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4.2 Vacancies and Self-Interstitials  •  107

              Figure 4.1  Two-dimensional representations of a vacancy
              and a self-interstitial.
              (Adapted from W. G. Moffatt, G. W. Pearsall, and J. Wulff, The
              Structure and Properties of Materials, Vol. I, Structure, p. 77.
              Copyright © 1964 by John Wiley & Sons, New York, NY.
              Reprinted by permission of John Wiley & Sons, Inc.)   Self-interstitial
                                                                                         Vacancy














               Scanning probe
               micrograph that
              shows a vacancy on
              a (111)-type surface
              plane for silicon.   defects. The necessity of the existence of vacancies is explained using principles of
              Approximately      thermodynamics; in essence, the presence of vacancies increases the entropy (i.e., the
              7,000,000 .
              (Micrograph courtesy   randomness) of the crystal.
              of D. Huang, Stanford   The equilibrium number of vacancies N y  for a given quantity of material (usually
              University.)       per meter cubed) depends on and increases with temperature according to
              Temperature
              dependence of the                           N y = N expa -  Q y  b                     (4.1)
              equilibrium number                                       kT
              of vacancies
                                 In this expression, N is the total number of atomic sites (most commonly per cubic me-
                                 ter), Q y  is the energy required for the formation of a vacancy (J/mol or eV/atom), T is
                                                              1
              Boltzmann’s constant  the absolute temperature in kelvins,  and k is the gas or Boltzmann’s constant. The value
                                                                             #
                                                       #
                                                                                                        2
                                                                     5
                                 of k is 1.38   10  23  J/atom K, or 8.62   10  eV/atom K, depending on the units of Q y .
                                 Thus, the number of vacancies increases exponentially with temperature—that is, as T
                                 in Equation 4.1 increases, so also does the term exp( Q y /kT). For most metals, the frac-
                                                                                                   4
                                 tion of vacancies N y /N just below the melting temperature is on the order of 10 —that
                                 is, one lattice site out of 10,000 will be empty. As ensuing discussions indicate, a number
                                 of other material parameters have an exponential dependence on temperature similar
                                 to that in Equation 4.1.
              self-interstitial     A  self-interstitial  is an atom from the crystal that is crowded into an interstitial
                                 site—a small void space that under ordinary circumstances is not occupied. This kind of
                                 defect is also represented in Figure 4.1. In metals, a self-interstitial introduces relatively
                  Tutorial Video:  large distortions in the surrounding lattice because the atom is substantially larger than
                 Computation of   the interstitial position in which it is situated. Consequently, the formation of this defect
                  the Equilibrium   is not highly probable, and it exists in very small concentrations that are significantly
                     Number of   lower than for vacancies.
                      Vacancies


              1 Absolute temperature in kelvins (K) is equal to  C   273.
              2                                                                            #
              Boltzmann’s constant per mole of atoms becomes the gas constant R; in such a case, R   8.31J/mol K.
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