156 Poster session, H43High-Resolution Spectroscopy of Hexamethylenetetramine (HMT)C 6 N 4 H 12Vincent Boudon 1 , Olivier Pirali 21 Laboratoire Interdisciplinaire Carnot de Bourgogne, UMR 6303 CNRS-Université deBourgogne, 9. Av. A. Savary, BP 47870, F-21078 Dijon Cedex, France,Vincent.Boudon@u-bourgogne.fr; 2 Ligne AILES, – Synchrotron SOLEIL, L’Orme desMerisiers, F-91192 Gif-sur-Yvette, and Institut des Sciences Moléculaires d’Orsay,UMR8214 CNRS-Université Paris-Sud, Bat. 210, 91405 Orsay cedex, France,Olivier.Pirali@synchrotron-soleil.frBoudon V.Pirali O.Hexamethylenetetramine, or HMT (C 6 N 4 H 12 ) is a N-substituted derivative ofadamantane C10H16 which is the smallest sample of the diamondoid molecules family.Thanks to their high stability, diamond-like molecules have long been suspected to bepresent in space [1] (note that diamond nanocrystals are extracted from the Murchinsonmeteorite [2]), and HMT is known to be an abundant residue of UV irradiatedinterstellar ice analogs [3] and might be present in Titan’s atmosphere. Using the BrukerIFS 125 coupled to a multipass cell (absorption path length of 150 m) of the AILESbeamline at SOLEIL, we recorded the IR spectrum of gas phase HMT in the 300–3000cm −1 spectral region with an unapodized resolution 0.001 cm −1 . HMT is a solid powderwith about 0.008 mbar vapour pressure at room temperature. It is a T d molecule (asadamantane) and has 25 vibrational modes from which only 9 are infrared active. Overthe 9 IR active fundamentals, we were able to rotationally resolve the spectra of 6 ofthem.The analysis of all the resolved bands has been performed thanks to the XTDS andSPVIEW softwares developed in Dijon for such molecules [4]. Each band can beconsidered as isolated and we obtained very good fits of line positions, with a root meansquare deviation better than 5 × 10 −4 cm −1 for J values up to 80 or more in every case.As for our recent study concerning adamantane [5], the resulting synthetic spectra mightpermit an active search of this very stable specie in different sources of the interstellarmedium.References[1] W. C. Saslaw and J. E. Gaustad, Nature, 221, 160 (1969)[2] R. S. Lewis et al., Nature, 326, 160 (1987)[3] M. P. Bernstein et al., ApJ, 454, 327 (1995)[4] Ch. Wenger, V. Boudon, M. Rotger, M. Sanzharov and J.-P. Champion, J. Mol.Spectrosc., 251 102–113 (2008).[5] O. Pirali, V. Boudon, J. Oomens, M. Vervloet, J. Chem. <strong>Ph</strong>ys., 136, 024310 (2012)
Poster session, H44 157A High Resolution FTIR Spectroscopic Study of Collisional - CooledCHF 3 : Re-Analysis of the Strongly Coupled States v 2 , v 5 , and v 3 +v 6A O. N. Ulenikov 1,2 , E. S. Bekhtereva 1,2 , I. B. Bolotova 1 , S. Albert 1 ,S. Bauerecker 1,3 , H. Hollenstein 1 , and M. Quack 11 <strong>Ph</strong>ysical Chemistry Laboratory, ETH-Zürich, CH-8093, Zürich, Switzerland; 2 TomskState University, <strong>Ph</strong>ysics Department, 634050, Tomsk, Russia; 3 Technische UniversitätBraunschweig, D - 38106, Braunschweig, GermanyUlenikov O.N.Bekhtereva E.S.Bolotova I.B.Albert S.Bauerecker S.Hollenstein H.Quack M.The infrared spectrum of CHF 3 is a prototypical spectrum of a classical symmetric topmolecule. Despite a long history 1-8 its rotationally resolved infrared spectrum is poorlyunderstood due to numerous strong interactions. For that reason we have started toreinvestigate the IR spectrum of CHF 3 . In this paper we present an analysis of the stronglycoupled triad of the states v 2 , v 5 , and v 3 +v 6 previously measured and analyzed using FTIRsupersonic jet spectroscopy. 5The high resolution FTIR spectrum of CHF 3 has been measured with the Bruker 125 HRspectrometer using a collisional cooling cell 9 in the regions 1000-3600 and 5800-6800 cm -1at two different temperatures, 120 and 295 K. As the result of analysis of the experimentaldata, transitions with maximum values of the quantum numbers J and K larger than 80 wereassigned to all the bands, v 2 , v 5 , and v 3 +v 6 , that is considerably more transitions than inprevious studies.In our present analysis we start by theoretical estimates of various parameters on the basis ofa known ab initio intramolecular potential function 6 . The equations, which connect the mostimportant interaction parameters with the parameters of the potential function, have beenderived on the basis of operator perturbation theory. This information was used in the fit ofexperimental upper energy levels obtained from the assignment of transitions in theexperimental spectrum. The fit results in a set of parameters which reproduce the initialexperimental data with an accuracy close to the experimental uncertainties.References[1] H. R. Dübal and M. Quack, Chem. <strong>Ph</strong>ys. Lett., 80, 439 - 444, 1981.[2] H. R. Dübal and M. Quack, J. Chem. <strong>Ph</strong>ys., 81, 3779 - 3791, 1984.[3] G. Graner, and G. Guelachvili, J. Mol. Spectrosc., 107, 215 - 228, 1984.[4] J. P. Champion, and G. Graner, Mol. <strong>Ph</strong>ys, 58, 475 - 484, 1986.[5] A. Amrein, M. Quack, and U. Schmitt, Mol. <strong>Ph</strong>ys., 60, 237 - 248, 1987.[6] J. Breidung, J. Cosleou, J. Demaison, K. Sarka, and W. Thiel, Mol. <strong>Ph</strong>ys., 102,1827 - 1841, 2004.[7] A. Amrein, M. Quack, and U. Schmitt, J. <strong>Ph</strong>ys. Chem., 92, 5455 - 5466, 1988.[8] S. Albert, K. Keppler Albert, H. Hollenstein, C. Manca Tanner, and M. Quack inHand<strong>book</strong> of High Resolution Spectroscopy, Vol. 1,M. Quack and F. Merkt eds.,Wiley Chichester 2011.[9] S. Albert, S. Bauerecker, M. Quack, and A. Steinlin, Mol. <strong>Ph</strong>ys., 105, 541 - 558, 2007.
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8 Program of sessionsInvited Lectur
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48 Poster session, D1Spectroscopic
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234 Author indexAAbdelghany A. —
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240 Author indexKhelkhal M. — D29
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242 Author indexMartin M.A. — D31
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246 Author indexSzajna W. — H29,
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248 Author indexZamotaeva V.A. —
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250 EmailsAbdelghany A.Abdelghany A
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252 EmailsGuarnieri A.ag@tf.uni-kie
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254 EmailsMichaut X.Xavier.Michaut@
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256 EmailsTyuterev Vl.G.vladimir.ti
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FT-IR spectrometerIFS 125HROutstand
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32nd International Symposium on Fre
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Some more information
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Addresses:Conference Site: National