Page 220 - Semiconductor For Micro- and Nanotechnology An Introduction For Engineers
P. 220

Local Equilibrium Description
                             field drops out. Thus for the inclusion of magnetic field dependence in
                             (6.30) higher order terms must be considered. Neglecting the whole
                             streaming motion term of  δf   was therefore a too restrictive approxima-
                             tion. To this end, we keep the keep the gradient with respect to k from the
                             streaming motion part

                                                f ∂
                                                 0
                                        δf =  – τ---------  v∇η +  q  B)∇ δf    (6.68)
                                                          --- v ×(
                                               ∂ E       —        k  
                             where we assumed the isothermal case, hence the temperature gradient
                             vanishes. Equation (6.68) can be solved iteratively by replacing ∇ δf   by
                                                                                 k
                             a series expansion in ascending powers of  . Then we have to the lowest
                                                               B
                             order

                                               f ∂  ∇η +  ( s ×  ∇η) +  ss∇η)
                                                                  (
                                                0
                                      δf =  – τ---------v------------------------------------------------------------------  (6.69)
                                              ∂ E              2
                                                           1 +  s
                                       (
                                                                    ⁄
                             with  s =  qτ m∗ ) – 1 B  , where we used v =  —k m∗  . For the case of an
                                              (
                             anisotropic material,  m∗ ) – 1   is the inverse of the mass tensor M
                                                     m   0   0
                                                       1
                                               M =    0 m    0                    (6.70)
                                                          2
                                                      0  0 m
                                                             3
                             where we assumed the effective mass tensor to be diagonal. This means,
                             furthermore, that in the iterative solution (6.69) all tensorial terms con-
                             taining the effective mass have to be maintained. In this case we obtain

                                                                  2 2
                                                                q τ
                                                         –
                                                          1
                                         f ∂  ∇η +  qτ B ×(  M ∇η) +  ---------- B∇η(  )MB
                                                                 M
                                          0
                                δf =  – τ------------------------------------------------------------------------------------------------------------------  (6.71)
                                        ∂ E               q τ
                                                           2 2
                                                       1 +  ----------BMB
                                                           M
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