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Free and Bound Electrons, Dimensionality Effects
                             • the excited electron bounces back to its ground state, emitting a pho-
                               ton.
                             All those processes require the transitions of electrons between different
                             electronic states. The scenario described above is what happens in a gas
                             discharge lamp. The analogous process can be found in the conduction
                             band of a semiconductor where an electron is hitting a defect atom that
                             has a spectrum of localized electronic states below the conduction band-
                             edge. The energy scale is of course one order of magnitude lower and
                             there are additional degrees of freedom to which the excess energy of the
                             electron may be transferred, e.g., phonons.


                             The quantum mechanical description of the electron as given above
                             focused on the stationary states of the electrons. Now the time depen-
                             dence of the Schrödinger equation has must be exploited.


                             3.2.7 Transitions Between Electronic States
                             The superposition of the time–dependent solutions of the Schrödinger
                             equation (3.16) gives the general form of the wavefunction with arbitrary
                             initial conditions

                                         Ψ x t,(  ) =  ∑ c exp  – (  iω t)ψ x()   (3.70)
                                          0
                                                              n
                                                                  n
                                                      n
                                                    n
                             where  ω =  E ⁄  —   and the  ψ x()   in (3.70) are the solution of the sta-
                                    n
                                                     n
                                         n
                             tionary eigen-value problem
                                                  ˆ
                                                 H 0 ψ =  E ψ                     (3.71)
                                                     n    n  n
                             The coefficients  c   are determined by the initial condition, i.e.,
                                             n
                                       |
                                          (
                                            ,
                                         0
                             c =  〈 ψ x() Ψ x 0)〉  . The superscript 0 of the wavefunction and the
                              n     n
                             subscript 0 of the Hamiltonian indicate the unperturbed stationary prob-
                             lem.

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