Diffuse X-ray scattering from polished silicon: application of the distorted wave Born approximation

Measured diffuse X-ray scattering data for a 'smooth' as well as for a 'rough' silicon sample were fit to theoretical expressions within the distorted wave Born approximation (DWBA). Data for the power spectral density (PSD) for both samples were also obtained by means of atomic force microscopy and optical interferometry. The Fourier transforms of trial correlation functions were fit to the PSD data and then applied to the DWBA formalism. The net correlation functions needed to fit the PSD data for each sample comprised the sum of two terms with different cutoff lengths and different self-affine fractal exponents. At zero distance these correlation functions added up to yield net values of sigma(2) = (2)(2) and (71)(2) angstrom(2) for the smooth and rough samples, respectively. X-ray scattering data were obtained at beamline 1-BM o of the Advanced Photon Source. Data A and fits at values of q(z) = 0.05 and 0.10 angstrom(-1) for the smooth sample are reported. Good fits for the smooth sample were obtained at both q(z) values simultaneously, that is, identical fitting parameters were applied at both values of q(z). The smooth sample also exhibited weak Yoneda wings and a clear distinction between the strong specular scattering and the weak diffuse scattering. Data for the rough sample were qualitatively different and exhibited very weak scattering at the specular condition in contrast to extremely large Yoneda wings. Fits for the rough sample are reported for q(z) = 0.04, 0.05, and 0.06 angstrom(-1). Although the large Yoneda wings could be fit quite well in both position and amplitude, scattering near the specular condition could not be equally well fit by applying the same fitting parameters at all values of q(z). Albeit imperfect, best-fitting results at the specular condition were obtained by invoking only diffuse scattering, that is, without including a separate theoretical expression for specular scattering.