Scattering Theory

The eigenstate of the Hamiltonian gives solve this equation with the conduction electron Green's function In the continuous -representation we have which is the Lippmann-Schwinger equation of scattering theory. To obtain the scattered wave affected by incoming Bloch wave of momentum , we have the Green's function of the following form and further define the eigenstate becomes therefore by iterating these two equations we have where the matrix element Consider the plane waves of a box of volume with periodic boundary conditions, the Green's function is using the sphere coordination we have Integrating out the angle contribution of this integral, consider the eigenvalue , therefore the Green's function is where , and this expression has two pole at . Perform the contour integration in the upper plane, we have With far field asymptotic approximation of and consider the Taylor's expansion , we have where and the exponential phase is simplified by Hence the scattered wave function becomes where the scattering amplitude The differential scattering cross-section is given by The integration form of this expression gives the total scattering cross-section : Using the relation the transition rate becomes Remind the perturbation form of the T-matrix with the operator identity we have taking the diagonal elements, Consider the matrix elements and the representation of the delta function the total scattering cross-section becomes which can be expressed in terms of the imaginary part of the forward scattering amplitude . This is known as optical theorem of scattering theorem. For a spherically symmetric scattering, the potential depends only on thee angle between and . Expand the term with Legendre polynomials , where is a real function, and is the phase shift of the th partial wave. The factor comes from the independence of the scattering on the -component of the angular momentum . Using the orthogonality relation of the Legendre polynomials, we have The total scattering cross-section in terms of phase shift is Expand the plane wave in terms of partial waves, where is a spherical Bessel function of order . Substituting this term back to the scattered wave function and using the asymptotic form, we have