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132    CHAPTER 6  Laser-assisted cancer treatment




                         6.1.1  Mie theory
                         This theory was introduced by Gustav Mie in 1908 [1]. This model is the analytical
                         solution of Maxwell’s equations to calculate the scattering properties of spherical
                         and nonmagnetic particles. Maxwell equations are:
                                                                 ( ) t,
                                                              ∂Er
                                                     ( ) =t,
                                                ∇ × Hr    ε () r    ,                    (6.1)
 ∇×Hr,t=εpr∂Er,t∂t,                                        p    ∂t
                                                              ∂Hr
                                                                 ( ) t,
                                                ∇ × Er     µ() r     ,                   (6.2)
                                                    ( ) = −t,
 ∇×Er,t=−µr∂Hr,t∂t,                                              ∂t
                                                         ( ) =t,
 ∇⋅Er,t=0,                                           ∇⋅Er      0,                        (6.3)
                                                         ( ) =t,
 ∇⋅Hr,t=0,                                           ∇⋅ Hr     0,                        (6.4)
 εp  µ                   where H, E, ε , and µ are the magnetic field, the electric field, the electric permittiv-
                                    p
                         ity, and the magnetic permeability, respectively. By applying Fourier transform to the
                         Eq. (6.4), the time variable in electromagnetic field meets the Helmholtz equations
                         [1]:
                                                           2
                                                      2
 2
 ∇ E+ k12E=0,                                       ∇ E  + k E  = 0,                     (6.5)
                                                           1
                                                      2
                                                           2
 ∇ H+k12E=0,                                        ∇ H  + k E  = 0,                     (6.6)
 2
                                                           1
                                             () =
                                             2
                                                     ε
                                                    r
 k12r=wrεprµrC w         where wave vector is  kr  ω () () r  µ() r   while ω and c are the frequency and
 2
                                            1
                                                      p
                                                   C 2
                         speed of light, respectively. By assuming the spherical harmonics shapes, E and
                         H are replaced by vectors M  and N . The subscript, n, represents different vec-
                                                       n
                                                 n
                         tor spherical harmonics to describe the polar contribution to the scattered fields
                         (n = 1 dipolar, n = 2 quadripolar). The scattered field is calculated using series
                         below [1]:
                                                     ∞
                                                E  = ∑ (      − bM  ),                   (6.7)
                                                      EiaN
 Esca=∑n=1∞EnianNein−bnMoin,                     sca  n =1  n  n  ein  n  oin
                                                     ∞
                                                H sca  = ∑ (ib N oin  − a M ein  ),      (6.8)
                                                      E
                                                       n
                                                          n
                                                                 n
 Hsca=∑n=1∞EnibnNoin−anMein,                         n =1
                                      2 n  +1  
 En=inE 2n+1nn+1         where E  = iE        and E  is the incident filed. The subscript of o and e are odd
                                   n
                                       ( +1
 0                             n    0    nn  )   0
                         and even parameter of the azimuthal solution to the vector. The a  and b  represent
                                                                              n
                                                                                    n
                         Mie coefficients. These values are calculated as fallow [1]:
                                                                  ψ ( )
                                                       ψ () −
                                                m ψ ( ) ′ x   ψ () ′ mx
                                                     mx
                                                                 x
                                             a n  =  n   n     n    n                    (6.9)
                                                                  ψ ( )
                                                                x
                                                        ξ′ x
                                                     mx
 an=mψnmxψ′nx−ψnxψ′nmxmψnmxξ′nx−ξnxψ′nmx         m ψ ( ) () −  ξ () ′ mx
                                                               n
                                                   n
                                                         n
                                                                   n
                                                                  ψ ( )
                                                                 x
                                                   mx
                                                      ψ () − m
                                                ψ ( ) ′ x     ψ () ′ mx
                                             b n  =  n  n      n    n                   (6.10)
                                                                 ψ ( )
                                                       ξ′ x
                                                                x
                                                    mx
 bn=ψnmxψ′nx−mψnxψ′nmxψnmxξ′nx−ξnxψ′nmx          ψ ( ) () −  ξ () ′ mx
                                                   n
                                                        n
                                                                   n
                                                              n
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