Statistical approach of the effects of roughness on the polarization of light scattered by dust grains

In order to study the effect of shape on the optical properties of dust gra ins, we statistically analyze the linear polarized scattered light. We star t by examining a homogeneous spherical grain using the discrete dipole appr oximation (DDA) Draine (Astrophys J 1988;333:848). Using a uniform law we r emove elements of matter on the surface of the grain to describe a random r oughness. Then, for various scattering angles, the linear polarization P-1 is calculated. We successively repeat the simulation in order to obtain a s ample of random variables constituting the values P-1 of the linear polariz ation. The analysis of the results is then achieved through a Gaussian kern el method which provides the probability density function of P-1 for each s cattering angle. We present the results for a typical interstellar grain of water-ice with radius a comparable to the incident wavelength lambda so th at the parameter size x drop 2 pia/lambda similar or equal to 1. We apply t his method for two wavelengths in the near IR, when water-ice is transparen t at 1.9 mum, and, when water-ice is absorbing at 3.1 mum. We find that the shape of the density function of the linear polarization is asymmetric to the mean value of the density function and non-unimodal for several scatter ing angles. This allows us to separate the effects of roughness from those of volume. When water-ice is absorbing, we also observe a significant shift of the polarization peak toward greater scattering angles. (C) 2001 Publis hed by Elsevier Science Ltd.