Open AccessThe infrared spectrum of ortho‐enstatite from reflectance experiments and first‐principle simulations
Author(s) -
Demichelis Raffaella,
Suto Hiroshi,
Noël Yves,
Sogawa Hisato,
Naoi Takahiro,
Koike Chiyoe,
Chihara Hiroki,
Shimobayashi Norimasa,
Ferrabone Matteo,
Dovesi Roberto
Publication year - 2012
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1111/j.1365-2966.2011.20018.x
Subject(s) - physics , enstatite , infrared , reflectivity , spectrum (functional analysis) , astrophysics , optics , astronomy , computational physics , meteorite , chondrite , quantum mechanics
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, MgSiO 3 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.