HIGH-RESOLUTION INFRARED SPECTROSCOPY OF CUBANE, C8H8
Author(s) -
Vincent Boudon,
Cosimo Annese,
Caterina Fusco,
Lucia D’Accolti,
Sébastien Gruet,
Olivier Pirali
Publication year - 2014
Publication title -
proceedings of the 74th international symposium on molecular spectroscopy
Language(s) - English
Resource type - Conference proceedings
DOI - 10.15278/isms.2014.rd05
Subject(s) - cubane , infrared spectroscopy , spectroscopy , infrared , high resolution , resolution (logic) , materials science , chemistry , geology , remote sensing , computer science , crystallography , physics , optics , crystal structure , artificial intelligence , astronomy , organic chemistry
Carbon-cage molecules have generated a considerable interest from both experimental and theoretical point of views. We recently performed a high-resolution study of adamantane (C10H16), the smallest hydrocarbon cage belonging to the diamandoid family. There exist another family of hydrocarbon cages with additional interesting chemical properties: the so-called Platonic hydrocarbons that comprise dodecahedrane (C20H20) and cubane (C8H8). Both possess C–C bond angles that deviate from the tetrahedral angle (109.8◦) of the sp hybridized form of carbon. This generates a considerable strain in the molecule. Cubane itself has the highest density of all hydrocarbons (1.29 g/cm). This makes it able to store larges amounts of energy, although the molecule is fully stable. Up to now, only one high-resolution study of cubane has been performed on a few bands [2]. We report here a new wide-range high-resolution study of the infrared spectrum of cubane. The sample was synthesized in Bari upon decarboxylation of 1,4-cubanedicarboxylic acid thanks to the improved synthesis of literature [3]; its H and C NMR, FTIR, and mass spectrometry agreed with reported data [4]. Several spectra have been recorded at the AILES beamline of the SOLEIL French synchrotron facility. They cover the 800 to 3100 cm−1 region. Besides the three infrared-active fundamentals (ν10, ν11 and ν12), we could record many combination bands, all of them displaying a wellresolved octahedral rotational structure. We present here a preliminary analysis of some of the recorded bands, performed thanks the SPVIEW and XTDS software, based on the tensrorial formalism developed in the Dijon group [5].
Accelerating Research
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom
Address
John Eccles HouseRobert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom