WI. Mini-symposium: Far-Infrared Spectroscopy
Wednesday, 2018-06-20, 01:45 PM
Chemistry Annex 1024
SESSION CHAIR: Brian Drouin (California Institute of Technology, Pasadena, CA)
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WI01 |
Invited Mini-Symposium Talk |
30 min |
01:45 PM - 02:15 PM |
P3374: PHOTONICS-BASED TERAHERTZ SOURCES FOR MOLECULAR SPECTROSCOPY |
JEAN-FRANÇOIS LAMPIN, UMR CNRS 8520, Institut d'Electronique de Microélectronique et de Nanotechnologie, Villeneuve d'Ascq, France; |
IDEALS Archive (Abstract PDF / Presentation File) |
DOI: https://dx.doi.org/10.15278/isms.2018.WI01 |
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r0pt
Figure
Since twenty years photonics-based terahertz (THz) sources have made great progress. They are now usable for low- and high-resolution molecular spectroscopy in the 0.1-4 THz range (3-130 cm−1).
We will present the principles of near-infrared laser-based THz set-ups: time-domain spectroscopy (see figure showing ambient pressure H2O lines) and frequency-domain photomixing. Then we will review the different types of high bandwidth semiconductors photodetectors used to convert laser beams into THz beams. Two families are mainly used: photoconductors and photodiodes. Advantages and drawbacks of each will be presented. The subject of THz antennas will be also discussed and a state of the art will be given including the devices developed at IEMN. Some example of molecular spectroscopy measurements using these devices at various frequencies and resolutions will be given. Finally new ways for photonics-based THz sources will be exposed.
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WI02 |
Contributed Talk |
15 min |
02:19 PM - 02:34 PM |
P3178: THZ HETERODYNE SPECTROSCOPY ON THE AILES BEAMLINE OF SOLEIL FACILITY USING THE SYNCHROTRON RADIATION EMITTED BY THE MULTIBUNCH OPERATION MODE |
OLIVIER PIRALI, AILES beamline, Synchrotron SOLEIL, Saint Aubin, France; GAËL MOURET, FRANCIS HINDLE, ARNAUD CUISSET, Laboratoire de Physico-Chimie de l'Atmosphère, Université du Littoral Côte d'Opale, Dunkerque, France; JEAN-FRANÇOIS LAMPIN, SOPHIE ELIET, JOAN TURUT, Institut d’Electronique de Microélectronique et de Nanotechnologie, Université de Lille 1, Villeneuve d'Ascq, France; P. ROY, AILES beam line, Synchrotron Soleil, Gif-sur-Yvette, France; |
IDEALS Archive (Abstract PDF / Presentation File) |
DOI: https://dx.doi.org/10.15278/isms.2018.WI02 |
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The goal of our project is to develop a new high-resolution spectrometer on the AILES beamline of synchrotron SOLEIL. The spectrometer will record absorption spectra in the 1-5 THz range with sub-MHz resolution using a heterodyne detection scheme. We recently performed a test experiment using the far-IR continuum produced by synchrotron radiation in the multibunch mode, a multiplication chain as local oscillator, and a hot electron bolometer (HEB) as heterodyne mixer. The set-up allowed the detection of one D2O absorption line centered at about 782 GHz (RQ(4)0,4) with a resolution better than 1 MHz. We will present the details of the experiment and some instrumental developments in progress.
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WI03 |
Contributed Talk |
15 min |
02:36 PM - 02:51 PM |
P2945: GAS-PHASE INFRARED SPECTROSCOPY OF METAL-LIGAND REDOX PAIRS |
MUSLEH UDDIN MUNSHI, FELIX Laboratory, Radboud University, Nijmegen, The Netherlands; GIEL BERDEN, JONATHAN K MARTENS, Institute for Molecules and Materials (IMM), Radboud University Nijmegen, Nijmegen, Netherlands; JOS OOMENS, FELIX Laboratory, Radboud University, Nijmegen, The Netherlands; |
IDEALS Archive (Abstract PDF / Presentation File) |
DOI: https://dx.doi.org/10.15278/isms.2018.WI03 |
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Transition metal organometallic complexes are known for their catalytic activation of small molecules. For example, CO 2 activation by Ni 1+(cyclam) complexes has recently been reported in the gas-phase F. S. Menges, S. M. Craig, N. Tötsch, A. Bloomfield, S. Ghosh, H. J. Krüger and M. A. Johnson, Angewandte Chemie International Edition, 2016, 55, 1282-1285. where the oxidation state of the metal appeared to be the key for the electrochemical reduction of CO 2. In this contribution, we show that metal(II) complexes, including Ni-cyclam, generated via electrospray ionization can be charge reduced inside a quadrupole ion trap mass spectrometer J. Martens, G. Berden, C. R. Gebhardt and J. Oomens, Review of Scientific Instruments, 2016, 87, 103108.QIT MS) via an electron transfer reduction (ETR) reaction using fluoranthene radical anions as reagents M. U. Munshi, S. M. Craig, G. Berden, J. Martens, A. F. DeBlase, D. J. Foreman, S. A. McLuckey, J. Oomens and M. A. Johnson, The Journal of Physical Chemistry Letters, 2017, 8, 5047-5052 Moreover, their IR spectra can be recorded by action spectroscopy using the FELIX free electron laser, which enables their structural characterization. The complex in either of two charge states is isolated by its m/z, stored and irradiated with tunable IR light in the range of 500-1800 cm −1. IR induced dissociation occurs upon resonant vibrational excitation of the trapped ions, so that an IR spectrum of the (charge reduced) complexes can be obtained by plotting the dissociation yield as a function of IR laser frequency. Experimental spectra are compared with theoretical spectra computed at the density functional theory (DFT) level to obtain detailed structural information of the complexes undergoing charge reduction, eventually providing new insights in their catalytic capabilities.
F. S. Menges, S. M. Craig, N. Tötsch, A. Bloomfield, S. Ghosh, H. J. Krüger and M. A. Johnson, Angewandte Chemie International Edition, 2016, 55, 1282-1285.,
J. Martens, G. Berden, C. R. Gebhardt and J. Oomens, Review of Scientific Instruments, 2016, 87, 103108.(
M. U. Munshi, S. M. Craig, G. Berden, J. Martens, A. F. DeBlase, D. J. Foreman, S. A. McLuckey, J. Oomens and M. A. Johnson, The Journal of Physical Chemistry Letters, 2017, 8, 5047-5052.
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WI04 |
Contributed Talk |
15 min |
02:53 PM - 03:08 PM |
P3392: HIGH-RESOLUTION TERAHERTZ GAIN SPECTRA OF MID-INFRARED PUMPED NH3 |
MARTIN MICICA, Institut d'électronique de microélectronique et de nanotechnologie, Université de Lille 1, Villeneuve d'Ascq, France; SOPHIE ELIET, Institut d’Electronique de Microélectronique et de Nanotechnologie, Université de Lille 1, Villeneuve d'Ascq, France; A. PIENKINA, Laboratoire PhLAM, UMR 8523 CNRS - Université Lille 1, Villeneuve d'Ascq, France; R. A. MOTIYENKO, UMR 8523 - PhLAM - Physique des Lasers Atomes et Molécules, University of Lille, CNRS, F-59000 Lille, France; L. MARGULÈS, Laboratoire PhLAM, UMR 8523 CNRS - Université Lille 1, Villeneuve d'Ascq, France; MATHIAS VANWOLLEGHEM, UMR CNRS 8520, Institut d'Electronique de Microélectronique et de Nanotechnologie, Villeneuve d'Ascq, France; KAMIL POSTAVA, IT4Innovations, VSB - Technical University of Ostrava, Ostrava - Poruba, Czech Republic; JEAN-FRANÇOIS LAMPIN, UMR CNRS 8520, Institut d'Electronique de Microélectronique et de Nanotechnologie, Villeneuve d'Ascq, France; |
IDEALS Archive (Abstract PDF / Presentation File) |
DOI: https://dx.doi.org/10.15278/isms.2018.WI04 |
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Inversion of population in the terahertz (THz) range can be obtained thanks to the optical pumping of polar molecules in the mid-infrared range. Generally it is done with CO2 lasers but recently we have demonstrated the first molecular laser pumped by a quantum cascade laser (QCL). It is based on the optical pumping of the NH3 molecule in the ν2=1 state. The gain is obtained by the stimulated emission on pure inversion transitions of NH3 (large amplitude motions) around 1 THz that are not accessible to continuous-wave (CW) CO2 lasers. We present here CW high-resolution gain measurements of two strong lines: the (3,3) around 1.073 THz and the (4,4) around 1.083 THz. The measurements are done with a THz multiplication chain and an InSb bolometer. The gain profiles are recorded at different pressure and different QCL frequencies as for an IR/THz double resonance experiment. The highest gain at the best conditions are obtained with the (3,3) line: 10 dB/m for a pump power of about 40 mW. To our knowledge this gain is highest measured in the THz range for a CW-pumped molecule. These measurements will help the understanding and the design of our NH3 lasers. This kind of laser will find applications in THz molecular spectroscopy/astronomy as a source or as a local oscillator for heterodyne detection.
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03:10 PM |
INTERMISSION |
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WI05 |
Invited Mini-Symposium Talk |
30 min |
03:44 PM - 04:14 PM |
P3070: EXPLORING THE SOLID STATE PHASE TRANSITION IN DL-NORVALINE WITH TERAHERTZ SPECTROSCOPY |
JENS NEU, COLEEN T. NEMES, KEVIN P. REGAN, Department of Chemistry, Yale University, New Haven, CT, USA; MICHAEL R. C. WILLIAMS, Center for Integrated Nanotechnologies, Los Alamos National Laboratory, Los Alamos, NM, USA; CHARLES A. SCHMUTTENMAER, Department of Chemistry, Yale University, New Haven, CT, USA; |
IDEALS Archive (Abstract PDF / Presentation File) |
DOI: https://dx.doi.org/10.15278/isms.2018.WI05 |
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DL-Norvaline is a molecular crystal at room temperature and it undergoes a phase transition when cooled below 190 K. This phase transition is believed to be Martensitic. We investigate this phase transition by measuring its terahertz (THz) spectrum over a range of temperatures. Temperature-dependent THz time-domain spectroscopy (THz-TDS) measurements reveal that the transition temperature (Tβ→ α) is 190 K. The influence of nucleation seeds was analyzed by determining the Tβ→ α of molecular crystals with varying grain size. Grains of 5 μm or less result in a lower transition temperature (Tβ→ α = 180 K) compared to larger grains of 125–250 μm (Tβ→ α = 190 K). Additionally, we gain insight into the physical process of the phase transition via temperature-dependent THz-TDS spectra of doped and mixed molecular crystals. The addition of molecular dopants, which differ from DL-norvaline only at the end of the side chain which resides in the hydrophobic layers of the crystal, decreases Tβ→ α. This is consistent with a solid-solid phase transition in which the unit cell shifts along this hydrophobic layer, and it leads us to believe that the phase transition in DL-norvaline is Martensitic in nature.
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WI06 |
Contributed Talk |
15 min |
04:18 PM - 04:33 PM |
P2980: PULSE-ECHO MILLIMETER WAVE IN SITU SENSOR WITH 65 nm CMOS TRANSMITTER AND HETERODYNE RECEIVER ELECTRONICS |
DEACON J NEMCHICK, BRIAN DROUIN, ADRIAN TANG, YANGHYO KIM, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA; GABRIEL VIRBILA, M.-C. FRANK CHANG, Electrical Engineering, University of California - Los Angeles, Los Angeles, CA, USA; |
IDEALS Archive (Abstract PDF / Presentation File) |
DOI: https://dx.doi.org/10.15278/isms.2018.WI06 |
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l0pt
Figure
Cavity enhanced pure rotational spectroscopy has long been a potent laboratory tool for the elucidation of structure and dynamics in isolated molecular systems where sensitive pulsed-echo techniques are routinely performed up to frequencies as high ∼ 50 GHz. Although the associated narrow linewidths ( ∼ 800kHz), wide-bandwidth (often > 10 GHz), and long optical path lengths have long been identified as a desirable combination for sensitive and specific gas sensing, the unaccommodating size and power requirements of traditional microwave optics/electronics are unsuitable for the stringent demands required for in situ deployment. Additionally, efforts to drive pulsed-echo techniques into millimeter and submillimeter wavelength regimes, where the size of optics can be reduced without suffering large diffraction losses, have failed largely due to inefficiencies of injecting radiation into the resonant optical cavity.
Recent pursuits at the Jet Propulsion Laboratory to realize compact, low-power devices capable of in situ chemical detections on extra-terrestrial objects have found success in calling upon novel transmitter and receiver elements built from CMOS architectures commonly employed in the high-speed communications industry. These low-power integrated circuit chipsets can be embedded directly into quasi-optical devices allowing for the realization of cavity based instruments where all source and detection electronics are hosted by a single 16 in 2 printed circuit board. The current talk will present a full system description of this miniaturized CMOS-based pulse-echo rotational spectrometer, D. J. Nemchick et al., "A 90-102 GHz CMOS Based Pulsed-Echo Fourier Transform Spectrometer: New Approaches for In Situ Chemical Detection and Millimeter-Wave Cavity-Based Molecular Spectroscopy," Rev. Sci. Inst., In Submission.hich has an operational bandwidth of 90-105 GHz, along with experimental trials taken in bulk gas flows and seeded molecular beam environments.
Footnotes:
D. J. Nemchick et al., "A 90-102 GHz CMOS Based Pulsed-Echo Fourier Transform Spectrometer: New Approaches for In Situ Chemical Detection and Millimeter-Wave Cavity-Based Molecular Spectroscopy," Rev. Sci. Inst., In Submission.w
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WI07 |
Contributed Talk |
15 min |
04:35 PM - 04:50 PM |
P3175: FOURIER TRANSFORM MILLIMETER-WAVE SPECTROMETER WITH ORIGINAL DESIGN |
R. A. MOTIYENKO, L. MARGULÈS, Laboratoire PhLAM, UMR 8523 CNRS - Université Lille 1, Villeneuve d'Ascq, France; E. A. ALEKSEEV, Radiospectrometry Department, Institute of Radio Astronomy of NASU, Kharkov, Ukraine; |
IDEALS Archive (Abstract PDF / Presentation File) |
DOI: https://dx.doi.org/10.15278/isms.2018.WI07 |
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Direct digital synthesizers (DDS) have a number of advantages, especially such as the high precision and rate of frequency adjustment. In addition, these synthesizers possess a unique property to allow changing the frequency from one value to another with continuous phase. Few years ago, we built fast-scan absorption spectrometer with Schottky diode frequency multiplication chains as a radiation source. A. Pienkina, R.A. Motiyenko, L. Margulès et al. ISMS, 71st symposium (2016), FB05he rapid frequency scan in the spectrometer is provided by RF synthesizer based on up-conversion of the DDS signal. Owing to the capability of fast frequency switching, the same up-converted RF synthesizer may generate short pulses to polarize molecules and subsequently may be used as a local oscillator in the heterodyne detection of free induction decay. This feature simplifies the spectrometer design, as it allows using only one radiation source to polarize molecular sample, and to detect molecular signal. Using this principle, we built a Fourier transform spectrometer in the millimeter wave range. The spectrometer covers the frequency range between 150 and 220 GHz. In the current design, the RF synthesizer allows generation of frequency pulses with a bandwidth inverse proportional to pulse duration, as well as chirped pulses with a bandwidth of about 350 MHz. The performances of the spectrometer will be presented and discussed.
Footnotes:
A. Pienkina, R.A. Motiyenko, L. Margulès et al. ISMS, 71st symposium (2016), FB05T
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WI08 |
Contributed Talk |
15 min |
04:52 PM - 05:07 PM |
P2927: THE ROTATIONAL SPECTRUM OF THE METHANETHIOL ISOTOPOLOG CH334SH |
OLENA ZAKHARENKO, FRANK LEWEN, STEPHAN SCHLEMMER, HOLGER S. P. MÜLLER, I. Physikalisches Institut, Universität zu Köln, Köln, Germany; V. ILYUSHIN, E. A. ALEKSEEV, IGOR KRAPIVIN, Radiospectrometry Department, Institute of Radio Astronomy of NASU, Kharkov, Ukraine; LI-HONG XU, RONALD M. LEES, Department of Physics, University of New Brunswick, Saint John, NB, Canada; ROBIN T. GARROD, Departments of Chemistry and Astronomy, The University of Virginia, Charlottesville, VA, USA; ARNAUD BELLOCHE, KARL M. MENTEN, Millimeter- und Submillimeter-Astronomie, Max-Planck-Institut für Radioastronomie, Bonn, NRW, Germany; |
IDEALS Archive (Abstract PDF / Presentation File) |
DOI: https://dx.doi.org/10.15278/isms.2018.WI08 |
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Methanethiol, CH 3SH, has been found in the warm and dense parts of high as well as low mass star-forming regions. See, e.g., H. S. P. Müller at al., Astron. Astrophys. 587 (2016) A92; M. N. Drozdovskaya et al., Mon. Not. R. Astron. Soc., accepted, arXiv: 1802.02977; and references therein.he molecule is also of fundamental interest because of the large amplitude internal rotation of the CH 3 group whose effects are somewhat less pronounced than in its lighter homolog CH 3OH. In the course of our ongoing study of CH 332SH, V. Ilyushin et al., TI04 at the 72nd ISMS, 2017e have recorded new spectra which currently cover 49−510 GHz. The work in Kharkov was done under support of the Volkswagen foundation. The assistance of the Science and Technology Center in the Ukraine is acknowledged (STCU partner project #P686). The work in Cologne was supported by the Deutsche Forschungsgemeinschaft (DFG) via grant SFB 956, project B3 and via the Gerätezentrum "Cologne Center for Terahertz Spectroscopy".hese spectra, as well as existing ones covering part of the 1.1−1.5 THz region, L.-H. Xu at al., J. Chem. Phys. 137 (2012) 104313.ere inspected for lines of CH 334SH. We made extensive assignments of ∆K = 0 transitions in v t = 0 to 2. Numerous assignments of ∆K = ±1 transitions were made in v t = 0 and to a lesser extent in the two higher torsional states. We will present results of modeling these data with the RAM36 program and of searches for this isotopolog in our 3 mm ALMA data of Sagittarius B2(N).
Footnotes:
See, e.g., H. S. P. Müller at al., Astron. Astrophys. 587 (2016) A92; M. N. Drozdovskaya et al., Mon. Not. R. Astron. Soc., accepted, arXiv: 1802.02977; and references therein.T
V. Ilyushin et al., TI04 at the 72nd ISMS, 2017w
The work in Kharkov was done under support of the Volkswagen foundation. The assistance of the Science and Technology Center in the Ukraine is acknowledged (STCU partner project #P686). The work in Cologne was supported by the Deutsche Forschungsgemeinschaft (DFG) via grant SFB 956, project B3 and via the Gerätezentrum "Cologne Center for Terahertz Spectroscopy".T
L.-H. Xu at al., J. Chem. Phys. 137 (2012) 104313.w
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