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P. 63

2. Two-Point Boundary Value Problems
        50
                           h
                      n
                                           Rate of convergence
                                   E h
                      5
                                0.0058853
                          1/6
                                                 1.969
                                0.0017847
                          1/11
                     10
                          1/21
                                                 1.996
                                0.0004910
                     20
                     40
                          1/41
                                                 2.000
                                0.0001288
                                                 2.000
                          1/81
                     80
                                0.0000330
        TABLE 2.1. The table shows the maximum error measured at the grid points for
        several values of h.
        Later, we will return to the problem of determining the rate of convergence
        for this numerical method and prove that the observed rate of convergence
        in the present example holds for a wide class of functions f.

        2.2.3   Gaussian Elimination for Tridiagonal Linear Systems
        The purpose of this section is to derive a numerical algorithm which can
        be used to compute the solution of tridiagonal systems of the form (2.14),
        (2.15). Furthermore, we shall derive conditions which can be used to verify
        that a given system has a unique solution. These criteria and the algorithm
        developed in this section will be useful throughout this course. We warn
        the reader that this section may be a bit technical — in fact Gaussian
        elimination is rather technical — and we urge you to keep track of the
        basic steps and not get lost in the forest of indices.
          We consider a system of the form
                                     Av = b,                        (2.17)
        where the coefficient matrix A has the form
                                                       
                                        0    ...     0
                                  γ 1
                              α 1
                                              .      .
                                              .     .  
                             β 2  α 2  γ 2    .     .  
                                                       
                                  .    .      .
                                  .    .      .        
                       A =   0     .    .     .     0   .         (2.18)
                                                       
                            .    .
                            . .   .  .  β n−1  α n−1  γ n−1  
                                                        
                              0   ...   0     β n   α n
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