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Applications of the Bose-Einstein Distributions
                             The normal vibrations of the crystal lattice as described in Chapter 2 may
                Lattice      5.3 Applications of the Bose-Einstein Distributions
                Vibrations   be described as set of linear non-interacting harmonic oscillators when
                             neglecting the nonlinear interaction between the lattice atoms. Each of
                             these oscillators   has a specific frequency  ω   and each of the phonons
                                          i
                                                                  i
                             contributes with an energy hω  . With n   phonons present frequency ω
                                                     i       i                        i
                             we have a contribution of E =  n hω   to the energy contained in that lat-
                                                   i   i  i
                             tice vibration mode.
                Photons      For photons, the situation looks alike and the only constraint on the parti-
                                                             β
                             tion function is given by the parameter  , the temperature, which deter-
                             mines the average energy of the system. There is no prescribed number
                                                   i
                             of particles for a single sate   in either cases of photons or phonons. Any
                             number of photons or phonons may occupy a given energy level. For this
                             case the partition function reads
                                                               ∞
                                  Z =  ∑  exp  – (  βΣ n E[  i i  i k  ∏ ∑  exp  – (  βE n )
                                                      ] ) =
                                                                          i i
                                        k                   i  n i =  0           (5.34)
                                                         1
                                                 =  ∏  --------------------
                                                          –
                                                        –
                                                           βE i
                                                     i  1 e
                             From (5.34) we can calculate the average number of particles with
                             energy E
                                    i
                                               ∂
                                              1  lnZ    e – βE j   1
                                        n =  – ---------------- =  -------------------- =  ------------------  (5.35)
                                         j
                                                ∂
                                              β E         – βE j  βE j
                                                        –
                                                  j   1 e        e  –  1
                Planck       which is the well known Planck distribution for photons. It gives the sta-
                Distribution  tistical occupation number of a specific energy level for a photonic sys-
                             tem. Consider a piece of material at a specific temperature, i.e., with
                                  β
                             given  . Then (5.35) describes the intensity distribution of the irradiated
                             electromagnetic spectrum with respect to the frequency (note that the
                             energy of the electromagnetic wave is proportional to its frequency.) Of
                             course this is a non-equilibrium situation. Strictly, we also have to take


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