                                                                                                        ik
              I 23.  Define R ij = R s .ijs  as the Ricci tensor and G = R − δ R as the Einstein tensor, where R = g R kj
                                                                    2 j
                                                                                                    j
                                                            j
                                                                 j
                         i
               and R = R . Show that
                         i
                                            ab
                                 (a)  R jk = g R jabk
                                            2
                                           ∂ log  √ g     b     ∂ log  √ g  ∂     a        b      a
                                 (b) R ij =         −              −           +
                                              i
                                            ∂x ∂x j    ij    ∂x b    ∂x a  ij     ia    jb
                                 (c)  R i ijk  =0
              I 24.  By employing the results from the previous problem show that in the case N =2 we have
                                                  R 11  R 22  R 12    R 1212
                                                      =     =     = −
                                                  g 11  g 22  g 12      g
               where g is the determinant of g ij .
              I 25.  Consider the case N = 2 wherewehave g 12 = g 21 = 0 and show that
                                                                       2R 1221
                           (a)    R 12 = R 21 =0            (c)    R =
                                                                       g 11 g 22
                           (b)    R 11 g 22 = R 22 g 11 = R 1221         1                   ij
                                                            (d)    R ij =  Rg ij ,  where  R = g R ij
                                                                         2
                                                                                              i
                                                                                                       1 i
                                                                                                   i
               The scalar invariant R is known as the Einstein curvature of the surface and the tensor G = R − δ R is
                                                                                              j    j   2 j
               known as the Einstein tensor.
              I 26.    For N =3 show that R 1212 ,R 1313 ,R 2323 ,R 1213 ,R 2123 ,R 3132 are independent components of the
               Riemann Christoffel tensor.
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