CHEM 344 – Molecular Modeling
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Transport of Dangerous Goods
ST/SG/AC.10/1/Rev.16 (Vol.I) Recommendations on the TRANSPORT OF DANGEROUS GOODS Model Regulations Volume I Sixteenth revised edition UNITED NATIONS New York and Geneva, 2009 NOTE The designations employed and the presentation of the material in this publication do not imply the expression of any opinion whatsoever on the part of the Secretariat of the United Nations concerning the legal status of any country, territory, city or area, or of its authorities, or concerning the delimitation of its frontiers or boundaries. ST/SG/AC.10/1/Rev.16 (Vol.I) Copyright © United Nations, 2009 All rights reserved. No part of this publication may, for sales purposes, be reproduced, stored in a retrieval system or transmitted in any form or by any means, electronic, electrostatic, magnetic tape, mechanical, photocopying or otherwise, without prior permission in writing from the United Nations. UNITED NATIONS Sales No. E.09.VIII.2 ISBN 978-92-1-139136-7 (complete set of two volumes) ISSN 1014-5753 Volumes I and II not to be sold separately FOREWORD The Recommendations on the Transport of Dangerous Goods are addressed to governments and to the international organizations concerned with safety in the transport of dangerous goods. The first version, prepared by the United Nations Economic and Social Council's Committee of Experts on the Transport of Dangerous Goods, was published in 1956 (ST/ECA/43-E/CN.2/170). In response to developments in technology and the changing needs of users, they have been regularly amended and updated at succeeding sessions of the Committee of Experts pursuant to Resolution 645 G (XXIII) of 26 April 1957 of the Economic and Social Council and subsequent resolutions. -
Resonance, and Formal Charge
3.091: Introduction to Solid State Chemistry Maddie Sutula, Fall 2018 Recitation 8 1 Resonance Often, there are many ways that electrons can be arranged around a molecule. The existence of multiple electronic configurations that are stable leads to resonance, which describes the delocalization of electrons in covalently bonded molecules. To be considered resonance structures, molecules must meet the following criteria: 1. Atoms must be in the same orientation relative to each other 2. All resonance structures must have the same number of valence electrons 3. The octet rule must be satisfied, with a few exceptions: - Not followed by some elements in periods three and higher, including Cl, Br, I, P, Si − - Sulfur can have up to 12 e − - Boron can have 6 e 4. Formal charge should be on the most electronegative atoms 2− Example: Draw resonance structures for ozone (O3) and CO3 . Ozone consists of three oxygen atoms, for a total of 18 valence electrons. These can be equivalently dis- tributed in two ways: 2− CO3 consists of a central carbon atom which brings 4 valence electrons, and four oxygen atoms that each bring 6 electrons, and two additional electrons that yield the additional 2− charge. The resonance structures can be represented as follows: These equivalent structures can be combined into one compact picture (shown above on the right) that is an average of the possible structures. All of the resonance structures are equally likely, as they equivalently satisfy the guidelines for stable Lewis structures. 1 3.091: Introduction to Solid State Chemistry Maddie Sutula, Fall 2018 Recitation 8 2 Formal charge (again) 2− In the CO3 example above, the formal charge on each atom is shown in circles. -
Asian Journal of Chemistry Asian Journal
Asian Journal of Chemistry; Vol. 28, No. 3 (2016), 555-561 ASIAN JOURNAL OF CHEMISTRY http://dx.doi.org/10.14233/ajchem.2016.19405 Chemical Evolution of Aminoacetonitrile to Glycine under Discharge onto Primitive Hydrosphere: Simulation Experiments Using Glow Discharge T. MUNEGUMI Department of Science Education, Naruto University of Education, Naruto, Tokushima 772-8502, Japan Corresponding author: Fax: +81 88 6876022; Tel: +81 88 6876418; E-mail: [email protected] Received: 15 June 2015; Accepted: 31 July 2015; Published online: 5 December 2015; AJC-17650 Aminoacetonitrile is an important precursor of abiotic amino acids, as shown in the mechanism that was developed to explain the results of the Miller-type spark-discharge experiment. In present experimental setup, a spark discharge is generated in a simulated reducing atmosphere to yield hydrogen cyanide, aldehyde and ammonia; in a second step, a solution-phase reaction proceeds via aminoacetonitrile to give amino acids. However, when the same experiment is carried out in a non-reducing atmosphere, the yield of amino acids is very low. Contact glow discharge electrolysis onto the aqueous phase, which simulates an energy source for chemical evolution, converted aminoacetonitrile via glycinamide to glycine. The mechanism of glycinamide formation was explained by considering the addition of hydrogen and hydroxyl radicals to the C-N triple bond and subsequent transformation into the amide, which was then oxidized to the amino acid. This research suggests that amino acid amides and amino acids can be obtained through oxidation-reduction with H and OH radicals in the primitive hydrosphere whether under reducing or non-reducing conditions. -
The Reaction of Aminonitriles with Aminothiols: a Way to Thiol-Containing Peptides and Nitrogen Heterocycles in the Primitive Earth Ocean
life Article The Reaction of Aminonitriles with Aminothiols: A Way to Thiol-Containing Peptides and Nitrogen Heterocycles in the Primitive Earth Ocean Ibrahim Shalayel , Seydou Coulibaly, Kieu Dung Ly, Anne Milet and Yannick Vallée * Univ. Grenoble Alpes, CNRS, Département de Chimie Moléculaire, Campus, F-38058 Grenoble, France; [email protected] (I.S.); [email protected] (S.C.); [email protected] (K.D.L.); [email protected] (A.M.) * Correspondence: [email protected] Received: 28 September 2018; Accepted: 18 October 2018; Published: 19 October 2018 Abstract: The Strecker reaction of aldehydes with ammonia and hydrogen cyanide first leads to α-aminonitriles, which are then hydrolyzed to α-amino acids. However, before reacting with water, these aminonitriles can be trapped by aminothiols, such as cysteine or homocysteine, to give 5- or 6-membered ring heterocycles, which in turn are hydrolyzed to dipeptides. We propose that this two-step process enabled the formation of thiol-containing dipeptides in the primitive ocean. These small peptides are able to promote the formation of other peptide bonds and of heterocyclic molecules. Theoretical calculations support our experimental results. They predict that α-aminonitriles should be more reactive than other nitriles, and that imidazoles should be formed from transiently formed amidinonitriles. Overall, this set of reactions delineates a possible early stage of the development of organic chemistry, hence of life, on Earth dominated by nitriles and thiol-rich peptides (TRP). Keywords: origin of life; prebiotic chemistry; thiol-rich peptides; cysteine; aminonitriles; imidazoles 1. Introduction In ribosomes, peptide bonds are formed by the reaction of the amine group of an amino acid with an ester function. -
Constrained Density Functional Theory
Constrained Density Functional Theory The MIT Faculty has made this article openly available. Please share how this access benefits you. Your story matters. Citation Kaduk, Benjamin, Tim Kowalczyk, and Troy Van Voorhis. “Constrained Density Functional Theory.” Chemical Reviews 112.1 (2012): 321–370. © 2012 American Chemical Society As Published http://dx.doi.org/ 10.1021/cr200148b Publisher American Chemical Society (ACS) Version Author's final manuscript Citable link http://hdl.handle.net/1721.1/74564 Terms of Use Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. Constrained Density Functional Theory Benjamin Kaduk, Tim Kowalczyk and Troy Van Voorhis Department of Chemistry, Massachusetts Institute of Technology 77 Massachusetts Avenue, Cambridge MA 02139 May 2, 2011 Contents 1 Introduction 3 2 Theory 7 2.1 OriginalCDFTEquations ............................ 7 2.2 ConstrainedObservables . .. .. 9 2.3 ChoosingaConstraint .............................. 13 2.4 Implementation .................................. 18 2.5 Promolecules ................................... 24 2.6 Illustrations .................................... 28 2.6.1 MetalImpurities ............................. 28 2.6.2 Long-range Charge-Transfer Excited States . .... 32 2.7 FutureChallenges................................. 34 3 Application to Electron Transfer 36 3.1 Background:MarcusTheory. 36 3.2 DiabaticETStatesfromCDFT ......................... 39 3.2.1 Choosing Suitable Density Constraints for ET . 39 3.2.2 Illustrations ................................ 41 3.3 IncorporatingSolventEffects. .. 46 3.4 Molecular Dynamics and Free Energy Simulations . 49 3.5 RelatedandOngoingWork ........................... 54 4 Low-lying Spin States 57 4.1 TracingOutConstant-spinStates . .. 59 4.2 The Heisenberg Picture of Molecular Magnets . .. 63 4.3 Singlet-Triplet Gaps of Intermolecular CT States . -
Formal Charge Worksheet / Chem 314 Beauchamp
Formal Charge Worksheet / Chem 314 Beauchamp Formal Charge – a convention designed to indicate an excess or deficiency of electron density compared to an atom’s neutral allocation of electrons. Formal electrons in 1 electrons in Charge =Zeffective lone pairs 2 covalent bonds This number never changes for an atom and represents positive Total valence electrons allocated to an atom charge not cancelled assuming electrons are shared evenly in bonds. by core electrons. This number varies depending on the bonding arrangement. It is negative because electrons are negative. Rules of Formal Charge 1. When an atom’s total valence electron credit exactly matches its Zeff, there is no formal charge. 2. Each deficiency of an electron credit from an atom’s normal number of valence electrons produces an additional positive charge. 3. If the formal charge calculation shows excess electron credit over an atom’s normal number of valence electrons, a negative formal charge is added for each extra electron. 4. The total charge on an entire molecule, ion or free radical is the sum of all of the formal charges on the individual atoms. Write 3D structures for all resonance contributors. Rank them from best (=1) to last. Judge your structures on the basis of 1. maximum number of bonds / full octets, 2. minimize formal charge, 3, consistent formal charge based on electronegativity. Cations a. b. c. d. e. f. H COH 2 H2CNH2 (CH3)2COH (CH3)2CNHCH3 (CH3)2CCH2CH3 H2CCOH 2 resonance 2 resonance 2 resonance 2 resonance 2 resonance structures structures structures structures structures g. h. i. j. -
Temporal and Spacial Variation of the Organic Particles in the Proto-Solar
46th Lunar and Planetary Science Conference (2015) 2591.pdf TEMPORAL AND SPATIAL VARIATION OF THE ORGANIC PARTICLES IN THE PROTO-SOLAR DISK M. Numata1 and H. Nagahara1, 1Department of Earth and Planetary Science, the University of Tokyo Introduction: More than 80 distinct amino acids Model: We calculate evolution of a viscous disk are discovered in meteorites, which, in addition to their with special interests on the location of individual precursors, are suggested to be extraterrestrial origin particles-in order to know the chemical change of (e.g., [1-3]). Even the detection of glycine, the simplest organic materials. The disk evolution model and amino acid, has been claimed in samples from comet particle-tracking model by Ciesla [12, 13] were applied. 81P/Wild 2 returned by NASA’s Stardust spacecraft Disk temperature is determined by balancing vertical [4]. These discoveries suggest that interstellar energy flux assuming that all of the energy dissipation chemistry can produce such complex molecules. occurs at the midplane [14]. We use alpha-prescription Motivated by these studies, some observational search of Shakura & Sunyaev [15] for viscosity. for complex molecules in the interstellar medium The initial gas density is assumed to distribute as a reported to detect acetic acid [5], acetamide [6], self-similar solution [16] and particles containing aminoacetonitrile [7], and ethyl formate [8] in organic materials are released at each 10AU from 10A Sagittarius B2 molecular cloud. More recently, ALMA to 100AU at t = 0. Disk vertical temperature gradient is observation is expected to find more complexity of neglected. Particles are supposed to be small enough to such organic materials [9]. -
Diaminomaleonitrile
PREBIOLOGICAL PROTEIN SYNTHESIS BY CLIFFORD N. MATTHEWS AND ROBERT E. MOSER CENTRAL RESEARCH DEPARTMENT, MONSANTO COMPANY, ST. LOUIS, MISSOURI Communicated by Charles A. Thomas, July 18, 1966 A major concern of chemical evolution research1 4 is to find an answer to the question: How were proteins originally formed on Earth before the appearance of life? A widely held view stimulated by the speculations of Oparin,5 Haldane,6 Bernal,7 and Urey8 is that the formation of polypeptides occurred via two essential steps, a-amino acid synthesis initiated by the action of natural high-energy sources on the components of a reducing atmosphere, followed by polycondensations in the oceans or on land. The results of a dozen years of simulation experiments1-4 appear to support this view. Experiments in which high-energy radiations were applied to reduced mixtures of gases have yielded many of the 20 a-amino acids commonly found in proteins. The pioneering research of M\iller9 showed that glycine, alanine, aspartic acid, and glutamic acid were among the products obtained by passing electric discharges through a refluxing mixture of hydrogen, methane, ammonia, and water. Exten- sions of these studies by Abelson10 and others'-4 showed that a-amino acid synthesis could be effected by almost any source of high energy so long as the starting mix- ture contained water and was reducing. Since mechanism studies by Miller9 indicated that aldehydes and hydrogen cyanide were transient intermediates during the course of the reaction, it was concluded that the a-amino acids were formed by the well-known Strecker route involving hydrolysis of aminoacetonitriles arising from the interactions of aldehydes, hydrogen cyanide, and ammonia. -
Formal Charge and Oxidation Number
FORMAL CHARGE AND OXIDATION NUMBER Although the total number of valence electrons in a molecule is easily calculated, there is not aways a simple and unambiguous way of determining how many reside in a particular bond or as non-bonding pairs on a particular atom. For example, one can write valid Lewis octet structures for carbon monoxide showing either a double or triple bond between the two atoms, depending on how many nonbonding pairs are placed on each: C::O::: and :C:::O: (see Problem Example 3 below). The choice between structures such as these is usually easy to make on the principle that the more electronegative atom tends to surround itself with the greater number of electrons. In cases where the distinction between competing structures is not all that clear, an arbitrarily-calculated quantity known as the formal charge can often serve as a guide. The formal charge on an atom is the electric charge it would have if all bonding electrons were shared equally with its bonded neighbors. How to calculate the formal charge on an atom in a molecule The formal charge on an atom is calculated by the following formula: In which the core charge is the electric charge the atom would have if all its valence electrons were removed. In simple cases, the formal charge can be worked out visually directly from the Lewis structure, as is illustrated farther on. Problem Example 1 Find the formal charges of all the atoms in the sulfuric acid structure shown here. Solution: The atoms here are hydrogen, sulfur, and double- and single-bonded oxygens. -
Carbon Tetrachloride
CARBON TETRACHLORIDE Data were last reviewed in IARC (1979) and the compound was classified in IARC Monographs Supplement 7 (1987a). 1. Exposure Data 1.1 Chemical and physical data 1.1.1 Nomenclature Chem. Abstr. Serv. Reg. No.: 56-23-5 Chem. Abstr. Name: Tetrachloromethane IUPAC Systematic Name: Carbon tetrachloride Synonyms: Benzinoform; carbona 1.1.2 Structural and molecular formulae and relative molecular mass Cl Cl CCl Cl CCl4 Relative molecular mass: 153.82 1.1.3 Chemical and physical properties of the pure substance (a) Description: Colourless, clear, nonflammable, liquid with a characteristic odour (Budavari, 1996) (b) Boiling-point: 76.8°C (Lide, 1997) (c) Melting-point: –23°C (Lide, 1997) (d) Solubility: Very slightly soluble in water (0.05% by volume); miscible with benzene, chloroform, diethyl ether, carbon disulfide and ethanol (Budavari, 1996) (e) Vapour pressure: 12 kPa at 20°C; relative vapour density (air = 1), 5.3 at the boiling-point (American Conference of Governmental Industrial Hygienists, 1991) (f) Conversion factor: mg/m3 = 6.3 × ppm 1.2 Production and use Production in the United States in 1991 was reported to be approximately 143 thousand tonnes (United States International Trade Commission, 1993). Information –401– 402 IARC MONOGRAPHS VOLUME 71 available in 1995 indicated that carbon tetrachloride was produced in 24 countries (Che- mical Information Services, 1995). Carbon tetrachloride is used in the synthesis of chlorinated organic compounds, including chlorofluorocarbon refrigerants. It is also used as an agricultural fumigant and as a solvent in the production of semiconductors, in the processing of fats, oils and rubber and in laboratory applications (Lewis, 1993; Kauppinen et al., 1998). -
Aminoacetonitrile Characterization in Astrophysical-Like Conditions
A&A 541, A114 (2012) Astronomy DOI: 10.1051/0004-6361/201218949 & c ESO 2012 Astrophysics Aminoacetonitrile characterization in astrophysical-like conditions F. Borget, G. Danger, F. Duvernay, M. Chomat, V. Vinogradoff, P. Theulé, and T. Chiavassa Aix-Marseille Université et CNRS, Laboratoire de Physique des Interactions Ioniques et Moléculaires, UMR 7345, Centre de St-Jérôme, case 252, Avenue Escadrille Normandie-Niémen, 13397 Marseille Cedex 20, France e-mail: [email protected] Received 2 February 2012 / Accepted 23 March 2012 ABSTRACT Context. Aminoacetonitrile (AAN) has been detected in 2008 in the hot core SgrB2. This molecule is of particular interest because it is a central molecule in the Strecker synthesis of amino acids. This molecule can be formed from methanimine (CH2NH), ammonia (NH3) and hydrogen cyanide (HCN) in astrophysical icy conditions. Nevertheless, few studies exist about its infrared (IR) identifica- tion or its astrophysical characterization. Aims. We present in this study a characterization of the pure solid AAN and when it is diluted in water to study the influence of H2O on the main IR features of AAN. The reactivity with CO2 and its photoreactivity are also studied and the main products were characterized. Methods. Fourier transformed infrared (FTIR) spectroscopy of AAN molecular ice was performed in the 10–300 K temperature range. We used temperature-programmed desorption coupled with mass spectrometry detection techniques to evaluate the desorption energy value. The influence of water was studied by quantitative FTIR spectroscopy and the main reaction and photochemical products were identified by FTIR spectroscopy. Results. We determined that in our experimental conditions, the IR limit of AAN detection in the water ice is about 1 × 1016 molecule cm−2, which means that the AAN detection is almost impossible within the icy mantle of interstellar grains. -
Chemical Bonding
Chemical Bonding: Fundamental Concepts Resonance Structures and Formal Charge Electronegativity, Formal Charge and Resonance Page [1 of 3] In this lecture we’re going to pull together ideas about formal charge, resonance structures, electronegativity, and really make some predictions and some rationalizations about why molecules behave the way they do. And the first one I want to do is to go back and look at the cyanate ion. Cyanate is NCO. And in a previous lecture I talked about the fact that there were several different possible resonance structures that are all in equivalence, and that it was possible at least to figure out which one contributed the most and which one contributed the least based on formal charge. So here are the formal charge evaluations for this left-hand resonance structure. Nitrogen has a formal charge of zero. Carbon has a formal charge of zero. Oxygen has a formal charge of -1. For B, nitrogen is -1, carbon is zero, oxygen is zero. And for C, nitrogen is -2, carbon is zero, and oxygen is +1. Now, the rule said that formal charges of plus or minus 1 and zero are okay. In fact, zero is great. And plus or minus 2 and bigger, that’s just not going to work. Why? Because remember, formal charges reflect how the electrons are distributed relative to how they are distributed in the free atom. So how they’re distributed in a molecule versus how they’re distributed in the free atom. And in this case nitrogen has a lot more electrons than it would if were a free atom formally; in other words, an accounting method.