Page 280 - Electrical Properties of Materials
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262                           Magnetic materials

                                     At normal temperatures and reasonable magnetic fields, a   1 and
                                   eqn (11.14) may be expanded to give
                                                                   2
                                                               N m μ μ 0 H
                                                                   m
                                                           M =          ,                  (11.15)
                                                                 3k B T
                                   leading to

                                                                    2
     Here χ m is definitely positive and                         N m μ μ 0
                                                                    m
     varies inversely with temperature.                    χ m =  3k B T  .                (11.16)
                                     At the other extreme of very low temperatures all the magnetic dipoles line
                                   up; this can be seen mathematically from the fact that the function L(a) (plotted
     1.0  L(a)                     in Fig. 11.2) tends to unity for large values of a. The total magnetic moment
                                   is then

                                                             M s = N m μ m ,               (11.17)
     0.5
                                   which is called the saturation magnetization, because this is the maximum
                                   contribution the material can provide.
     0.0                             We have now briefly discussed two distinct cases: (i) when the induced mag-
       0      2     4     6   a
                                   netic moment opposes the magnetic field, called diamagnetism; and (ii) when
                                   the aligned magnetic moments strengthen the magnetic field, called paramag-
     Fig. 11.2
                                   netism. Both phenomena give rise to small magnetic effects that are of little
     The Langevin function, L(a).
                                   use when the aim is the production of high magnetic fluxes. What about our
                                   most important magnetic material, iron? Can we explain its properties with the
                                   aid of our model? Not in its present state. We have to modify our model by in-
                                   troducing the concept of the internal field. This is really the same sort of thing
                                   that we did with dielectrics. We said then that the local electric field differs
                                   from the applied electric field because of the presence of the electric dipoles
                                   in the material. We may argue now that in a magnetic material the local mag-
                                   netic field is the sum of the applied magnetic field and the internal magnetic
                                   field, and we may assume (as Pierre Weiss did in 1907) that this internal field
                                   is proportional to the magnetization, that is
     λ is called the Weiss constant.                         H int = λM.                   (11.18)

                                     Using this newly introduced concept of the internal field, we may replace H
                                   in eqn (11.13) by H + λM to obtain for the magnetization,

                                                       M      	  μ m μ 0
                                                           = L       (H + λM) .            (11.19)
                                                     N m μ m    k B T
                                   Thus for any given value of H we need to solve eqn (11.19) to get the cor-
                                   responding magnetization. It is interesting to note that eqn (11.19) still has
                                   solutions when H = 0. To prove this, let us introduce the notations,
                                                                           2
                                               b = μ m μ 0 λM/k B T,  θ = N m μ μ 0 λ/3k B ,  (11.20)
                                                                           m
                                   and
                                                      M     Tμ m μ 0 λM/k B T  Tb
                                                          =                =   .           (11.21)
                                                                 2
                                                    N m μ m  3N m μ μ 0 λ/3 k B  3θ
                                                                 m
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