%0 Journal Article
%T Effects of structural and chemical disorders on the visible/UV spectra of carbonaceous interstellar grains
%A R. J. Papoular
%A S. Yuan
%A R. Roldan
%A M. I. Katsnelson
%A R. Papoular
%J Physics
%D 2013
%I arXiv
%R 10.1093/mnras/stt656
%X The recent spectacular progress in the experimental and theoretical understanding of graphene, the basic constituent of graphite, is applied here to compute, from first principles, the UV extinction of nano-particles made of stacks of graphene layers. The theory also covers cases where graphene is affected by structural, chemical or orientation disorder, each disorder type being quantitatively defined by a single parameter. The extinction bumps carried by such model materials are found to have positions and widths falling in the same range as the known astronomical 2175 \AA features: as the disorder parameter increases, the bump width increases from 0.85 to 2.5 $\mu$m$^{-1}$, while its peak position shifts from 4.65 to 4.75 $\mu$m$^{-1}$. Moderate degrees of disorder are enough to cover the range of widths of the vast majority of observed bumps (0.75 to 1.3 $\mu$m$^{-1}$). Higher degrees account for outliers, also observed in the sky. The introduction of structural or chemical disorder amounts to changing the initial $sp^{2}$ bondings into $sp^{3}$ or $sp^{1}$, so the optical properties of the model material become similar to those of the more or less amorphous carbon-rich materials studied in the laboratory: a-C, a-C:H, HAC, ACH, coals etc. The present treatment thus bridges gaps between physically different model materials.
%U http://arxiv.org/abs/1304.4725v1