Dimethyl Sulfoxide Oxidation of Primary Alcohols
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Dimethyl Sulfoxide MSDS
He a lt h 1 2 Fire 2 2 0 Re a c t iv it y 0 Pe rs o n a l Pro t e c t io n F Material Safety Data Sheet Dimethyl sulfoxide MSDS Section 1: Chemical Product and Company Identification Product Name: Dimethyl sulfoxide Contact Information: Catalog Codes: SLD3139, SLD1015 Sciencelab.com, Inc. 14025 Smith Rd. CAS#: 67-68-5 Houston, Texas 77396 RTECS: PV6210000 US Sales: 1-800-901-7247 International Sales: 1-281-441-4400 TSCA: TSCA 8(b) inventory: Dimethyl sulfoxide Order Online: ScienceLab.com CI#: Not applicable. CHEMTREC (24HR Emergency Telephone), call: Synonym: Methyl Sulfoxide; DMSO 1-800-424-9300 Chemical Name: Dimethyl Sulfoxide International CHEMTREC, call: 1-703-527-3887 Chemical Formula: (CH3)2SO For non-emergency assistance, call: 1-281-441-4400 Section 2: Composition and Information on Ingredients Composition: Name CAS # % by Weight Dimethyl sulfoxide 67-68-5 100 Toxicological Data on Ingredients: Dimethyl sulfoxide: ORAL (LD50): Acute: 14500 mg/kg [Rat]. 7920 mg/kg [Mouse]. DERMAL (LD50): Acute: 40000 mg/kg [Rat]. Section 3: Hazards Identification Potential Acute Health Effects: Slightly hazardous in case of inhalation (lung irritant). Slightly hazardous in case of skin contact (irritant, permeator), of eye contact (irritant), of ingestion, . Potential Chronic Health Effects: Slightly hazardous in case of skin contact (irritant, sensitizer, permeator), of ingestion. CARCINOGENIC EFFECTS: Not available. MUTAGENIC EFFECTS: Mutagenic for mammalian somatic cells. Mutagenic for bacteria and/or yeast. TERATOGENIC EFFECTS: Not available. DEVELOPMENTAL TOXICITY: Not available. The substance may be toxic to blood, kidneys, liver, mucous membranes, skin, eyes. -
Accurate Enthalpies of Formation of Astromolecules: Energy, Stability and Abundance
Accurate Enthalpies of Formation of Astromolecules: Energy, Stability and Abundance Emmanuel E. Etim and Elangannan Arunan* Inorganic and Physical Chemistry Department, Indian Institute of Science Bangalore, India-560012 *email: [email protected] ABSTRACT: Accurate enthalpies of formation are reported for known and potential astromolecules using high level ab initio quantum chemical calculations. A total of 130 molecules comprising of 31 isomeric groups and 24 cyanide/isocyanide pairs with atoms ranging from 3 to 12 have been considered. The results show an interesting, surprisingly not well explored, relationship between energy, stability and abundance (ESA) existing among these molecules. Among the isomeric species, isomers with lower enthalpies of formation are more easily observed in the interstellar medium compared to their counterparts with higher enthalpies of formation. Available data in literature confirm the high abundance of the most stable isomer over other isomers in the different groups considered. Potential for interstellar hydrogen bonding accounts for the few exceptions observed. Thus, in general, it suffices to say that the interstellar abundances of related species are directly proportional to their stabilities. The immediate consequences of this relationship in addressing some of the whys and wherefores among astromolecules and in predicting some possible candidates for future astronomical observations are discussed. Our comprehensive results on 130 molecules indicate that the available experimental enthalpy -
Polycarbodiimides As Classification-Free and Easy to Use Crosslinkers for Water-Based Coatings
White paper Polycarbodiimides as classification-free and easy to use crosslinkers for water-based coatings By Dr. A.J. Derksen, Stahl International bv, The Netherlands Polycarbodiimides (CDl) selectively react with carboxylic acid (–COOH) groups in polymer chains. This type of crosslinking reaction results in a classic 3D polymer-crosslinker network. Compared to polyisocyanates, polycarbodiimides are much less sensitive to presence of water and able to achieve long pot lives. Due to the high reactivity, curing with CDI type crosslinkers can be done under room temperature or typical oven conditions used for drying of applied coatings. In addition to standard CDI crosslinker chemistry, on offer is also a range of dual reactivity CDI crosslinkers. A second type of reactive groups is attached to the polycarbodiimide in this range. Upon curing, this crosslinker not only reacts with the –COOH groups in the polymer chains, but also two of the reactive groups attached to the separate CDI molecules can couple to form an even denser network structure. Building further on the success of these polycarbodiimide crosslinkers, VOC-free polycarbodiimides, in aqueous delivery form, were introduced, which give extreme long pot lives. 1. Introduction when dealing with flexible substrates. A high level of crosslinking Crosslinking is widely practiced in nearly all the coating may be acceptable for hard coatings on rigid substrates, but industries in order to improve the performance of the coating. low levels may be best for soft coatings on extensible, flexible These improvements include wear, abrasion and chemical substrates such as rubber and leather. An important crosslinking resistances and toughness1. The improved performance originates system for aqueous resins involves the use of water-dispersible from the formation of a continuous three-dimensional network, oligomeric polyisocyanates. -
Origins of Life: Transition from Geochemistry to Biogeochemistry
December 2016 Volume 12, Number 6 ISSN 1811-5209 Origins of Life: Transition from Geochemistry to Biogeochemistry NITA SAHAI and HUSSEIN KADDOUR, Guest Editors Transition from Geochemistry to Biogeochemistry Staging Life: Warm Seltzer Ocean Incubating Life: Prebiotic Sources Foundation Stones to Life Prebiotic Metal-Organic Catalysts Protometabolism and Early Protocells pub_elements_oct16_1300&icpms_Mise en page 1 13-Sep-16 3:39 PM Page 1 Reproducibility High Resolution igh spatial H Resolution High mass The New Generation Ion Microprobe for Path-breaking Advances in Geoscience U-Pb dating in 91500 zircon, RF-plasma O- source Addressing the growing demand for small scale, high resolution, in situ isotopic measurements at high precision and productivity, CAMECA introduces the IMS 1300-HR³, successor of the internationally acclaimed IMS 1280-HR, and KLEORA which is derived from the IMS 1300-HR³ and is fully optimized for advanced U-Th-Pb mineral dating. • New high brightness RF-plasma ion source greatly improving spatial resolution, reproducibility and throughput • New automated sample loading system with motorized sample height adjustment, significantly increasing analysis precision, ease-of-use and productivity • New UV-light microscope for enhanced optical image resolution (developed by University of Wisconsin, USA) ... and more! Visit www.cameca.com or email [email protected] to request IMS 1300-HR³ and KLEORA product brochures. Laser-Ablation ICP-MS ~ now with CAMECA ~ The Attom ES provides speed and sensitivity optimized for the most demanding LA-ICP-MS applications. Corr. Pb 207-206 - U (238) Recent advances in laser ablation technology have improved signal 2SE error per sample - Pb (206) Combined samples 0.076121 +/- 0.002345 - Pb (207) to background ratios and washout times. -
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). -
A Flexible All-Atom Model of Dimethyl Sulfoxide for Molecular Dynamics Simulations
1074 J. Phys. Chem. A 2002, 106, 1074-1080 A Flexible All-Atom Model of Dimethyl Sulfoxide for Molecular Dynamics Simulations Matthew L. Strader and Scott E. Feller* Department of Chemistry, Wabash College, CrawfordsVille, Indiana 47933 ReceiVed: October 1, 2001 An all-atom, flexible dimethyl sulfoxide model has been created for molecular dynamics simulations. The new model was tested against experiment for an array of thermodynamic, structural, and dynamic properties. Interactions with water were compared with previous simulations and experimental studies, and the unusual changes exhibited by dimethyl sulfoxide/water mixtures, such as the enhanced structure of the solution, were reproduced by the new model. Particular attention was given to the design of the electrostatic component of the force field and to providing compatibility with the CHARMM parameter sets for biomolecules. Introduction mixtures,14,17,18 and its interaction with a phospholipid bi- Theoretical methods for the investigation of biological layer.19,20 Simulations published to date have utilized a rigid, molecules have become commonplace in biochemistry and united-atom model where each methyl group is represented by biophysics.1 These approaches provide detailed atomic models a single atomic center and all bond lengths and angles are fixed of biological systems, from which structure-function relation- at their equilibrium values. Another feature common to most ships can be elucidated. Methods based on empirical force fields, of these models is the use of the same charge distribution, such as molecular dynamics (MD) simulations, allow for namely that obtained by Rao and Singh from a Hartree-Fock calculations on relatively large systems, e.g., complete biomol- 6-31G* ab initio quantum mechanical calculation.21 ecules or assemblies of biomolecules in their aqueous environ- Recent advances in computer hardware now allow a flexible, ment. -
Hydroxyacetonitrile (HOCH2CN) As a Precursor for Formylcyanide (CHOCN), Ketenimine (CH2CNH), and Cyanogen (NCCN) in Astrophysical Conditions
A&A 549, A93 (2013) Astronomy DOI: 10.1051/0004-6361/201219779 & c ESO 2013 Astrophysics Hydroxyacetonitrile (HOCH2CN) as a precursor for formylcyanide (CHOCN), ketenimine (CH2CNH), and cyanogen (NCCN) in astrophysical conditions G. Danger1, F. Duvernay1, P. Theulé1, F. Borget1, J.-C. Guillemin2, and T. Chiavassa1 1 Aix-Marseille Univ, CNRS, PIIM UMR 7345, 13397 Marseille, France e-mail: [email protected] 2 Institut des Sciences Chimiques de Rennes, École Nationale Supérieure de Chimie de Rennes, CNRS, UMR 6226, Avenue du Général Leclerc, CS 50837, 35708 Rennes Cedex 7, France Received 8 June 2012 / Accepted 19 November 2012 ABSTRACT Context. The reactivity in astrophysical environments can be investigated in the laboratory through experimental simulations, which provide understanding of the formation of specific molecules detected in the solid phase or in the gas phase of these environments. In this context, the most complex molecules are generally suggested to form at the surface of interstellar grains and to be released into the gas phase through thermal or non-thermal desorption, where they can be detected through rotational spectroscopy. Here, we focus our experiments on the photochemistry of hydroxyacetonitrile (HOCH2CN), whose formation has been shown to compete with aminomethanol (NH2CH2OH), a glycine precursor, through the Strecker synthesis. Aims. We present the first experimental investigation of the ultraviolet (UV) photochemistry of hydroxyacetonitrile (HOCH2CN) as a pure solid or diluted in water ice. Methods. We used Fourier transform infrared (FT-IR) spectroscopy to characterize photoproducts of hydroxyacetonitrile (HOCH2CN) and to determine the different photodegradation pathways of this compound. To improve the photoproduct identifications, irradiations of hydroxyacetonitrile 14N and 15N isotopologues were performed, coupled with theoretical calculations. -
The Prebiotic Molecular Inventory of Serpens SMM1
Astronomy & Astrophysics manuscript no. SMM1_C2H3NO_isomers ©ESO 2021 January 1, 2021 The prebiotic molecular inventory of Serpens SMM1 I. An investigation of the isomers CH3NCO and HOCH2CN N.F.W. Ligterink1, A. Ahmadi2, A. Coutens3, Ł. Tychoniec2 H. Calcutt4; 5, E.F. van Dishoeck2; 6, H. Linnartz7, J.K. Jørgensen8, R.T. Garrod9, and J. Bouwman7 1 Physics Institute, University of Bern, Sidlerstrasse 5, 3012 Bern, Switzerland e-mail: [email protected] 2 Leiden Observatory, Leiden University, PO Box 9513, 2300 RA Leiden, The Netherlands 3 Laboratoire d’Astrophysique de Bordeaux, Univ. Bordeaux, CNRS, B18N, allée Geoffroy Saint-Hilaire, 33615 Pessac, France 4 Department of Space, Earth and Environment, Chalmers University of Technology, 41296, Gothenburg, Sweden 5 Institute of Astronomy, Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University, Grudziadzka 5, 87-100 Torun, Poland 6 Max-Planck Institut für Extraterrestrische Physik (MPE), Giessenbachstr. 1, 85748 Garching, Germany 7 Laboratory for Astrophysics, Leiden Observatory, Leiden University, PO Box 9513, 2300 RA Leiden, The Netherlands 8 Centre for Star and Planet Formation, Niels Bohr Institute & Natural History Museum of Denmark, University of Copenhagen, Øster Voldgade 5–7, 1350 Copenhagen K., Denmark 9 Departments of Chemistry and Astronomy, University of Virginia, Charlottesville, VA 22904, USA Received October 8, 2020; accepted December 22, 2020 ABSTRACT Aims. Methyl isocyanate (CH3NCO) and glycolonitrile (HOCH2CN) are isomers and prebiotic molecules that are involved in the formation of peptide structures and the nucleobase adenine, respectively. These two species are investigated to study the interstellar chemistry of cyanides (CN) and isocyanates (NCO) and to gain insight into the reservoir of interstellar prebiotic molecules. -
Photochemical Generation of Carbenes and Ketenes from Phenanthrene-Based Precursors Part I: Dimethylalkylidene Part II: Diphenylketene
Colby College Digital Commons @ Colby Honors Theses Student Research 2017 Photochemical Generation of Carbenes and Ketenes from Phenanthrene-based Precursors Part I: Dimethylalkylidene Part II: Diphenylketene Tarini S. Hardikar Student Tarini Hardikar Colby College Follow this and additional works at: https://digitalcommons.colby.edu/honorstheses Part of the Organic Chemistry Commons Colby College theses are protected by copyright. They may be viewed or downloaded from this site for the purposes of research and scholarship. Reproduction or distribution for commercial purposes is prohibited without written permission of the author. Recommended Citation Hardikar, Tarini S. and Hardikar, Tarini, "Photochemical Generation of Carbenes and Ketenes from Phenanthrene-based Precursors Part I: Dimethylalkylidene Part II: Diphenylketene" (2017). Honors Theses. Paper 948. https://digitalcommons.colby.edu/honorstheses/948 This Honors Thesis (Open Access) is brought to you for free and open access by the Student Research at Digital Commons @ Colby. It has been accepted for inclusion in Honors Theses by an authorized administrator of Digital Commons @ Colby. Photochemical Generation of Carbenes and Ketenes from Phenanthrene-based Precursors Part I: Dimethylalkylidene Part II: Diphenylketene TARINI HARDIKAR A Thesis Presented to the Department of Chemistry, Colby College, Waterville, ME In Partial Fulfillment of the Requirements for Graduation With Honors in Chemistry SUBMITTED MAY 2017 Photochemical Generation of Carbenes and Ketenes from Phenanthrene-based Precursors Part I: Dimethylalkylidene Part II: Diphenylketene TARINI HARDIKAR Approved: (Mentor: Dasan M. Thamattoor, Professor of Chemistry) (Reader: Rebecca R. Conry, Associate Professor of Chemistry) “NOW WE KNOW” - Dasan M. Thamattoor Vitae Tarini Shekhar Hardikar was born in Vadodara, Gujarat, India in 1996. She graduated from the S.N. -
The Development of the First Catalyzed Reaction of Ketenes and Imines: Catalytic, Asymmetric Synthesis of Â-Lactams Andrew E
Published on Web 00/00/0000 The Development of the First Catalyzed Reaction of Ketenes and Imines: Catalytic, Asymmetric Synthesis of â-Lactams Andrew E. Taggi, Ahmed M. Hafez, Harald Wack, Brandon Young, Dana Ferraris, and Thomas Lectka* Contribution from the Department of Chemistry, Johns Hopkins UniVersity, 3400 North Charles Street, Baltimore, Maryland 21218 Received February 5, 2002 Abstract: We report practical methodology for the catalytic, asymmetric synthesis of â-lactams resulting from the development of a catalyzed reaction of ketenes (or their derived zwitterionic enolates) and imines. The products of these asymmetric reactions can serve as precursors to a number of enzyme inhibitors and drug candidates as well as valuable synthetic intermediates. We present a detailed study of the mechanism of the â-lactam forming reaction with proton sponge as the stoichiometric base, including kinetics and isotopic labeling studies. Stereochemical models based on molecular mechanics (MM) calculations are also presented to account for the observed stereoregular sense of induction in our reactions and to provide a guidepost for the design of other catalyst systems. Introduction this structural motif a worthwhile goal for the synthetic organic 10 The clinical relevance of â-lactams continues to expand at a chemist, thus the synthesis of these nonantibiotic â-lactams surprising rate. Although their use as antibiotics is being will be the focus of this contribution. While considerable effort compromised to some extent by bacterial resistance pressures,1 has been put into synthetic methodology to construct the basic recently â-lactams (especially nonnatural ones) have achieved â-lactam skeleton, there have been few general methods many important nonantibiotic uses. -
Part 1 : Studies of the Synthesis of Bicyclo[2.2.0] Hexane And
PART 1. STUDIES OF THE SYNTHESIS OF B1CYCLO[2.2.0]HEXANE AND CERTAIN REACTIONS OF 3-BENZHYDRYLCYCLOPENTENE-4-CARBOXYL1C ACID PART 11. ATTEMPTED SYNTHESES OF BENZCYCL0BUTENE-3,4-D10NE AND BENZCYCLOBUTENE by ALBERT C. KOVELESKY B. S., Pennsylvania State University, 1958 A MASTER'S THESIS submitted in partial fulfillment of the requirements for the degree MASTER OF SCIENCE Department of Chemistry KANSAS STATE UNIVERSITY Manhattan, Kansas 1962 This work is dedicated to my parents, Mr, and Mrs, Albert J. Kovelesky, for their patience, encouragement and financial assistance which made this work possible. ii ACKNOV/LEDGEMENT The author wishes to express his sincere gratitude to Dr. R, N, McDonald, for his competent supervision and continued encouragement throughout this in- vestigation. The author also vdshes to express his thanks to the other members of the graduate faculty and to his graduate student colleagues for the many helpful discussions and suggestions. Special thanks are extended to Kansas State Iftiiversity and to the National Science Foundation for the financial aid that was received during this investi- gation. iii TABLE OF CONTENTS Page PART I: STUDIES OF THE SYNTHESIS OF BICYCLO [j.Z.oJ HEXANE AND CERTAIN REACTIONS OF 3-BENZHYDRYLCYCLOPENTENE-2»- CARBOXYLIC ACID INTRODUCTION 1 OBJECTIVES OF THIS INVESTIGATION 3 DISCUSSION OF EXPERIMENTAL RESULTS k Proposed Route to Bicyclo j_2.2.oJ hexane ... k Elimination Studies of 3-Benzhydrylcyclopentene-2t-carboxylic Acid. .•.•.•.«•*. .*.. 8 SUMI4ARY 12 EXPERIMENTAL 18 Cyclopentadiene 18 Ketene ....«..*• • 18 Bicyclo [3»2.0j hept-2-en-6-one 18 Bicyclo [_3. 2. o] hept-2-ene 19 Oxidation of Bicyclo j_3.2.oJ hept-2-ene 20 1. -
Ketenes 25/01/2014 Part 1
Baran Group Meeting Hai Dao Ketenes 25/01/2014 Part 1. Introduction Ph Ph n H Pr3N C A brief history Cl C Ph + nPr NHCl Ph O 3 1828: Synthesis of urea = the starting point of modern organic chemistry. O 1901: Wedekind's proposal for the formation of ketene equivalent (confirmed by Staudinger 1911) Wedekind's proposal (1901) 1902: Wolff rearrangement, Wolff, L. Liebigs Ann. Chem. 1902, 325, 129. 2 Wolff adopt a ketene structure in 1912. R 2 hν R R2 1905: First synthesis and characterization of a ketene: in an efford to synthesize radical 2, 1 ROH R C Staudinger has synthesized diphenylketene 3, Staudinger, H. et al., Chem. Ber. 1905, 1735. N2 1 RO CH or Δ C R C R1 1907-8: synthesis and dicussion about structure of the parent ketene, Wilsmore, O O J. Am. Chem. Soc. 1907, 1938; Wilsmore and Stewart Chem. Ber. 1908, 1025; Staudinger and Wolff rearrangement (1902) O Klever Chem. Ber. 1908, 1516. Ph Ph Cl Zn Ph O hot Pt wire Zn Br Cl Cl CH CH2 Ph C C vs. C Br C Ph Ph HO O O O O O O O 1 3 (isolated) 2 Wilsmore's synthesis and proposal (1907-8) Staudinger's synthesis and proposal (1908) wanted to make Staudinger's discovery (1905) Latest books: ketene (Tidwell, 1995), ketene II (Tidwell, 2006), Science of Synthesis, Vol. 23 (2006); Latest review: new direactions in ketene chemistry: the land of opportunity (Tidwell et al., Eur. J. Org. Chem. 2012, 1081). Search for ketenes, Google gave 406,000 (vs.