REACTIONS of HALOCYCLOPROPANES. The

Total Page:16

File Type:pdf, Size:1020Kb

REACTIONS of HALOCYCLOPROPANES. The This dissertation has been microfilmed exactly as received 69-11,652 HOUSER, Charles W., 1934- REACTIONS OF HALOCYCLOPROPANES. The Ohio State University, Ph.D., 1968 Chemistry, organic University Microfilms, Inc., Ann Arbor, Michigan REACTIONS OF HALOCYCLOPROPANES DISSERTATION Presented in Partial Fulfillment of the Requirements for the Degree Doctor of Philosophy in the Graduate School o f The Ohio State U niversity By Charles W. Houser, B.A. ******** The Ohio State U niversity 1968 Approved hy /Adviser Department of Chemistry Dedicated to Jane and Brian i l ACKNOWLEDGMENTS The author wishes to express sincere appreciation to Professor Harold Shechter for the inception of this problem and for his helpful discussions throughout the course of this research. His editorial guidance during preparation of this manuscript is also gratefully acknowledged. National Science Foundation and Petroleum Research Fund are thanked for their financial assistance to this research. The author owes a special debt of gratitude to his wife, Jane, for her patience and encouragement during completion of this work. i i i VITA October 20, 1934 Born - Parkersburg, West Virginia 1954-1958 U. S. Marine Corps 1962 B.A., David Lipscomb College, Nashville, Tennessee 1962-1965 Teaching Assistant, The Ohio State University, Columbus, Ohio I965-I968 Research Associate, The Ohio State University, Columbus, Ohio iv CONTENTS Page ACKNOWLEDGMENTS.......................................................................................................... i i i VITA .......................................................................... iv TABLES ..................................................................................................... .................. STATEMENT OF PROBLEM ............................................................................................ 1 PART I INTRODUCTION.............................................................................................................. 7 DISCUSSION........................................................................................................................ 19 Syntheses of polyhalogenated cyclopropanes ........................................ 19 Thermal reaction s o f halocyclopropanes ...................................................... 22 Electrophilic reactions of halocyclopropanes with metal acetates ............................................................................................ 27 Reactions of halocyclopropanes with bases ........................................ 28 PART II INTRODUCTION .............................................................................................................. 46 Displacement reactions of 2,2-dichlorocyclopropylmethyl derivatives ................................................................................................. 46 DISCUSSION........................................................................................................................ 60 Displacement reactions of electronegatively substituted cyclopropylmethyl derivatives .......................................................... 60 EXPERIMENTAL..............................................................................................................• 77 Preparation of 3-bromo-l,l-dichloro-2,2-dimethylcyclopropane . j8 Preparation of l,l,3-trichloro-2,2-dimethylcyclopropane . 79 Preparation of l,l-dibromo-2,2-dichloro-3,3-diraethyl- cyclopropane ................................................................................ 79 Preparation of l,l,2,2-tetrachloro-3-phenylcyclopropane. 80 Preparation of methyl 2,2-dichloro-trans-3-phenylcyclo- propanecarboxylate ......................................................................................... 8l v CONTENTS (Contd.) Page Preparation of 2-(bromomethyl)-l,l-dichlorocyclopropane . 8l Preparation of l,l,2-trichloro-2-(chloromethyl)- cyclopropane ................................................................................................ 82 Preparation of (2,2-dichlorocyclopropyl)methyl acetate .... 82 Preparation of (2,2-dichlorocyclopropyl)methanol .......................... 83 Preparation of (2,2-dichlorocyclopropyl)methyl p-toluene- s u lf o n a t e ..................................................................... T .............................. 83 Attempted preparation of (2,2-dichlorocyclopropyl)- metbylamine .................... ..... 84 Preparation of (2,2-dichlorocyclopropyl)methylamine .................. 85 Preparation of 2,2,3,3-tetrachlorospiro(cyclopropane-l,9'- f lu o r e n e ) ......................................................................................................... 85 Preparation of methyl 2,2-dichlorocyclopropanecarboxylate . 86 Preparation of l,l-dichloro-2-cyanocyclopropane ........................... 87 Preparation of l,l,2,3-tetrachloro-2-(chloromethyl)cyclo- p ro p a n e ............................................................................................................. 87 Preparation of 2,2-dichlorocyclopropanecarboxaldehyde d ie th y l a c e ta l ............................................................................................ 88 Preparation of 2,2-dichlorocyclopropanecarboxaldehyde 2,4-dinitrophenylhydrazone ................................................................. 88 Thermal reaction of 3-kromo-l,l-dichloro-2,2-dimethyl- cyclopropane ................................................................................................ 89 Thermal reaction of l,l,3" ‘trichloro-2,2-dimethylcyclopropane . 89 Thermal reaction of l,l,2,2-tetrachloro-3-phenylcyclopropane . 89 Thermal reaction of 2,2,3j3-tetrachlorospiro(cyclopropane- l ,9'-fluorene) ............................................................................................ 90 Attempted thermal reaction of 2-(bromomethyl)-l,l- dichlorocyclopropane .............................................................................. 90 Attempted thermal reaction of l,l,2-trichloro-2-(chloro- me thy l) cyclopropane ................................................... ........ 90 Reaction of l,l,3-trichloro-2,2-dimethylcyclopropane vith alcoholic potassium hydroxide ..................................................... 91- Reaction of l,l,3-trichloro-2,2-dimethylcyclopropane vith lithium piperidide .............................. 92 Reaction of 1,1,3-trichloro-2,2-dimethylcyclopropane vith potassium jt-butoxide ...................................................................... 93 Reaction of 3"’bromo-l,l-dichloro-2,2-dimethylcyclopropane vith n-butyllithium .......................................................................... 93 Attempted reaction of l,l,3-trichloro-2,2-dimethylcyclopro- pane with sodium h yd rid e ............................................................. 94 Reaction of l,l,2,2-tetrachloro-3_phenylcyclopropane vith sodium h yd rid e ....................................... 94 Hydrolysis of 2,3j3-trichloro-l-phenylcyclopropene ...................... 95 Reaction of 2,3>3“trichloro-l-phenylcyclopropene vith toluene catalyzed by aluminum chloride ........................................ 96 vi CONTENTS (Contd.) Page Reaction of methyl 2,2-dichloro-trans-3-phenylcyclo- propanecarboxylate with methanolic potassium hydroxide . 96 Reaction of l,l,3-trichloro-2,2-dimethylcyclopropane vith sodium ..................................................................................................... 97 Reaction of l,l,3~trichloro-2,2-dimethylcyclopropane with magnesium and methyl iodide .................................................................. 98 Attempted reaction of l,l,3 -trichloro-2,2-dimethylcyclo- propane and l,l-dichioro-3-bromo-2,2-dimethylcyclo- propane vith zinc in a lco h o l ............................................................. 99 Reaction of 3-hromo-l>-dichloro-2,2-dimethylcyclopropane vith silver acetate ............................................... 100 Reaction of 2-(bromomethyl)-l,l-dichlorocyclopropane with sodium methoxide ............................................................................... 100 Reaction of 2-(bromomethyl)-l,l-dichlorocyclopropane with potassium t-butoxide . ............................................................. 101 Attempted reaction of 2 -(bromomethyl)-l,l-dichlorocyclo- propane with sodium hydride .................................................................. 101 Reactions of 2-(bromomethyl)-l,l-dichlorocyclopropane with sodium cyanide ................................................................................................. 102 Reaction of 2-(bromomethyl)-l,l-dichlorocyclopropane vith piperidine ................................................................................................. 102 Reaction of 2-(bromoraethyl)-l,l-dichlorocyclopropane with triphenylphosphine ........................................................................................ 103 Attempted oxidation of 2-(bromomethyl)-l,l-dichlorocyclo- propane with dimethyl sulfoxide ...................... 10*i- Reaction of 2-(bromomethyl)-l,l-dichlorocyclopropane with benzene and aluminum chloride .................................................................. 10^ Reaction of 2-(bromomethyl)-l,l-dichlorocyclopropane with silver acetate ................................................................................. 106 Solvolysis of (2,2-dichlorocyclopropyl)methyl £-toluene- sulfonate in acetic a c id .............................................................. 106 Reaction of (2,2-dichlorocyclopropyl)methylamine
Recommended publications
  • The Role of Norrish Type-I Chemistry in Photoactive Drugs: an Ab Initio Study of a Cyclopropenone-Enediyne Drug Precursor
    Leger, S. J., Marchetti, B., Ashfold, M. N. R., & Karsili, T. N. V. (2020). The Role of Norrish Type-I Chemistry in Photoactive Drugs: An ab initio Study of a Cyclopropenone-Enediyne Drug Precursor. Frontiers in Chemistry, 8, [596590]. https://doi.org/10.3389/fchem.2020.596590 Publisher's PDF, also known as Version of record License (if available): CC BY Link to published version (if available): 10.3389/fchem.2020.596590 Link to publication record in Explore Bristol Research PDF-document This is the final published version of the article (version of record). It first appeared online via Fromtiers Media at https://doi.org/10.3389/fchem.2020.596590. Please refer to any applicable terms of use of the publisher. University of Bristol - Explore Bristol Research General rights This document is made available in accordance with publisher policies. Please cite only the published version using the reference above. Full terms of use are available: http://www.bristol.ac.uk/red/research-policy/pure/user-guides/ebr-terms/ ORIGINAL RESEARCH published: 22 December 2020 doi: 10.3389/fchem.2020.596590 The Role of Norrish Type-I Chemistry in Photoactive Drugs: An ab initio Study of a Cyclopropenone-Enediyne Drug Precursor Spencer J. Léger 1,2, Barbara Marchetti 1, Michael N. R. Ashfold 3 and Tolga N. V. Karsili 1* 1 Department of Chemistry, University of Louisiana at Lafayette, Lafayette, LA, United States, 2 Department of Chemical Engineering, University of Louisiana at Lafayette, Lafayette, LA, United States, 3 School of Chemistry, University of Bristol, Bristol, United Kingdom We present a contemporary mechanistic description of the light-driven conversion of cyclopropenone containing enediyne (CPE) precusors to ring-opened species amenable to further Bergman cyclization and formation of stable biradical species that have been proposed for use in light-induced cancer treatment.
    [Show full text]
  • The Observed Chemical Structure of L1544? ?? S
    Astronomy & Astrophysics manuscript no. Maps_L1544 c ESO 2017 July 20, 2017 The observed chemical structure of L1544? ?? S. Spezzano, P. Caselli, L. Bizzocchi, B. M. Giuliano, and V. Lattanzi Max Planck Institute for Extraterrestrial Physics, Giessenbachstrasse 1, 85748 Garching, Germany July 20, 2017 ABSTRACT Context. Prior to star formation, pre-stellar cores accumulate matter towards the centre. As a consequence, their central density increases while the temperature decreases. Understanding the evolution of the chemistry and physics in this early phase is crucial to study the processes governing the formation of a star. Aims. We aim at studying the chemical differentiation of a prototypical pre-stellar core, L1544, by detailed molecular maps. In contrast with single pointing observations, we performed a deep study on the dependencies of chemistry on physical and external conditions. Methods. We present the emission maps of 39 different molecular transitions belonging to 22 different molecules in the central 6.25 arcmin2 of L1544. We classified our sample in five families, depending on the location of their emission peaks within the core. Furthermore, to systematically study the correlations among different molecules, we have performed the principal component analysis (PCA) on the integrated emission maps. The PCA allows us to reduce the amount of variables in our dataset. Finally, we compare the maps of the first three principal components with the H2 column density map, and the Tdust map of the core. Results. The results of our qualitative analysis is the classification of the molecules in our dataset in the following groups: (i) the c-C3H2 family (carbon chain molecules like C3H and CCS), (ii) the dust peak family (nitrogen-bearing species + like N2H ), (iii) the methanol peak family (oxygen-bearing molecules like methanol, SO and SO2), (iv) the HNCO peak family (HNCO, propyne and its deuterated isotopologues).
    [Show full text]
  • Exhaustive Product Analysis of Three Benzene Discharges by Microwave Spectroscopy Michael C
    pubs.acs.org/JPCA Article Exhaustive Product Analysis of Three Benzene Discharges by Microwave Spectroscopy Michael C. McCarthy,* Kin Long Kelvin Lee, P. Brandon Carroll, Jessica P. Porterfield, P. Bryan Changala, James H. Thorpe, and John F. Stanton Cite This: J. Phys. Chem. A 2020, 124, 5170−5181 Read Online ACCESS Metrics & More Article Recommendations *sı Supporting Information ABSTRACT: Using chirped and cavity microwave spectroscopies, automated double resonance, new high-speed fitting and deep learning algorithms, and large databases of computed structures, the discharge products of benzene alone, or in combination with molecular oxygen or nitrogen, have been exhaustively characterized between 6.5 and 26 GHz. In total, more than 3300 spectral features were observed; 89% of these, accounting for 97% of the total intensity, have now been assigned to 152 distinct chemical species and 60 of their variants (i.e., isotopic species and vibrationally excited states). Roughly 50 of the products are entirely new or poorly characterized at high resolution, including many heavier by mass than the precursor benzene. These findings provide direct evidence for a rich architecture of two- and three-dimensional carbon and indicate that benzene growth, particularly the formation of ring−chain molecules, occurs facilely under our experimental conditions. The present analysis also illustrates the utility of microwave spectroscopy as a precision tool for complex mixture analysis, irrespective of whether the rotational spectrum of a product species is known a priori or not. From this large quantity of data, for example, it is possible to determine with confidence the relative abundances of different product masses, but more importantly the relative abundances of different isomers with the same mass.
    [Show full text]
  • Possible Gas-Phase Syntheses for Seven Neutral Molecules Studied Recently with the Green Bank Telescope
    A&A 474, 521–527 (2007) Astronomy DOI: 10.1051/0004-6361:20078246 & c ESO 2007 Astrophysics Possible gas-phase syntheses for seven neutral molecules studied recently with the Green Bank Telescope D. Quan1 and E. Herbst2 1 Chemical Physics Program, The Ohio State University, Columbus, Ohio 43210, USA e-mail: [email protected] 2 Departments of Physics, Chemistry and Astronomy, The Ohio State University, Columbus, OH 43210, USA Received 9 July 2007 / Accepted 17 August 2007 ABSTRACT Aims. With the Green Bank telescope (GBT), seven neutral molecules have been newly detected or confirmed towards either the cold interstellar core TMC-1 or the hot core source Sgr B2(N) within the last 1–2 years. Towards TMC-1, the new molecules seen are cyanoallene (CH2CCHCN) and methyl triacetylene (CH3C6H) while methyl cyanoacetylene (CH3CCCN) and methyl cyanodiacety- lene (CH3C5N) were confirmed. Towards Sgr B2(N), the three newly detected molecules are cyclopropenone (c-C3H2O), ketenimine (CH2CNH), and acetamide (CH3CONH2); these are mainly seen in absorption and are primarily located in an envelope around the hot core. In this work, we report a detailed study of the gas-phase chemistry of all seven molecules. Methods. Starting with our updated gas-phase chemical reaction network osu.01.2007, we added formation and depletion reactions to treat the chemistry of each of the seven molecules. Some of these were already in our network but with incomplete chemistry, while most were not in the network at all prior to this work. We assumed the standard physical conditions for TMC-1 and assumed that these also hold for the envelope around Sgr B2(N).
    [Show full text]
  • Formation Mechanism of C60 Under Nonequilibrium and Irreversible
    This article was downloaded by: [Eiji Osawa] On: 14 May 2012, At: 15:10 Publisher: Taylor & Francis Informa Ltd Registered in England and Wales Registered Number: 1072954 Registered office: Mortimer House, 37-41 Mortimer Street, London W1T 3JH, UK Fullerenes, Nanotubes and Carbon Nanostructures Publication details, including instructions for authors and subscription information: http://www.tandfonline.com/loi/lfnn20 Formation Mechanism of C60 under Nonequilibrium and Irreversible Conditions — An Annotation a Eiji Ōsawa a NanoCarbon Research Institute, AREC, Shinshu University, Nagano, Japan Available online: 14 May 2012 To cite this article: Eiji Ōsawa (2012): Formation Mechanism of C60 under Nonequilibrium and Irreversible Conditions — An Annotation, Fullerenes, Nanotubes and Carbon Nanostructures, 20:4-7, 299-309 To link to this article: http://dx.doi.org/10.1080/1536383X.2012.655104 PLEASE SCROLL DOWN FOR ARTICLE Full terms and conditions of use: http://www.tandfonline.com/page/terms-and-conditions This article may be used for research, teaching, and private study purposes. Any substantial or systematic reproduction, redistribution, reselling, loan, sub-licensing, systematic supply, or distribution in any form to anyone is expressly forbidden. The publisher does not give any warranty express or implied or make any representation that the contents will be complete or accurate or up to date. The accuracy of any instructions, formulae, and drug doses should be independently verified with primary sources. The publisher shall not be liable for any loss, actions, claims, proceedings, demand, or costs or damages whatsoever or howsoever caused arising directly or indirectly in connection with or arising out of the use of this material.
    [Show full text]
  • Investigation of Au Sams Photoclick Derivatization by PM-IRRAS Wilson Luoa, Sydney M
    Investigation of Au SAMs Photoclick Derivatization by PM-IRRAS Wilson Luoa, Sydney M. Leggea, Johnny Luob,c, François Lagugné-Labarthet*a, and Mark S. Wor- kentin*a aDepartment of Chemistry and the Centre for Materials and Biomaterials Research, Western University, 1151 Rich- mond Street, London, ON, N6A 5B7, Canada. bDepartment of Biochemistry, Western University, London, Ontario N6A 5C1, Canada. cLawson Health Research Institute, London, Ontario N6C 2R5, Canada. ABSTRACT: In this work we present a clean one-step process for modifying headgroups of self-assembled monolayers (SAMs) on gold using photo-enabled click chemistry. A thiolated, cyclopropenone-caged strained alkyne precursor was first functionalized onto a flat gold substrate through self-assembly. Exposure of the cyclopropenone SAM to UV-A light initi- ated the efficient photochemical decarbonylation of the cyclopropenone moiety, revealing the strained alkyne capable of undergoing the interfacial strain-promoted alkyne-azide cycloaddition (SPAAC). Irradiated SAMs were derivatized with a series of model azides with varied hydrophobicity to demonstrate the generality of this chemical system for the modification and fine-tuning of the surface chemistry on gold substrates. SAMs were characterized at each step with polarization-mod- ulation infrared reflection-absorption spectroscopy (PM-IRRAS) to confirm successful functionalization and reactivity. Fur- thermore, to showcase the compatibility of this approach with biochemical applications, cyclopropenone SAMs were irra- diated and modified with azide-bearing cell adhesion peptides to promote human fibroblast cell adhesion, then imaged by live cell fluorescence microscopy. Thus, the “photoclick” methodology reported here represents an improved, versatile, catalyst-free protocol that allows for a high degree of control over the modification of material surfaces, with applicability in materials science as well as biochemistry.
    [Show full text]
  • A Study of the C3H2 Isomers and Isotopologues: first Interstellar Detection of HDCCC?
    A&A 586, A110 (2016) Astronomy DOI: 10.1051/0004-6361/201527460 & c ESO 2016 Astrophysics A study of the C3H2 isomers and isotopologues: first interstellar detection of HDCCC? S. Spezzano1;3, H. Gupta2;??, S. Brünken3, C. A. Gottlieb4, P. Caselli1, K. M. Menten5, H. S. P. Müller3, L. Bizzocchi1, P. Schilke3, M. C. McCarthy4, and S. Schlemmer3 1 Max-Planck-Institut für extraterrestrische Physik, Giessenbachstr. 1, 85748 Garching, Germany e-mail: [email protected] 2 California Institute of Technology, 770 S. Wilson Ave., M/C 100-22, Pasadena, CA 91125, USA 3 I. Physikalisches Institut, Universität zu Köln, Zülpicher Str. 77, 50937 Köln, Germany 4 Harvard-Smithsonian Center for Astrophysics, and School of Engineering & Applied Sciences, Harvard University, Cambridge, MA 02138, USA 5 Max-Planck Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany Received 28 September 2015 / Accepted 12 November 2015 ABSTRACT The partially deuterated linear isomer HDCCC of the ubiquitous cyclic carbene (c-C3H2) was observed in the starless cores TMC- 1C and L1544 at 96.9 GHz, and a confirming line was observed in TMC-1 at 19.38 GHz. To aid the identification in these narrow line sources, four centimetre-wave rotational transitions (two in the previously reported Ka = 0 ladder and two new ones in the Ka = 1 ladder) and 23 transitions in the millimetre band between 96 and 272 GHz were measured in high-resolution laboratory spectra. Ten spectroscopic constants in a standard asymmetric top Hamiltonian allow the main transitions of astronomical interest −1 in the Ka ≤ 3 rotational ladders to be calculated to within 0.1 km s in radial velocity up to 400 GHz.
    [Show full text]
  • Experimental and Density Functional Theory Studies of Some Novel Piperidine-Containing Acetylene Glycols
    General Papers ARKIVOC 2016 (iv) 86-99 Experimental and density functional theory studies of some novel piperidine-containing acetylene glycols Amina Mirsakiyeva,a, c, e* Darya Botkina,d, f Karim Elgammal,a, c Assel Ten,f Håkan W. Hugosson,a Anna Delin,a, b, c and Valentina Yue, f a Department of Materials and Nano Physics, School of Information and Communication Technology, KTH Royal Institute of Technology, Electrum 229, SE-16440 Kista, Sweden b Department of Physics and Astronomy, Materials Theory Division, Uppsala University, Box 516, SE-75120 Uppsala, Sweden c Swedish e-Science Research Center (SeRC), KTH Royal Institute of Technology, SE-10044 Stockholm, Sweden d Department of Production Engineering, School of Industrial Engineering and Management, KTH Royal Institute of Technology, Brinellvägen 68, 10044 Stockholm, Sweden e Kazakh-British Technical University, Department of Chemical Engineering, Tole bi 59, 050000 Almaty, Kazakhstan f Institute of Chemical Sciences, Walikhanov str. 106, 050010, Almaty city, Kazakhstan E-mail: [email protected] DOI: http://dx.doi.org/10.3998/ark.5550190.p009.452 Abstract Synthesis routes of novel piperidine-containing acetylenes are presented. The new molecules are expected to exhibit plant growth stimulation properties. In particular, the yield in a situation of drought is expected to increase. Our synthesis makes use of the Favorskii reaction between cyclohexanone/piperidone and triple-bond containing alcohols. The structures of the obtained molecules were determined using nuclear magnetic resonance (NMR). The electronic structure and geometries of the molecules were studied theoretically using first-principles calculations based on density functional theory. The calculated geometries agree very well with the experimentally determined ones, and also allow us to determine bond lengths, angles and charge distributions inside the molecules.
    [Show full text]
  • Design, Synthesis and Reactivity of Cyclopropenone
    DESIGN, SYNTHESIS AND REACTIVITY OF CYCLOPROPENONE- CONTAINING NINE MEMBERED CYCLIC ENEDIYNE AND ENYNE-ALLENE PRECURSORS AS PROTOTYPE PHOTOSWITCHABLE ANTITUMOR AGENTS by DINESH R. PANDITHAVIDANA (Under the Direction of Vladimir V. Popik) ABSTRACT The extreme cytotoxicity of natural enediyne antibiotics is attributed to the ability of the ( Z)-3-hexene-1,5-diyne (enediyne) and ( Z)-1,2,4-heptatrien-6-yne (enyne–allene) fragments incorporated into a 10- or 9-membered ring cyclic system to undergo cycloaromatization producing dDNA-damaging 1,4-diradicals. The rate of cyclization of enediynes to p-benzynes strongly depends on the distance between acetylenic termini, which in turn can be controlled by the ring size. Thus, 11-membered ring enediynes are stable, 10-membered ring analogs undergo slow cycloaromatization under ambient conditions or mild heating, 9- membered ring enediynes are virtually unknown and believed to undergo very fast spontaneous cyclization. Cyclic enyne-allenes have not been synthesized so far due to very facile Myers-Saito cyclization. We have developed thermally stable photo-precursors of 9-membered enediynes ( 2.22 , 2.26 ) and enyne-allene ( 2.44 ), in which one of the triple bonds is replaced by the cyclopropenone group. UV irradiation of 2.14 results in the efficient decarbonylation (Φ 254 = 0.34) and the formation of reactive enediyne 2.22. The latter undergoes clean cycloaromatization to 2,3-dihydro-1H- cyclopenta[b]naphthalen-1-ol ( 2.24 ) with a life-time of ca. 2 h in 2-propanol at 25 °C. The rate of this reaction depends linearly on the concentration of hydrogen donor and shows a primary kinetic isotope effect in 2-propanol-d8.
    [Show full text]
  • Gas Phase Synthesis of Interstellar Cumulenes. Mass Spectrometric and Theoretical Studies."
    rl ì 6. .B,1l thesis titled: "Gas Phase Synthesis of Interstellar Cumulenes. Mass Spectrometric and Theoretical studies." submitted for the Degree of Doctor of Philosophy (Ph.D') by Stephen J. Blanksby B.Sc.(Hons,) from the Department of ChemistrY The University of Adelaide Cì UCE April 1999 Preface Contents Title page (i) Contents (ii) Abstract (v) Statement of OriginalitY (vi) Acknowledgments (vii) List of Figures (ix) Phase" I Chapter 1. "The Generation and Characterisation of Ions in the Gas 1.I Abstract I 1.II Generating ions 2 t0 l.ru The Mass SPectrometer t2 1.IV Characterisation of Ions 1.V Fragmentation Behaviour 22 Chapter 2 "Theoretical Methods for the Determination of Structure and 26 Energetics" 26 2,7 Abstract 27 2.IT Molecular Orbital Theory JJ 2.TII Density Functional Theory 2.rv Calculation of Molecular Properties 34 2.V Unimolecular Reactions 35 Chapter 3 "Interstellar and Circumstellar Cumulenes. Mass Spectrometric and 38 Related Studies" 3.I Abstract 38 3.II Interstellar Cumulenes 39 3.III Generation of Interstellar Cumulenes by Mass Spectrometry 46 3.IV Summary 59 Preface Chapter 4 "Generation of Two Isomers of C5H from the Corresponding Anions' 61 ATheoreticallyMotivatedMassSpectrometricStudy.'. 6l 4.r Abstract 62 4.rl Introduction 66 4.III Results and Discussion 83 4.IV Conclusions 84 4.V Experimental Section 89 4.VI Appendices 92 Chapter 5 "Gas Phase Syntheses of Three Isomeric CSHZ Radical Anions and Their Elusive Neutrals. A Joint Experimental and Theoretical Study." 92 5.I Abstract 93 5.II Introduction 95 5.ru Results and Discussion t12 5.IV Conclusions 113 5.V Experimental Section ttl 5.VI Appendices t20 Chapter 6 "Gas Phase Syntheses of Three Isomeric ClHz Radical Anions and Their Elusive Neutrals.
    [Show full text]
  • On the Road to Carbene and Carbyne Complexes
    ON THE ROAD TO CARBENE AND CARBYNE COMPLEXES Nobel Lecture, 11 December 1973 by ERNST OTTO FISCHER Inorganic Chemistry Laboratory, Technical University, Munich, Federal Republic of Germany Translation from the German text INTRODUCTION In the year 1960, I had the honour of giving a talk at this university* about sandwich complexes on which we were working at that time. I think I do not have to repeat the results of those investigations today. I would like to talk instead about a field of research in which we have been intensely interested in recent years: namely, the field of carbene complexes and, more recently, carbyne complexes. If we substitute one of the hydrogen atoms in a hydrocarbon of the alkane type - for example, ethane - by a metal atom, which can of course bind many more ligands, we arrive at an organometallic compound in which the organic radical is bound to the metal atom by a σ-bond (Fig. la). The earliest compounds of this kind were prepared more than a hundred years ago; the first was cacodyl, prepared by R. Bunsen (1), and then zinc dialkyls were prepared by E. Frankland (2). Later V. Grignard was able to synthesise alkyl magnesium halides by treating magnesium with alkyl halides (3). Grignard was awarded the Nobel Prize in 1912 for this effort. We may further recall the organo-aluminium compounds (4) of K. Ziegler which form the basis for the low pressure polymerisation, for example of ethylene. Ziegler and G. Natta were together honoured with the Nobel Prize in 1963 for their work on organometallic compounds.
    [Show full text]
  • Transfer of Radiation Through Cyclopropenylidene and Ethylene Oxide
    A&A 402, 1–3 (2003) Astronomy DOI: 10.1051/0004-6361:20030229 & c ESO 2003 Astrophysics Transfer of radiation through cyclopropenylidene and ethylene oxide S. Chandra School of Physical Sciences, SRTM University, Nanded 431 606, India Received 29 June 1999 / Accepted 17 October 2002 Abstract. Cyclopropenylidene and ethylene oxide molecules are of astronomical importance as their observed lines, distributed throughout the observable microwave region, have a number of pairs having nearly equal frequencies, but different excitation energies and/or belonging to two different species of the molecule. Hence, these molecules may play important role in detecting physical conditions in cosmic objects. Therefore, in order to calculate intensities of the lines, we have investigated transfer of radiation through a cosmic object containing the molecule at a kinetic temperature of 10 K. Our results show that some lines of the molecule may be found in absorption against the cosmic 2.7 K background. Key words. ISM: molecules – molecular data – radiative transfer 1. Introduction The molecular data required as input for the present inves- tigation are: (i) Einstein A-coefficients for radiative transitions Cyclopropenylidene (C3H2), in astronomical objects, was iden- between the rotational energy levels accounted for, and (ii) rate tified by Thaddeus et al. (1985); they reported twelve emission coefficients for collisional transitions between the energy levels lines of the molecule, distributed throughout the observable mi- due to collisions with H2 molecules. crowave region. Ethylene oxide (C H O) has been observed by 2 4 Both cyclopropenylidene and ethylene oxide are b-type Dickens et al. (1997) in Sgr B2N; twelve emission lines of the asymmetric top molecules having a large electric dipole mo- molecule, distributed throughout the observable microwave re- ment of 3.325 D and 1.88 D, respectively, along their b-axis gion, have been reported by them.
    [Show full text]