Effects of structural and chemical disorders on the visible/UV spectra of carbonaceous interstellar grains
R.J. Papoular, S. Yuan, R. Roldan, M.I. Katsnelson, R. Papoular

TL;DR
This study uses first-principles calculations to show how structural and chemical disorders in graphene-based nano-particles influence their UV spectra, explaining variations in the astronomical 2175 Å feature.
Contribution
It introduces a quantitative model linking disorder parameters in graphene stacks to UV spectral features, bridging different carbonaceous dust models.
Findings
Disorder increases the width of the UV bump from 0.85 to 2.5 μm$^{-1}$.
Peak position shifts from 4.65 to 4.75 μm$^{-1}$ with increasing disorder.
Moderate disorder explains most observed bump variations.
Abstract
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 m, while its peak position shifts from 4.65 to 4.75 m. Moderate degrees of disorder are enough to cover the range of widths of the vast majority of observed bumps (0.75 to 1.3 m). Higher…
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