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138     3 Matrix eigenvalue analysis



                   compute the energy states of a single electron in a 1-D external potential field that has the
                   spatial periodicity
                                     V (x + n2P) = V (x)  n = 0, ±1, ±2,...          (3.202)

                   Such a periodic system may be interpreted to be a 1-D “crystal.”
                                                                   2
                   The probability of finding an electron in [x, x + dx]is |ψ(x)| dx, where ψ(x)isthe wave-
                   function of the electron, satisfying the Schr¨odinger equation,
                                               2
                                           h ¯ 2  d ψ
                                        −        2  + V (x)ψ(x) = Eψ(x)              (3.203)
                                          2m e dx
                                             ¯
                   m e is the mass of an electron and h = h/2π where h is Planck’s constant. E is the energy of
                   the electron. For a more detailed discussion, consult Leach (2001) and Atkins & Friedman
                   (1989).


                   Numerical solution of a differential equation eigenvalue problem
                   In (3.203), we have a differential equation eigenvalue problem, but we have been study-
                   ing techniques to solve matrix eigenvalue problems. To convert this problem into a matrix
                   one, we expand ψ(x) as a linear combination of basis functions that satisfy the appro-
                   priate boundary conditions; here the periodicity condition ψ(x + n2P) = ψ(x), since
                   if V(x) is periodic, we expect ψ(x) to be also. We choose a plane wave basis set with
                   members

                                       χ m (x) = e iq m x  = cos(q m x) + i sin(q m x)  (3.204)

                   The reasoning behind this choice of basis set is discussed in Chapter 9. Periodicity is satisfied
                   if the allowable wavenumbers q m satisfy
                                               mπ
                                          q m =     m = 0, ±1, ±2,...                (3.205)
                                               P
                   Using this basis, we write a trial form of the wavefunction as
                                               N             N
                                              	             	       iq m x
                                      ψ(x) =      b m χ m (x) =  b m e               (3.206)
                                             m=−N           m=−N
                   We wish to compute the coefficients {b m } that satisfy (3.203) best and thus truncate the
                   expansion to order N to make the problem dimension finite. Substituting this expansion into
                   (3.203), we have
                           N             2                        N
                          	         h ¯ 2  d
                              b m −       χ m (x) + V (x)χ m (x) = E  b m χ m (x)    (3.207)
                                   2m e dx 2
                         m=−N                                   m=−N
                   We now multiply this differential equation by the complex conjugates of each basis function,
                    ∗
                   χ (x), to obtain a set of equations:
                    n
                      N              ¯ 2  2                       N
                     	              h   d
                             ∗                                          ∗
                          b m χ (x) −     2  χ m (x) + V (x)χ m (x) = E  b m χ (x)χ m (x)  (3.208)
                                                                        n
                             n
                     m=−N           2m c dx                     m=−N
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