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Transition Metal Complexes of Dicyanoacetylene
Louisiana State University LSU Digital Commons LSU Historical Dissertations and Theses Graduate School 1971 Transition Metal Complexes of Dicyanoacetylene: a Study of the Reaction Chemistry of Low Valence States of the Transition Metals, Platinum, Palladium, Nickel, Rhodium, and Iridium. Gregory Lloyd Mcclure Louisiana State University and Agricultural & Mechanical College Follow this and additional works at: https://digitalcommons.lsu.edu/gradschool_disstheses Recommended Citation Mcclure, Gregory Lloyd, "Transition Metal Complexes of Dicyanoacetylene: a Study of the Reaction Chemistry of Low Valence States of the Transition Metals, Platinum, Palladium, Nickel, Rhodium, and Iridium." (1971). LSU Historical Dissertations and Theses. 2001. https://digitalcommons.lsu.edu/gradschool_disstheses/2001 This Dissertation is brought to you for free and open access by the Graduate School at LSU Digital Commons. It has been accepted for inclusion in LSU Historical Dissertations and Theses by an authorized administrator of LSU Digital Commons. For more information, please contact [email protected]. 71-29,382 McCLURE, Gregory Lloyd, 1993- TRANSITION METAL COMPLEXES OF DICYANOACETYLENE: A STUDY OF THE REACTION CHEMISTRY OF LOW VALENCE STATES OF THE TRANSITION METALS, PLATINUM, PALLADIUM, NICKEL, RHODIUM, AND IRIDIUM. The Louisiana State University and Agricultural and Mechanical College, Ph.D., 1971 C hem i stry, inorgan ic University Microfilms, A XEROX Company , Ann Arbor. Michigan THIS DISSERTATION HAS BEEN MICROFILMED EXACTLY AS RECEIVED TRANSITION -
Ionization Photophysics and Spectroscopy of Dicyanoacetylene Sydney Leach, Martin Schwell, Gustavo A
Ionization photophysics and spectroscopy of dicyanoacetylene Sydney Leach, Martin Schwell, Gustavo A. Garcia, Yves Bénilan, Nicolas Fray, Marie-Claire Gazeau, François Gaie-Levrel, Norbert Champion, and Jean-Claude Guillemin Citation: The Journal of Chemical Physics 139, 184304 (2013); doi: 10.1063/1.4826467 View online: http://dx.doi.org/10.1063/1.4826467 View Table of Contents: http://scitation.aip.org/content/aip/journal/jcp/139/18?ver=pdfcov Published by the AIP Publishing This article is copyrighted as indicated in the article. Reuse of AIP content is subject to the terms at: http://scitation.aip.org/termsconditions. Downloaded to IP: 193.51.99.1 On: Wed, 05 Feb 2014 16:48:49 THE JOURNAL OF CHEMICAL PHYSICS 139, 184304 (2013) Ionization photophysics and spectroscopy of dicyanoacetylene Sydney Leach,1,a) Martin Schwell,2,a) Gustavo A. Garcia,3 Yves Bénilan,2 Nicolas Fray,2 Marie-Claire Gazeau,2 François Gaie-Levrel,3,b) Norbert Champion,1 and Jean-Claude Guillemin4 1LERMA UMR CNRS 8112, Observatoire de Paris-Meudon, 5 place Jules-Jansen, 92195 Meudon, France 2LISA UMR CNRS 7583, Université Paris-Est Créteil and Université Paris Diderot, Institut Pierre Simon Laplace, 61 Avenue du Général de Gaulle, 94010 Créteil, France 3Synchrotron SOLEIL, L’Orme des Merisiers, St. Aubin, B.P. 48, 91192 Gif-sur-Yvette Cedex, France 4Institut des Sciences Chimiques de Rennes, Ecole Nationale Supérieure de Chimie de Rennes, CNRS UMR 6226, 11 Allée de Beaulieu, CS 50837, 35708 Rennes Cedex 7, France (Received 17 June 2013; accepted 8 October 2013; published online 11 November 2013) Photoionization of dicyanoacetylene was studied using synchrotron radiation over the excitation range 8–25 eV, with photoelectron-photoion coincidence techniques. -
Polymerization of Dicyanoacetylene † ‡ ○ † ○ ■ ¶ § ■ § ■ Huiyang Gou,*, , , Li Zhu, , Haw-Tyng Huang, , Arani Biswas, , Derek W
Article pubs.acs.org/cm From Linear Molecular Chains to Extended Polycyclic Networks: Polymerization of Dicyanoacetylene † ‡ ○ † ○ ■ ¶ § ■ § ■ Huiyang Gou,*, , , Li Zhu, , Haw-Tyng Huang, , Arani Biswas, , Derek W. Keefer, , ∥ ◆ ⊥ † ‡ † ‡ † Brian L. Chaloux, , Clemens Prescher, Liuxiang Yang, , Duck Young Kim, , Matthew D. Ward, ■ # # ∇ ∥ § ■ ¶ □ Jordan Lerach, Shengnan Wang, Artem R. Oganov, , Albert Epshteyn, John V. Badding, , , , † and Timothy A. Strobel*, † Geophysical Laboratory, Carnegie Institution of Washington, Washington, DC 20015, United States ‡ Center for High Pressure Science and Technology Advanced Research, Beijing 100094, China § Department of Chemistry, The Pennsylvania State University, University Park, Pennsylvania 16802, United States ■ Materials Research Institute, The Pennsylvania State University, University Park, Pennsylvania 16802, United States ¶ Department of Materials Science and Engineering, The Pennsylvania State University, University Park, Pennsylvania 16802, United States □ Department of Physics, The Pennsylvania State University, University Park, Pennsylvania 16802, United States ∥ Naval Research Laboratory, 4555 Overlook Avenue, SW, Washington, DC 20375, United States ⊥ Center for Advanced Radiation Sources, University of Chicago, Argonne, Illinois 60437, United States # Department of Geosciences, Center for Materials by Design, and Institute for Advanced Computational Science, State University of New York, Stony Brook, New York 11794-2100, United States ∇ Skolkovo Institute of Science and Technology, -
The Center for the Study of Terrestrial and Extraterrestrial Atmospheres (CSTEA) Dr
_ ; i •_ '. : .' _ ";¢ hi-__¸_:_7 NASA-CR-204199 The Center For The Study Of Terrestrial And Extraterrestrial Atmospheres (CSTEA) Dr. Arthur N. Thorpe, Director Dr. Vernon R. Morris, Deputy Director Funded By The National Aeronautics And Space Administration (NASA) NAGW 2950 Five-Year Report April 1992-December 1996 Howard University 2216 6th Street, NW Room 103 Washington, DC 20059 202-806-5172 202-806-4430 (FAX) URL Home Page: http://www.cstea.howard.edu e-mail: thorpe@ cstea.cstea.howard.edu TABLE OF CONTENTS CSTEA's Existence ... Then And Now 1 The CSTEA PIs ... Their Research And Students 6 Dr. Peter Bainum ... 7 Dr. Anand Batra ... 10 Dr. Robert Catchings ... 10 Dr. L. Y. Chiu ... 11 Dr. Balaram Dey ... 13 Dr. Joshua Halpern ... 14 Dr. Peter Hambright ... 20 Dr. Gary Harris ... 24 Dr. Lewis Klein ... 26 Dr. Cidambi Kumar ... 28 Dr. James Lindesay ... 29 Dr. Prabhakar Misra ... 32 Dr. Vernon Morris ... 35 Dr. Hideo Okabe ... 39 Dr. Steven Pollack ... 41 Dr. Steven Richardson ... 42 Dr. Yehuda Salu ... 43 Dr. Sonya Smith ... 45 Dr. Michael Spencer ... 46 Dr. George Morgenthaler ... 48 Five Year Report (April 1992-31 December 1996) Center for the Study of Terrestrial and Extraterrestrial Atmospheres (CSTEA) Dr. Arthur N. Thorpe, Director CSTEA's EXISTENCE ... THEN AND NOW The Center for the Study of Terrestrial and Extraterrestrial Atmospheres (CSTEA) was established in 1992 by a grant from the National Aeronautics and Space Administra- tion (NASA) Minority University Research and Education Division (MURED). Since CSTEA was first proposed in October of 1991 by Dr. William Gates, then Chairman of the Department of Physics at Howard University, it has become a world-class, comprehen- sive, nationally competitive university center for atmospheric research .. -
The Neutral Photochemistry of Nitriles, Amines and Imines in the Atmosphere of Titan
The neutral photochemistry of nitriles, amines and imines in the atmosphere of Titan J.C. Loisonc,d, E. H´ebrarda,b, M. Dobrijevica,b,∗, K.M. Hicksonc,d, F. Caralpc,d, V. Huea,b, G. Gronoffe, O. Venotf, Y. Benilang aUniversit´ede Bordeaux, Laboratoire d'Astrophysique de Bordeaux, UMR 5804, F-33270 Floirac, France bCNRS, Laboratoire d'Astrophysique de Bordeaux, UMR 5804, F-33270, Floirac, France cUniversit´ede Bordeaux, Institut des Sciences Mol´eculaires, UMR 5255, F-33400 Talence, France dCNRS, Institut des Sciences Mol´eculaires, UMR 5255, F-33400 Talence, France eSSAI/NASA LaRC, Hampton, Va, USA fKatholieke Univ Leuven, Inst Sterrenkunde, B-3001 Louvain, Belgium gLaboratoire Interuniversitaire des Syst`emesAtmosph´eriques, UMR CNRS 7583, Universit´esParis Est Cr´eteil(UPEC) et Paris Diderot (UPD), Cr´eteil,France Abstract The photochemistry of N2 and CH4 in the atmosphere of Titan leads to a very rich chemistry which is not well understood. The aim of our study is to improve our understanding of the production of nitrogen compounds and to predict the abundances of those with high molar mass with better accuracy. We have made a careful investigation of the neutral nitrogen photochemistry to improve current chemical schemes including the most abundant species and the most efficient reactions. We also studied the propagation of uncertainties on rate constants in our model and determined the key reactions from a global sensitivity analysis. Our photochemical model contains 124 species, 60 of which are nitrogen con- taining compounds, and 1141 reactions. Our results are in reasonable agreement with Cassini/INMS data in the higher atmosphere but our model overestimates the mole fractions of several nitriles in the lower stratosphere. -
SUPLEMENTARY INFORMATION Canonical and Explicitly-Correlated
Electronic Supplementary Material (ESI) for Physical Chemistry Chemical Physics. This journal is © the Owner Societies 2021 SUPLEMENTARY INFORMATION Canonical and explicitly-correlated coupled cluster correlation energies of sub-kJ/mol accuracy via cost-effective hybrid-post-CBS extrapolation A.J.C. Varandas∗,y,z,{ yDepartment of Physics, Qufu Normal University, China zDepartment of Physics, Universidade Federal do Espírito Santo, 29075-910 Vitória, Brazil {Department of Chemistry, and Chemistry Centre, University of Coimbra, 3004-535 Coimbra, Portugal E-mail: [email protected] Table 1: Systems in TS-106 # in TS-106 Formula Name # in A24 + TS-106 1 CFN Cyanogen fluoride 25 2 CFN Isocyanogen fluoride 26 3 CF2 Singlet difluoromethylene 27 4 CF2O Carbonyl fluoride 28 Continued on next page 1 continued from previous page # in TS-106 Formula Name # in A24 + TS-106 5 CF4 Tetrafluoromethane 29 6 CHF Singlet fluoromethylene 30 7 CHFO Formyl fluoride 31 8 CHF3 Trifluoromethane 32 9 CHN Hydrogen cyanide 33 10 CHN Hydrogen isocyanide 34 11 CHNO Cyanic acid 35 12 CHNO Isocyanic acid 36 13 CHNO Formonitrile oxide 37 14 CHNO Isofulminic acid 38 15 CH2 Singlet methylene 39 16 CH2F2 Difluoromethane 40 17 CH2N2 Cyanamide 41 18 CH2N2 3H-Diazirine 42 19 CH2N2 Diazomethane 43 20 CH2O Formaldehyde 44 21 CH2O Hydroxymethylene 45 22 CH2O2 Dioxirane 46 23 CH2O2 Formic acid 47 ∗ 24 CH2O3 Performic acid 48 25 CH3F Fluoromethane 49 26 CH3N Methanimine 50 27 CH3NO Formamide 51 ∗ 28 CH3NO2 Methyl nitrite 52 Continued on next page 2 continued from previous page # in TS-106 Formula -
Polymerization of Dicyanoacetylene † ‡ ○ † ○ ■ ¶ § ■ § ■ Huiyang Gou,*, , , Li Zhu, , Haw-Tyng Huang, , Arani Biswas, , Derek W
Article pubs.acs.org/cm From Linear Molecular Chains to Extended Polycyclic Networks: Polymerization of Dicyanoacetylene † ‡ ○ † ○ ■ ¶ § ■ § ■ Huiyang Gou,*, , , Li Zhu, , Haw-Tyng Huang, , Arani Biswas, , Derek W. Keefer, , ∥ ◆ ⊥ † ‡ † ‡ † Brian L. Chaloux, , Clemens Prescher, Liuxiang Yang, , Duck Young Kim, , Matthew D. Ward, ■ # # ∇ ∥ § ■ ¶ □ Jordan Lerach, Shengnan Wang, Artem R. Oganov, , Albert Epshteyn, John V. Badding, , , , † and Timothy A. Strobel*, † Geophysical Laboratory, Carnegie Institution of Washington, Washington, DC 20015, United States ‡ Center for High Pressure Science and Technology Advanced Research, Beijing 100094, China § Department of Chemistry, The Pennsylvania State University, University Park, Pennsylvania 16802, United States ■ Materials Research Institute, The Pennsylvania State University, University Park, Pennsylvania 16802, United States ¶ Department of Materials Science and Engineering, The Pennsylvania State University, University Park, Pennsylvania 16802, United States □ Department of Physics, The Pennsylvania State University, University Park, Pennsylvania 16802, United States ∥ Naval Research Laboratory, 4555 Overlook Avenue, SW, Washington, DC 20375, United States ⊥ Center for Advanced Radiation Sources, University of Chicago, Argonne, Illinois 60437, United States # Department of Geosciences, Center for Materials by Design, and Institute for Advanced Computational Science, State University of New York, Stony Brook, New York 11794-2100, United States ∇ Skolkovo Institute of Science and Technology, -
Pyrolysis and Combustion of Acetonitrile (Ch3cn)
OAK RIDGE ORNL/TM-2002/113 NATIONAL LABORATORY MANAGED BY UT-BATTELLE FOR THE DEPARTMENT OF ENERGY Pyrolysis and Combustion of Acetonitrile (CH3CN) Phillip F. Britt DOCUMENT AVAILABILITY Reports produced after January 1, 1996, are generally available free via the U.S. Department of Energy (DOE) Information Bridge. Web site http://www.osti.gov/bridge Reports produced before January 1, 1996, may be purchased by members of the public from the following source. National Technical Information Service 5285 Port Royal Road Springfield, VA 22161 Telephone 703-605-6000 (1-800-553-6847) TDD 703-487-4639 Fax 703-605-6900 E-mail [email protected] Web site http://www.ntis.gov/support/ordernowabout.htm Reports are available to DOE employees, DOE contractors, Energy Technology Data Exchange (ETDE) representatives, and International Nuclear Information System (INIS) representatives from the following source. Office of Scientific and Technical Information P.O. Box 62 Oak Ridge, TN 37831 Telephone 865-576-8401 Fax 865-576-5728 E-mail [email protected] Web site http://www.osti.gov/contact.html This report was prepared as an account of work sponsored by an agency of the United States Government. Neither the United States Government nor any agency thereof, nor any of their employees, makes any warranty, express or implied, or assumes any legal liability or responsibility for the accuracy, completeness, or usefulness of any information, apparatus, product, or process disclosed, or represents that its use would not infringe privately owned rights. Reference herein to any specific commercial product, process, or service by trade name, trademark, manufacturer, or otherwise, does not necessarily constitute or imply its endorsement, recommendation, or favoring by the United States Government or any agency thereof. -
Nasa Scientists Find 'Impossible' Cloud on Titan—Again 21 September 2016, by Preston Dyches
Nasa scientists find 'impossible' cloud on Titan—again 21 September 2016, by Preston Dyches this one on Titan. What has puzzled scientists ever since is this: they detected less than 1 percent of the dicyanoacetylene gas needed for the cloud to condense. Recent observations from NASA's Cassini mission yielded a similar result. Using Cassini's composite infrared spectrometer, or CIRS—which can identify the spectral fingerprints of individual chemicals in the atmospheric brew—researchers found a large, high-altitude cloud made of the same frozen chemical. Yet, just as Voyager found, when it comes to the vapor form of this chemical, CIRS reported that Titan's stratosphere is as dry as a desert. "The appearance of this ice cloud goes against everything we know about the way clouds form on Titan," said Carrie Anderson, a CIRS co- investigator at NASA's Goddard Space Flight Center in Greenbelt, Maryland, and lead author of the study. The hazy globe of Titan hangs in front of Saturn and its rings in this natural color view from NASA's Cassini spacecraft. Credit: NASA/JPL-Caltech/Space Science The typical process for forming clouds involves Institute condensation. On Earth, we're familiar with the cycle of evaporation and condensation of water. The same kind of cycle takes place in Titan's troposphere—the weather-forming layer of Titan's The puzzling appearance of an ice cloud atmosphere—but with methane instead of water. seemingly out of thin air has prompted NASA scientists to suggest that a different process than A different condensation process takes place in the previously thought—possibly similar to one seen stratosphere—the region above the troposphere—at over Earth's poles—could be forming clouds on Titan's north and south winter poles. -
Suplementary Information
Electronic Supplementary Material (ESI) for Physical Chemistry Chemical Physics. This journal is © the Owner Societies 2018 SUPLEMENTARY INFORMATION CBS extrapolation in electronic structure pushed to end: A revival of minimal and sub-minimal basis sets A.J.C. Varandas∗,y,z ySchool of Physics and Physical Engineering, Qufu Normal University, 273165 Qufu, China. zChemistry Centre and Department of Chemistry, University of Coimbra, 3004-535 Coimbra, Portugal E-mail: [email protected] Table 1: TS-106 and TS-106’ of molecular systems # in TS-106 Formula Name # in TS-106’ 1 CFN Cyanogen fluoride 1 2 CFN Isocyanogen fluoride 2 3 CF2 Singlet difluoromethylene 3 4 CF2O Carbonyl fluoride 4 5 CF4 Tetrafluoromethane 5 Continued on next page 1 continued from previous page # in TS-106 Formula Name # in TS-106’ 6 CHF Singlet fluoromethylene 6 7 CHFO Formyl fluoride 7 8 CHF3 Trifluoromethane 8 9 CHN Hydrogen cyanide 9 10 CHN Hydrogen isocyanide 10 11 CHNO Cyanic acid 11 12 CHNO Isocyanic acid 12 13 CHNO Formonitrile oxide 13 14 CHNO Isofulminic acid 14 15 CH2 Singlet methylene 15 16 CH2F2 Difluoromethane 16 17 CH2N2 Cyanamide 17 18 CH2N2 3H-Diazirine 18 19 CH2N2 Diazomethane 19 20 CH2O Formaldehyde 20 21 CH2O Hydroxymethylene 21 22 CH2O2 Dioxirane 22 23 CH2O2 Formic acid 23 ∗ 24 CH2O3 Performic acid 74 25 CH3F Fluoromethane 24 26 CH3N Methanimine 25 27 CH3NO Formamide 26 ∗ 28 CH3NO2 Methyl nitrite 75 ∗ 29 CH3NO2 Nitromethane 76 Continued on next page 2 continued from previous page # in TS-106 Formula Name # in TS-106’ 30 CH4 Methane 27 ∗ 31 CH4N2O Urea 77 32 CH4O -
Photodissociation Dynamics in Titan's Atmosphere Welvidanalage Ruchira Silva Wayne State University
Wayne State University DigitalCommons@WayneState Wayne State University Dissertations 1-1-2010 Photodissociation Dynamics In Titan's Atmosphere Welvidanalage Ruchira Silva Wayne State University Follow this and additional works at: http://digitalcommons.wayne.edu/oa_dissertations Recommended Citation Silva, Welvidanalage Ruchira, "Photodissociation Dynamics In Titan's Atmosphere" (2010). Wayne State University Dissertations. Paper 63. This Open Access Dissertation is brought to you for free and open access by DigitalCommons@WayneState. It has been accepted for inclusion in Wayne State University Dissertations by an authorized administrator of DigitalCommons@WayneState. PHOTODISSOCIATION DYNAMICS IN TITAN’S ATMOSPHERE by W. RUCHIRA SILVA DISSERTATION Submitted to the Graduate School of Wayne State University, Detroit, Michigan in partial fulfillment of the requirements for the degree of DOCTOR OF PHILOSOPHY 2010 MAJOR: CHEMISTRY (Physical) Approved by: Advisor Date © COPYRIGHT BY WELVIDANALAGE RUCHIRA ROHAN SILVA 2010 All Rights Reserved DEDICATION ~ To my Parents, Madu and Netuli… ii ACKNOWLEDGMENTS First and foremost, I owe my deepest gratitude to my advisor, Professor Arthur G. Suits, whose guidance, encouragement and support enabled me to complete my graduate studies through Wayne State University. This dissertation would not have been possible without his forgiveness, kind considerations, great efforts and continuous support. I am very fortunate to have an advisor like Prof. Suits who not only guided me to understand the subject but also helped me to overcome every major difficulty I faced in my life over the last five years. If it was not his support my dreams would not have become a reality. His passion towards research is inspiring and motivating. I’m grateful for him for everything I learnt throughout my graduate career. -
Enthalpies of Vaporization of Organic and Organometallic Compounds, 1880–2002
Enthalpies of Vaporization of Organic and Organometallic Compounds, 1880–2002 James S. Chickosa… Department of Chemistry, University of Missouri-St. Louis, St. Louis, Missouri 63121 William E. Acree, Jr.b… Department of Chemistry, University of North Texas, Denton, Texas 76203 ͑Received 17 June 2002; accepted 17 October 2002; published 21 April 2003͒ A compendium of vaporization enthalpies published within the period 1910–2002 is reported. A brief review of temperature adjustments of vaporization enthalpies from temperature of measurement to the standard reference temperature, 298.15 K, is included as are recently suggested reference materials. Vaporization enthalpies are included for organic, organo-metallic, and a few inorganic compounds. This compendium is the third in a series focusing on phase change enthalpies. Previous compendia focused on fusion and sublimation enthalpies. Sufficient data are presently available for many compounds that thermodynamic cycles can be constructed to evaluate the reliability of the measure- ments. A protocol for doing so is described. © 2003 American Institute of Physics. ͓DOI: 10.1063/1.1529214͔ Key words: compendium; enthalpies of condensation; evaporation; organic compounds; vaporization enthalpy. Contents inorganic compounds, 1880–2002. ............. 820 1. Introduction................................ 519 8. References to Tables 6 and 7.................. 853 2. Reference Materials for Vaporization Enthalpy Measurements.............................. 520 List of Figures 3. Heat Capacity Adjustments. ................. 520 1. A thermodynamic cycle for adjusting vaporization ϭ 4. Group Additivity Values for C (298.15 K) enthalpies to T 298.15 K.................... 521 pl 2. A hypothetical molecule illustrating the different Estimations................................ 521 hydrocarbon groups in estimating C ........... 523 5. A Thermochemical Cycle: Sublimation, p Vaporization, and Fusion Enthalpies...........