Journal Article

The infrared spectrum of ortho-enstatite from reflectance experiments and first-principle simulations

Raffaella Demichelis, Hiroshi Suto, Yves Noël, Hisato Sogawa, Takahiro Naoi, Chiyoe Koike, Hiroki Chihara, Norimasa Shimobayashi, Matteo Ferrabone and Roberto Dovesi

in Monthly Notices of the Royal Astronomical Society

Published on behalf of The Royal Astronomical Society

Volume 420, issue 1, pages 147-154
Published in print February 2012 | ISSN: 0035-8711
Published online January 2012 | e-ISSN: 1365-2966 | DOI:
The infrared spectrum of ortho-enstatite from reflectance experiments and first-principle simulations

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Infrared (IR) spectra provide a rich amount of information concerning chemical composition, lattice structure, size and shape of circumstellar dust. Accurate reference data are then required for the analysis of the various detected components. This study provides the IR characterization of one of the most frequently observed compounds, MgSiO3 ortho-enstatite, and shows that IR experiments and ab initio techniques can be used synergically to obtain high-quality data concerning crystalline materials. The IR reflectance spectrum of synthetic ortho-enstatite was collected and compared to ab initio results (Gaussian-type basis set, PBE0 hybrid density functional theory (DFT) functional). An excellent agreement is observed both for vibrational frequencies (ν) and intensities, the latter estimated through the oscillator strength. The mean absolute difference between experimental and calculated ν is of the order of 7–8 cm−1 (43 out of 65 peaks differ by less than 10 cm−1, only four peaks differ by 15–19 cm−1). The static dielectric tensor and its components (electronic and ionic contributions) were measured and compared to calculated data: differences are in the 2–5 per cent range.

Keywords: techniques: miscellaneous; astronomical data bases: miscellaneous; circumstellar matter

Journal Article.  4181 words.  Illustrated.

Subjects: Astronomy and Astrophysics

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