Page 362 - Numerical Methods for Chemical Engineering
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Brownian dynamics and SDEs                                          351



                    Some care must be taken if the diffusivity is itself a function of position, as the correct
                  microscopic balance for the concentration field is
                                        ∂c     ∂         ∂      ∂c
                                           =−    [J c c] +  D(x)                    (7.204)
                                        ∂t     ∂x       ∂x      ∂x
                  Applying the chain rule,
                                      ∂ ∂         ∂     ∂c     ∂     dD
                                           [Dc] =    D     +     c                  (7.205)
                                     ∂x ∂x       ∂x    ∂x    ∂x    dx
                  we rewrite (7.204) as the correct form of the Fokker–Planck equation for a position-
                  dependent diffusivity D(x):
                                  ∂c     ∂         dD        ∂ 2
                                     =−       J c +    c +     [D(x)c(t, x)]        (7.206)
                                  ∂t     ∂x        dx       ∂x 2
                  The corresponding Langevin equation is
                                                  dD             1/2
                                                     1
                                     dx = J c (x) +    dt + [2D(x)]  dW t           (7.207)
                                                  dx
                  The additional deterministic contribution from the position-dependent diffusivity is known
                  as spurious drift.

                  The Einstein relation

                  We are now ready to derive the proper relationship between the drag constant ζ and the
                  diffusivity D. If the diffusion is constant, the Fokker–Planck equation (7.202) takes the
                  form
                                                1
                                       ∂p    ∂       dU           ∂p
                                          =             p(t, x) + D                 (7.208)
                                       ∂t   ∂x  ζ   dx            ∂x
                  As t →∞, the system approaches a stable steady state for D > 0 at which

                                         d  1   dU          dp
                                                     p(x) + D    = 0                (7.209)
                                        dx  ζ   dx          dx
                  Integrating yields
                                      1    dU         dp
                                              p(x) + D   = constant = 0             (7.210)
                                      ζ   dx          dx
                  In the latter equality we use the fact that since the probability field is conserved (there is no
                  source term), the net flux (convective and diffusive) is zero everywhere at the steady state.
                  We want this condition to be satisfied by the equilibrium Boltzmann distribution (7.180).
                  Taking the derivative of p eq (x) yields

                   dp eq  d     −1     U(x)   1   −1     1 dU        U(x)       1 dU
                       =     Z   exp −        = Z    −         exp −       =−         p eq
                   dx    dx             k b T          k b T dx       k b T    k b T dx
                                                                                    (7.211)
                  Substituting this into the no-flux condition (7.210) we obtain
                           1     dU           1 dU    1      dU     1  D
                       0 =         p eq + D −      p eq =          −       p eq     (7.212)
                          ζ   dx             k b T dx       dx    ζ   k b T
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