TJ. Rotational structure/frequencies
Tuesday, 2018-06-19, 01:45 PM
Noyes Laboratory 217
SESSION CHAIR: Ranil Gurusinghe (Tennessee Tech University, Cookeville, TN)
|
|
|
TJ01 |
Contributed Talk |
15 min |
01:45 PM - 02:00 PM |
P3145: HIGH SENSITIVITY CRDS OF CO2 IN THE 1.74 μM TRANSPARENCY WINDOW. A VALIDATION TEST FOR THE SPECTROSCOPIC DATABASES |
PETER ČERMÁK, Department of Experimental Physics, Comenius University, Bratislava, Slovakia; EKATERINA KARLOVETS, Laboratory of Quantum Molecular Mechanics and Radiation Processes, Tomsk State University, Tomsk, Russia; DIDIER MONDELAIN, SAMIR KASSI, UMR5588 LIPhy, Université Grenoble Alpes/CNRS, Saint Martin d'Hères, France; VALERY PEREVALOV, Molecular Spectroscopy, V.E. Zuev Institute of Atmospheric Optics, Tomsk, Russia; ALAIN CAMPARGUE, UMR5588 LIPhy, Université Grenoble Alpes/CNRS, Saint Martin d'Hères, France; |
IDEALS Archive (Abstract PDF / Presentation File) |
DOI: https://dx.doi.org/10.15278/isms.2018.TJ01 |
CLICK TO SHOW HTML
The very weak absorption spectrum of natural CO2 near 1.74 μm (5702 - 5879 cm−1) is studied at high sensitivity. The investigated region corresponds to a transparency window of very weak opacity which is of particular interest for Venus. Very weak lines with intensity value as low as 10−30 cm/molecule at 296 K are detected by Cavity Ring Down Spectroscopy. On the basis of the predictions of effective Hamiltonian models, 1135 lines of six carbon dioxide isotopologues - 12C16O2, 13C16O2, 16O12C18O, 16O12C17O, 16O13C18O and 16O13C17O - were rovibrationnally assigned to 26 bands. The accurate spectroscopic parameters of 16 bands are determined from standard band-by-band analysis (typical rms deviations of the line positions are 8 ×10−4 cm−1).
These newly observed bands include perturbed bands, weak hot bands and bands of minor isotopologues (in particular 16O12C18O in natural abundance) and provide critical validation tests for the most recent spectroscopic databases. The comparison to the Carbon Dioxide Spectroscopic Databank (CDSD), HITRAN2016 database and recent ab initio line lists will be presented. Deficiencies are evidenced for some weak perpendicular bands of the HITRAN2016 list and identified as due to inaccurate CDSD intensities which were preferred to ab initio intensities. New results based on 18O enriched CO2 spectra will also be detailed.
|
|
TJ02 |
Contributed Talk |
15 min |
02:02 PM - 02:17 PM |
P2913: LINE POSITIONS AND INTENSITIES FOR THE ν3 BAND OF 5 ISOTOPOLOGUES OF GERMANE FOR PLANETARY APPLICATIONS |
VINCENT BOUDON, TIGRAN GRIGORYAN, FLORIAN PHILIPOT, CYRIL RICHARD, Laboratoire ICB, CNRS/Université de Bourgogne, DIJON, France; F. KWABIA TCHANA, LISA, CNRS, Universités Paris Est Créteil et Paris Diderot, Créteil, France; LAURENT MANCERON, Synchrotron SOLEIL, CNRS-MONARIS UMR 8233 and Beamline AILES, Saint Aubin, France; ATHENA RIZOPOULOS, JEAN VANDER AUWERA, Service de Chimie Quantique et Photophysique, Universit\'{e} Libre de Bruxelles, Brussels, Belgium; THÉRÈSE ENCRENAZ, LESIA, Observatoire de Paris / CNRS / UPMC, Meudon, France; |
IDEALS Archive (Abstract PDF / Presentation File) |
DOI: https://dx.doi.org/10.15278/isms.2018.TJ02 |
CLICK TO SHOW HTML
Germane (GeH 4) is present in the atmospheres of the giant planets Jupiter and Saturn. The ongoing NASA mission Juno has renewed interest in its spectroscopy. The accurate modeling of which is essential for the retrieval of other tropospheric species. We present here the first complete analysis and modeling of line positions and intensities in the strongly absorbing ν 1/ν 3 stretching dyad region near 2100 cm −1, for all five germane isotopologues in natural abundance V. Boudon, T. Grigoryan, F. Philipot, C. Richard, F. Kwabia Tchana, L. Manceron, A. Rizopoulos, J. Vander Auwera and T. Encrenaz, J. Quant. Spectrosc. Radiat. Transfer 205, 174-183 (2018) New infrared spectra were recorded, absolute intensities were extracted through a careful procedure and modeled thanks to the formalism and programs developed in Dijon. A database of calculated germane lines, GeCaSDa, is available online through the Virtual Atomic and Molecular Data Centre (VAMDC) portal ( http://portal.vamdc.org) and at http://vamdc.icb.cnrs.fr/PHP/gecasda.php. GeH 4 will integrate the HITRAN database as molecule number 50.
Footnotes:
V. Boudon, T. Grigoryan, F. Philipot, C. Richard, F. Kwabia Tchana, L. Manceron, A. Rizopoulos, J. Vander Auwera and T. Encrenaz, J. Quant. Spectrosc. Radiat. Transfer 205, 174-183 (2018).
|
|
TJ03 |
Contributed Talk |
15 min |
02:19 PM - 02:34 PM |
P2975: INVESTIGATION OF THIOKETENE ISOMERS: MICROWAVE SPECTROSCOPY AND FORMATION CHEMISTRY OF HCCSH |
KELVIN LEE, Radio and Geoastronomy Division, Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, USA; MARIE-ALINE MARTIN-DRUMEL, CNRS, Institut des Sciences Moleculaires d'Orsay, Orsay, France; VALERIO LATTANZI, The Center for Astrochemical Studies, Max-Planck-Institut für extraterrestrische Physik, Garching, Germany; BRETT A. McGUIRE, NAASC, National Radio Astronomy Observatory, Charlottesville, VA, USA; MICHAEL C McCARTHY, Atomic and Molecular Physics, Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, USA; |
IDEALS Archive (Abstract PDF / Presentation File) |
DOI: https://dx.doi.org/10.15278/isms.2018.TJ03 |
CLICK TO SHOW HTML
Because of their curious electronic properties, carbon-sulfide chains possess peculiar molecular structures and chemical reactivity. In this talk, we present the spectroscopic characterization of ethynethiol (HCCSH) - an isomer of thioketene (H2CCS) and thiirene (c-H2C2S) - and its isotopologues using Fourier-transform microwave cavity and millimeter-wave absorption spectroscopies. HCCSH is produced in an electrical discharge of HCCH and H2S. In our cavity spectrometer (10 - 40 GHz), the J=1−0, 2−1, 3−2 a-type transitions have been observed. HCC34SH was detected in natural abundance while the deuterated isotologues required HCCD and D2S for DCCSH and HCCSD respectively. Based on ab initio predictions, the fundamental b-type transitions were also measured using double resonance (150 - 300 GHz), allowing the A constant to be determined approximately and guiding subsequent surveys into the millimeter-wave (280 - 655 GHz). Based on the information derived from the isotopologues, we will also discuss the molecular structure and inferred formation chemistry, in addition to its relative abundance to thioketene.
|
|
TJ04 |
Contributed Talk |
15 min |
02:36 PM - 02:51 PM |
P3196: THE MILLIMETER/SUBMILLIMETER-WAVE SPECTRUM OF F2SO (~X1A′) |
JOHN P KEOGH, Department of Chemistry and Biochemistry, University of Arizona, Tucson, AZ, USA; DeWAYNE T HALFEN, Department of Chemistry and Biochemistry, Department of Astronomy, The University of Arizona, Tucson, AZ, USA; LUCY M. ZIURYS, Department of Chemistry and Biochemistry; Department of Astronomy, Arizona Radio Observatory, University of Arizona, Tuscon, AZ, USA; |
IDEALS Archive (Abstract PDF / Presentation File) |
DOI: https://dx.doi.org/10.15278/isms.2018.TJ04 |
CLICK TO SHOW HTML
The millimeter/submillimeter spectrum of F 2SO (~X 1A′) has been measured using direct absorption techniques in the frequency range 271 – 508 GHz. Thionyl fluoride was created in the process of searching for a number of metal-containing fluoride molecules. This species was serendipitously produced from SF 6 as the fluorine source with residual water in the presence of a DC discharge. Multiple rotational transitions in the range J = 16 to J = 30 were recorded, each consisting of a c-type asymmetric top pattern, due to the large dipole moment along the ^c molecular axis μ c = 1.62 D. The data were analyzed using an asymmetric top Hamiltonian and rotational and centrifugal distortion constants were established. This work considerably expands the spectroscopic characterization of F 2SO. Previous microwave data consisted of measurements below 77 GHz.
|
|
TJ05 |
Contributed Talk |
15 min |
02:53 PM - 03:08 PM |
P3057: FLUORINATION EFFECT ON HYDROGEN BOND TOPOLOGIES IN WATER ADDUCTS OF FLUOROPYRIDINES |
JUAN WANG, XIAOLONG LI, GANG FENG, QIAN GOU, School of Chemistry and Chemical Engineering, Chongqing University, Chongqing, China; |
IDEALS Archive (Abstract PDF / Presentation File) |
DOI: https://dx.doi.org/10.15278/isms.2018.TJ05 |
CLICK TO SHOW HTML
The rotational spectra of a series of 1:1 adducts of water-fluoropyridines have been investigated by using pulsed jet Fourier transform microwave spectroscopy. Depending on the fluorination sites, the hydrogen bond topologies are quite different from each other. The water links with the N n-obital of 2,3-difluoropyridine and 2,6-difluoropyridine, respectively. through an O-H...N bond. In addition, one weak C-H...O bond might be contributable to the stabilization of the complex 2,3-difluoropyridine-water, while an O-H...F bond plausibly formed in the complex 2,6-difluoropyridine-water in which water acts as a double proton donor. Additional fluorination of the third site of 2,6-difluoropyridine creates a new active site ready to interact with water: the isomer stabilized by one C-H...O and one O-H...F hydrogen bond is proved by the experimental evidences to be the global minimum. This hydrogen topology is quite different from the all former rotational studied complexes involving pyridine and fluoropyridines.
|
|
|
|
|
03:10 PM |
INTERMISSION |
|
|
TJ06 |
Contributed Talk |
15 min |
03:44 PM - 03:59 PM |
P3079: TIPPING THE BALANCE BETWEEN ELECTROSTATICS AND STERIC EFFECTS: THE MICROWAVE SPECTRA AND MOLECULAR STRUCTURES OF 2-CHLORO-1,1-DIFLUOROETHYLENE–ACETYLENE AND CIS-1,2-DIFLUOROETHYLENE–ACETYLENE |
HELEN O. LEUNG, MARK D. MARSHALL, Chemistry Department, Amherst College, Amherst, MA, USA; |
IDEALS Archive (Abstract PDF / Presentation File) |
DOI: https://dx.doi.org/10.15278/isms.2018.TJ06 |
CLICK TO SHOW HTML
We have found that the observed average structures of haloethylene-protic acid heterodimers result from an interplay between favorable electrostatic interactions and steric effects. For vinyl fluoride and 1,1-difluoroethylene complexes, steric effects predominate and the acid binds across the double bond ("top"), while for trifluoroethylene, favorable electrostatics forces the complexes to adopt a sterically strained structure with the acid at one end of the olefin ("side"). A relaxation of steric requirements for binding with a chlorine atom leads to different geometries being observed for each of the vinyl chloride complexes with hydrogen fluoride, hydrogen chloride, and acetylene. The side binding motif to chlorine persists in (Z)-1-chloro-2-fluoroethylene–acetylene despite the presence of the more electronegative fluorine atom. For 2-chloro-1,1-difluoroethylene ethylene–acetylene, the acetylene is presented with the option of top binding to fluorine versus side binding to chlorine, whereas with cis-1,2-difluoroethylene, the only option is side binding to fluorine. The structures of these two complexes are compared to reveal the balance between electrostatics and sterics.
|
|
TJ07 |
Contributed Talk |
15 min |
04:01 PM - 04:16 PM |
P3030: MICROWAVE SPECTRUM AND MOLECULAR STRUCTURE OF 2,3,3,3-TETRAFLUOROPROPENE–HYDROGEN CHLORIDE |
HELEN O. LEUNG, MARK D. MARSHALL, MILES A. WRONKOVICH, Chemistry Department, Amherst College, Amherst, MA, USA; |
IDEALS Archive (Abstract PDF / Presentation File) |
DOI: https://dx.doi.org/10.15278/isms.2018.TJ07 |
CLICK TO SHOW HTML
Our systematic study of the structures of heterodimers of haloethylenes with protic acids has provided a wealth of information, along with a few surprises, regarding the sometimes cooperative and sometimes competing effects of electrostatic, steric, and dispersion forces that contribute to the binding of these species. We seek to apply this knowledge to larger systems with a wider variety of possible interactions and binding sites via the addition of a trifluoromethyl moiety to the olefin to form halopropenes. The microwave spectrum of the complex formed between 2,3,3,3-tetrafluoropropene, which can be considered a trifluoromethyl analogue of vinyl fluoride, and hydrogen chloride is obtained and analyzed to determine the molecular structure of this species.
|
|
TJ08 |
Contributed Talk |
15 min |
04:18 PM - 04:33 PM |
P3182: THE CONFORMATIONS OF PROTEINOGENIC AMINO ACID GLUTAMINE: MORE ACCURACY IS URGENTLY NEEDED IN THEORETICAL CALCULATIONS |
IKER LEÓN, ELENA R. ALONSO, CARLOS CABEZAS, SANTIAGO MATA, JOSÉ L. ALONSO, Grupo de Espectroscopia Molecular, Lab. de Espectroscopia y Bioespectroscopia, Unidad Asociada CSIC, Universidad de Valladolid, Valladolid, Spain; |
IDEALS Archive (Abstract PDF / Presentation File) |
DOI: https://dx.doi.org/10.15278/isms.2018.TJ08 |
CLICK TO SHOW HTML
Glutamine is α-amino acid that is used in the biosynthesis of proteins. The large flexibility of the molecule has several potential conformational candidates. Among them, the three most stable isomers have been characterized both using a laser ablation chirped pulse Fourier-transform microwave spectrometer (LA-CP-FTMW) and a laser ablation molecular-beam Fourier-transform microwave spectrometer (LA-MB-FTMW). S. Mata, I. Peña, C. Cabezas, J. C. López and J. L. Alonso, J. Mol. Spectrosc., 2012, 280, 91–96.^, J. L. Alonso and J. C. López, in Gas−Phase IR Spectroscopy and Structure of Biological Molecules, eds. A. M. Rijs and J. Oomens, Topics in., 2015, vol. 364, pp. 335–402.wo of the conformers can be determined using the spectroscopic constants provided by the theoretical methods. On the other hand, the third conformer is not reproduced by conventional theoretical methods and one should use some tricks to characterize the conformer’s structure. In addition, even the slightest different prediction in the site position of the nitrogen atoms makes the conformer’s spectroscopic characterization very challenging because the nuclear quadrupole coupling interactions depend critically on the electronic environment, position and orientation of the ^14
J. L. Alonso and J. C. López, in Gas-Phase IR Spectroscopy and Structure of Biological Molecules, eds. A. M. Rijs and J. Oomens, Topics in., 2015, vol. 364, pp. 335–402.T
|
|
TJ09 |
Contributed Talk |
15 min |
04:35 PM - 04:50 PM |
P3327: SULFUR HYDROGEN BONDING: A COMPARISON OF THE DIMERS AND MONOHYDRATES OF THENYL AND FURFURYL ALCOHOLS AND MERCAPTANS |
MARCOS JUANES, RIZALINA TAMA SARAGI, ALBERTO LESARRI, Departamento de Química Física y Química Inorgánica, Universidad de Valladolid, Valladolid, Spain; RUTH PINACHO, JOSÉ EMILIANO RUBIO, LOURDES ENRIQUEZ, MARTIN JARAIZ, Departamento de Electrónica, ETSIT, University of Valladolid, Valladolid, SPAIN; |
IDEALS Archive (Abstract PDF / Presentation File) |
DOI: https://dx.doi.org/10.15278/isms.2018.TJ09 |
CLICK TO SHOW HTML
r0pt
Figure
The dimers of thenyl alcohol (TA 2) and furfuryl alcohol (FA 2), and the monohydrates of both alcohols (TA···H 2O, FA···H 2O) and their corresponding mercaptans (TM···H 2O, FM···H 2O) were generated in a supersonic jet expansion and probed using both chirped-pulse and cavity Fourier transform microwave spectroscopy. The experimental results, supported by ab initio molecular orbital calculations, allow comparing the conformational preferences and the role of the sulfur and oxygen atoms in the O-H···O/O-H···S/S-H···O hydrogen bonds (HBs) stabilizing the dimers. In the furfuryl monohydrates (FA···H 2O, FM···H 2O) water behaves as a proton donor to the ring oxygen, in competence with a second HB to the alcohol or thiol side chain M. Juanes, A. Lesarri, R. Pinacho, E. Charro, J. E. Rubio, L. Enriquez, M. Jaraiz, Chem. Eur. J., 2018, 24, 1–9, in press Different behavior was observed when the ring oxygen is replaced by sulfur atom in the thenyl monohydrates (TA··· H 2O and TM···H 2O) as the water molecule is binding to the side chain and the π electronic cloud of the ring. The water motion in both thenyl dimers is detected by tunneling splittings of the rotational transitions, denoting a weaker binding compared to the furfuryl compounds. The alcohol dimers (TA) 2 and (FA) 2 again reveal the different HB strengths in the furfuryl and thenyl groups. The alcohol dimer forms a network of two consecutive O-H···O hydrogen bonds involving the oxygen ring, while in the thenyl dimer the alcohol group prefers binding to the π cloud than to the sulfur atom in the ring. Spectroscopic, structural and computational data will be reported.
Footnotes:
M. Juanes, A. Lesarri, R. Pinacho, E. Charro, J. E. Rubio, L. Enriquez, M. Jaraiz, Chem. Eur. J., 2018, 24, 1–9, in press.
|
|
TJ10 |
Contributed Talk |
15 min |
04:52 PM - 05:07 PM |
P3423: STRUCTURE DETERMINATION OF 5 MEMBERED SILANE RINGS USING MICROWAVE SPECTROSCOPY |
FRANK E MARSHALL, AMANDA JO DUERDEN, NICOLE MOON, DAVID JOSEPH GILLCRIST, Department of Chemistry, Missouri University of Science and Technology, Rolla, MO, USA; IVAN SEDLACEK, Chemistry, Missouri University of Science and Technology, Rolla, MO, USA; GRIER JONES, THEODORE CARRIGAN-BRODA, GAMIL A GUIRGIS, Department of Chemistry and Biochemistry, College of Charleston, Charleston, SC, USA; G. S. GRUBBS II, Department of Chemistry, Missouri University of Science and Technology, Rolla, MO, USA; |
IDEALS Archive (Abstract PDF / Presentation File) |
DOI: https://dx.doi.org/10.15278/isms.2018.TJ10 |
CLICK TO SHOW HTML
Rotational spectra of 1,1-difluorosilacyclopent-3-ene, silacyclopent-3-ene,
1-(chloromethyl)-1-fluoro-silacyclopentane, 1,1-difluorosilacyclopentane, and
1,1-difluorosilacylopent-2-ene were observed in the 6 to 18 GHz range of the electromagnetic spectrum. The molecular structure for the parent and various isotopically substituted species were obtained from their respective spectra. The differences in structure between these similar molecules will be presented, showing how different functional groups and bond locations affect the overall structure and behavior of each system (ring puckering effects, etc.). Comparisons to similar known cyclopentane and silacyclopentane species will be presented.
|
|