Mass Spectrometry Across the Sciences
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Type of Ionising Radiation Gamma Rays Versus Electro
MY9700883 A National Seminar on Application of Electron Accelerators, 4 August 1994 INTRODUCTION TO RADIATION CHEMISTRY OF POLYMER Khairul Zaman Hj. Mohd Dahlan Nuclear Energy Unit What is Radiation Chemistry? Radiation Chemistry is the study of the chemical effects of ionising radiation on matter. The ionising radiation flux in a radiation field may be expressed in terms of radiation intensity (i.e the roentgen). The roentgen is an exposure dose rather than absorbed dose. For radiation chemist, it is more important to know the absorbed dose i.e. the amount of energy deposited in the materials which is expressed in terms of Rad or Gray or in electron volts per gram. The radiation units and radiation power are shown in Table 1 and 2 respectively. Type of Ionising Radiation Gamma rays and electron beam are two commonly used ionising radiation in industrial process. Gamma rays, 1.17 and 1.33 MeV are emitted continuously from radioactive source such as Cobalt-60. The radioactive source is produced by bombarding Cobalt-59 with neutrons in a nuclear reactor or can be produced from burning fuel as fission products. Whereas, electrons are generated from an accelerator to produce a stream of electrons called electron beam. The energy of electrons depend on the type of machines and can vary from 200 keV to 10 MeV. Gamma Rays versus Electron Beam Gamma rays are electromagnetic radiation of very short wavelength about 0.01 A (0.001 nm) for a lMeV photon. It has a very high penetration power. Whereas, electrons are negatively charge particles which have limited penetration power. -
Mechanistic Studies of the Desorption Ionization
Mechanistic studies of the desorption ionization process in fast atom bombardment mass spectrometry by Jentaie Shiea A thesis submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy in Chemistry Montana State University © Copyright by Jentaie Shiea (1991) Abstract: The mechanisms involved in Desorption Ionization (DI) continue to be a very active area of research. The answer to the question of how involatile and very large molecules are transferred from the condensed phase to the gas phase has turned out to involve many different phenomena. The effect on Fast Atom Bombardment (FAB) mass spectra of the addition of acids to analyte bases has been quantitatively investigated. Generally, the pseudomolecular ion (M+H+) intensity increased with the addition of acid, however, decreases in ion intensity were also noted. For the practical use of FAB, it is important to clarify the reasons for this acid effect. By critical evaluation, a variety of different explanations were found. However, contrary to other studies, no unambiguous example was found in which the effect of "preformed ions" could adequately explain the observed results. The mechanistic implications of these findings are briefly discussed. The importance of surface activity in FAB has been pointed out by many researchers. A systematic study was conducted, involving the addition of negatively charged surfactants to samples containing small organic and inorganic cations. An enhancement of the positive ion spectra of these analytes was observed. The study of mass transport processes of two surfactants was performed by varying the analyte concentration and matrix temperature in FAB. The study of the desorption process in SIMS by varying the viscosity of the matrix solutions shows that such studies may help to bridge the mechanisms in solid and liquid SIMS and, in the process, increase our understanding of both techniques. -
Biomolecules
biomolecules Communication MBLinhibitors.com, a Website Resource Offering Information and Expertise for the Continued Development of Metallo-β-Lactamase Inhibitors Zishuo Cheng 1, Caitlyn A. Thomas 1, Adam R. Joyner 2, Robert L. Kimble 1, Aidan M. Sturgill 1 , Nhu-Y Tran 1, Maya R. Vulcan 1, Spencer A. Klinsky 1, Diego J. Orea 1, Cody R. Platt 2, Fanpu Cao 2, Bo Li 2, Qilin Yang 2, Cole J. Yurkiewicz 1, Walter Fast 3 and Michael W. Crowder 1,* 1 Department of Chemistry and Biochemistry, Miami University, Oxford, OH 45056, USA; [email protected] (Z.C.); [email protected] (C.A.T.); [email protected] (R.L.K.); [email protected] (A.M.S.); [email protected] (N.-Y.T.); [email protected] (M.R.V.); [email protected] (S.A.K.); [email protected] (D.J.O.); [email protected] (C.J.Y.) 2 Department of Computer Science and Software Engineering, Miami University, Oxford, OH 45056, USA; [email protected] (A.R.J.); [email protected] (C.R.P.); [email protected] (F.C.); [email protected] (B.L.); [email protected] (Q.Y.) 3 Division of Chemical Biology and Medicinal Chemistry, College of Pharmacy and the LaMontagne Center for Infectious Disease, University of Texas, Austin, TX 78712, USA; [email protected] * Correspondence: [email protected]; Tel.: +1-513-529-2813 Received: 17 February 2020; Accepted: 12 March 2020; Published: 16 March 2020 Abstract: In an effort to facilitate the discovery of new, improved inhibitors of the metallo-β-lactamases (MBLs), a new, interactive website called MBLinhibitors.com was developed. -
To Undergraduate Studies in Chemistry, Chemical Engineering, and Chemical Biology College of Chemistry, University of California, Berkeley, 2011-12
Guide to Undergraduate Studies in Chemistry, Chemical Engineering, and -2012 Chemical Biology College of Chemistry 2011 University of California, Berkeley Academic Calendar 2011-12 Fall Semester 2011 Tele-BEARS Begins April 11 Monday Fee Payment Due August 15 Monday Fall Semester Begins August 18 Thursday Welcome Events August 22-26 Monday-Friday Instruction Begins August 25 Thursday Labor Day Holiday September 5 Monday Veterans Day Holiday November 11 Friday Thanksgiving Holiday November 24-25 Thursday-Friday Formal Classes End December 2 Friday Reading/Review/Recitation Week December 5-9 Monday-Friday Final Examinations December 12-16 Monday-Friday Fall Semester Ends December 16 Friday Winter Holiday December 26-27 Monday-Tuesday New Year’s Holiday December 29-30 Thursday-Friday Spring Semester 2012 Tele-BEARS Begins October 17, 2011 Monday Spring Semester Begins January 10 Tuesday Fee Payment Due January 15 Sunday Martin Luther King Jr. Holiday January 16 Monday Instruction Begins January 17 Tuesday Presidents’ Day Holiday February 20 Monday Spring Recess March 26-30 Monday-Friday César Chávez Holiday March 30 Friday Cal Day To Be Determined Formal Classes End April 27 Friday Reading/Review/Recitation Week April 30-May 4 Monday-Friday Final Examinations May 7-11 Monday-Friday Spring Semester Ends May 11 Friday Summer Sessions 2012 Tele-BEARS Begins February 6 Monday First Six-Week Session May 21-June 29 Monday-Friday Memorial Day Holiday May 28 Monday Ten-Week Session June 4-August 10 Monday-Friday Eight-Week Session June 18-August -
Methods of Ion Generation
Chem. Rev. 2001, 101, 361−375 361 Methods of Ion Generation Marvin L. Vestal PE Biosystems, Framingham, Massachusetts 01701 Received May 24, 2000 Contents I. Introduction 361 II. Atomic Ions 362 A. Thermal Ionization 362 B. Spark Source 362 C. Plasma Sources 362 D. Glow Discharge 362 E. Inductively Coupled Plasma (ICP) 363 III. Molecular Ions from Volatile Samples. 364 A. Electron Ionization (EI) 364 B. Chemical Ionization (CI) 365 C. Photoionization (PI) 367 D. Field Ionization (FI) 367 IV. Molecular Ions from Nonvolatile Samples 367 Marvin L. Vestal received his B.S. and M.S. degrees, 1958 and 1960, A. Spray Techniques 367 respectively, in Engineering Sciences from Purdue Univesity, Layfayette, IN. In 1975 he received his Ph.D. degree in Chemical Physics from the B. Electrospray 367 University of Utah, Salt Lake City. From 1958 to 1960 he was a Scientist C. Desorption from Surfaces 369 at Johnston Laboratories, Inc., in Layfayette, IN. From 1960 to 1967 he D. High-Energy Particle Impact 369 became Senior Scientist at Johnston Laboratories, Inc., in Baltimore, MD. E. Low-Energy Particle Impact 370 From 1960 to 1962 he was a Graduate Student in the Department of Physics at John Hopkins University. From 1967 to 1970 he was Vice F. Low-Energy Impact with Liquid Surfaces 371 President at Scientific Research Instruments, Corp. in Baltimore, MD. From G. Flow FAB 371 1970 to 1975 he was a Graduate Student and Research Instructor at the H. Laser Ionization−MALDI 371 University of Utah, Salt Lake City. From 1976 to 1981 he became I. -
Protein Identification Strategies in MALDI Imaging Mass Spectrometry
Available online at www.sciencedirect.com ScienceDirect Protein identification strategies in MALDI imaging mass spectrometry: a brief review 1,2 1,2,3 Daniel J Ryan , Jeffrey M Spraggins and 1,2,3,4,5 Richard M Caprioli Matrix assisted laser desorption/ionization (MALDI) imaging specimens [1,2 ,3,4]. MALDI IMS allows for the label- mass spectrometry (IMS) is a powerful technology used to free, multiplex analysis of thousands of analytes across a investigate the spatial distributions of thousands of molecules samples surface yielding 2-dimensional molecular maps throughout a tissue section from a single experiment. As that elucidate both the localization and relative abundance proteins represent an important group of functional molecules of endogenous species. The technology has been used to in tissue and cells, the imaging of proteins has been an study awiderangeofanalyteclasses,includingmetabolites, important point of focus in the development of IMS drugs, lipids, peptides, and proteins [5,6 ,7 ,8]. The imag- technologies and methods. Protein identification is crucial for ing of proteins has garnered particular attention due to the the biological contextualization of molecular imaging data. role the proteins play in cellular processes [9], and because However, gas-phase fragmentation efficiency of MALDI MALDI IMS allows for the visualization of a protein and its generated proteins presents significant challenges, making various proteoforms (i.e. varying post-translational modifi- protein identification directly from tissue difficult. This review cations) in a single imaging experiment [10,11 ,12]. As highlights methods and technologies specifically related to highlighted in Figure 1, MALDI IMS is performed by first protein identification that have been developed to overcome coating a tissue section with a MALDI matrix, which assists these challenges in MALDI IMS experiments. -
Hydrocarbon Radiation Chemistry in Ices of Cometary Relevance
ICARUS 126, 233±235 (1997) ARTICLE NO. IS975678 NOTE Hydrocarbon Radiation Chemistry in Ices of Cometary Relevance R. L. HUDSON Department of Chemistry, Eckerd College, St. Petersburg, Florida 33733 E-mail: [email protected] AND M. H. MOORE Code 691, Astrochemistry Branch, NASA/Goddard Space Flight Center, Greenbelt, Maryland 20771 Received August 19, 1996; revised January 3, 1997 emphasis on the chemistry of hydrocarbons in a H2O-dominated mixture Recent discoveries of acetylene, methane, and ethane in at p15 K. Details concerning our laboratory techniques are already in print Comet Hyakutake, C/1996 B2, have led us to investigate these (Moore et al. 1996, Hudson and Moore 1995, and references therein). and other hydrocarbons in irradiated ices of cometary rele- Brie¯y, we condensed H2O-rich gas-phase mixtures onto a cold ®nger at vance. Laboratory experiments showed that chemical reactions, p15 K in a vacuum chamber (P p 1028 Torr), after which an infrared particularly those involving H atoms, in¯uence the C2H6 :CH4 (IR) spectrum of the solid mixture was recorded. Next, the icy sample 1 ratio in H2O 1 hydrocarbon mixtures. 1997 Academic Press was irradiated with a 0.8 MeV proton (p ) beam from a Van de Graaff accelerator. IR spectra were recorded before and after each irradiation, as well as after various thermal annealings. Molecular abundances were determined by established procedures in which a laser interference system Three new cometary molecules, acetylene (C2H2), methane (CH4), and was used to measure ice thickness in a sample of known composition. ethane (C2H6), have been discovered recently in Comet Hyakutake, C/1996 B2. -
Suppression of Matrix Ions by N-Phosphorylation Labeling Using
Electronic Supplementary Material (ESI) for Chemical Communications This journal is © The Royal Society of Chemistry 2012 Supporting Information Suppression of Matrix Ions by N-Phosphorylation Labeling Using Matrix-Assisted Laser Desorption/Ionization Time-of-Flight Mass Spectrometry Xiang Gao,a, b Zhi Tang,a Minghua Lu,a Hongxia Liu,b Yuyang Jiang,b Yufen Zhao c and Zongwei Cai*, a, b a Department of Chemistry, Hong Kong Baptist University, Kowloon Tong, Hong Kong, SAR, China b The Key Laboratory for Cancer Metabolomics of Shenzhen, Graduate School at Shenzhen, Tsinghua University, Shenzhen, 518055, China c Department of Chemistry and The Key Laboratory for Chemical Biology of Fujian Province, College of Chemistry and Chemical Engineering, Xiamen University, Xiamen, 361005, P. R. China * Corresponding author. E-mail: [email protected]. 1 Electronic Supplementary Material (ESI) for Chemical Communications This journal is © The Royal Society of Chemistry 2012 EXPERIMENTAL SECTION Materials and Reagents. L-Amino acids, D-(+)-glucosamine hydrochloride, agmatine sulfate salt, formic acid, magnesium sulfate (MgSO4), trifluoroacetic acid (TFA), triethylamine (TEA), tetrachloromethane (CCl4), -cyano-4-hydroxycinnamic acid (CHCA), and 2, 5-dihydroxybenzoic acid (DHB) were purchased from Sigma (St. Louis, MO, USA) and used without further purification. Diisopropyl phosphate (DIPP-H) and anhydrous ethanol were obtained from Alfa Aesar Chemical Ltd. (Tianjin, China). Peptide calibration standard used for calibration of MALDI-MS instrument was obtained from Bruker Daltonics (Bruker, Germany). Sep-Pak Vac C18 cartridges were purchased from Waters (MA, USA). Porous graphitic carbon (PGC) cartridges were obtained from Alltech Associates, Inc. (Deerfield, IL). Graphene nonopowder (8 nm flakes) was obtained from Graphene Laboratories Inc. -
Radiation Chemistry of Liquid Systems
Chapter 4 RADIATION CHEMISTRY OF LIQUID SYSTEMS Krzysztof Bobrowski Institute of Nuclear Chemistry and Technology, Dorodna 16, 03-195 Warszawa, Poland 1. INTRODUCTION The radiation chemistry of liquid systems illustrates a versatile use of high energy ionizing radiation [1-4]. Radiolysis, the initiation of reactions by high energy radiation, is a very valuable and powerful chemical tool for inducing and studying radical reactions in liquids. In many cases radiolysis offers a convenient and relatively easy way of initiating radical reactions in all phases (including liquid phase) that cannot be or can be performed with some limita- tions by chemical, electrochemical and photolytic methods. Radiolysis of most liquids produces solvated electrons and relatively simple free radicals, some of which can oxidize and/or reduce materials [5]. This chapter is divided into four main sections: “Introduction”, “Radiolysis of water”, “Radiolysis of or- ganic solvents”, and “Radiolysis of ionic liquids”. The fi rst section summa- rizes the mechanisms and features of radiation energy deposition along with a quantifi cation of chemical effects induced by radiation, and techniques used in radiation chemical studies. The second section focuses on radiation-induced radical reactions in water and aqueous solutions using low and high linear energy transfer (LET) irradiation at ambient and high temperatures, and high pressures. Relevant examples include radical reactions initiated by primary and secondary radicals from water radiolysis with a variety of compounds. The third section describes the most important features of radiolysis in organic liquids using common solvents for inducing and studying radical reactions. Relevant examples include radical reactions connected with the selective for- mation of radical cations, radical anions and excited states. -
Research Article Prebiotic Geochemical Automata at the Intersection of Radiolytic Chemistry, Physical Complexity, and Systems Biology
Hindawi Complexity Volume 2018, Article ID 9376183, 21 pages https://doi.org/10.1155/2018/9376183 Research Article Prebiotic Geochemical Automata at the Intersection of Radiolytic Chemistry, Physical Complexity, and Systems Biology Zachary R. Adam ,1,2 Albert C. Fahrenbach ,3 Betul Kacar ,2,3,4 and Masashi Aono 5 1 Department of Earth and Planetary Sciences, Harvard University, Cambridge, MA, USA 2Blue Marble Space Institute of Science, Seattle, WA, USA 3Earth-Life Science Institute, Tokyo Institute of Technology, Tokyo, Japan 4Department of Molecular and Cellular Biology and Department of Astronomy, University of Arizona, Tucson, AZ, USA 5Faculty of Environment and Information Studies, Keio University, Kanagawa, Japan Correspondence should be addressed to Zachary R. Adam; [email protected] Received 27 October 2017; Accepted 20 February 2018; Published 26 June 2018 Academic Editor: Roberto Natella Copyright © 2018 Zachary R. Adam et al. Tis is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. Te tractable history of life records a successive emergence of organisms composed of hierarchically organized cells and greater degrees of individuation. Te lowermost object level of this hierarchy is the cell, but it is unclear whether the organizational attributes of living systems extended backward through prebiotic stages of chemical evolution. If the systems biology attributes of the cell were indeed templated upon prebiotic synthetic relationships between subcellular objects, it is not obvious how to categorize object levels below the cell in ways that capture any hierarchies which may have preceded living systems. -
Radiation Chemistry Vs. Photochemistry Cosmic Synthesis
Radiation Chemistry vs. Photochemistry Cosmic Synthesis of Prebiotic Molecules Chris Arumainayagam Wellesley College, Massachusetts, USA First Evidence of molecules in space: Annie Jump Cannon (Wellesley College Class of 1884) Molecular Physics, 2015,113, 2159-2168 Five Mechanisms for Processing Interstellar Ices Shock Waves Arumainayagam et. al., Chemical Society Reviews 2019, 48, 8, 2267–2496. What is the difference between radiation chemistry and photochemistry? Radiation Chemistry Radiation chemistry is the “study of the chemical changes produced by the absorption of radiation of sufficiently high energy to produce ionization.” RADIATION CHEMISTRY INVOLVES IONIZATION. R.J. Woods, Basics of Radiation Chemistry, in: R.D.C. William J. Cooper, Kevin E. O'Shea Flux of Cosmic Rays Reaching Earth Formation of Secondary Electrons in Cosmic Ices and Dust Grains secondary electron cascade (0‐20 eV) thin (~100 ML) ice layers (10 K) cosmic ray 107‐1020 eV Importance of Low‐Energy Electrons Secondary Electron “Tail” Dissociation Cross-Section Dissociation Yield 1 MeV parcle → 100,000 low‐energy electrons DEA Resonances Ionization and Excitation C. Arumainayagam et al., Surface Science Reports 65 (2010) 1‒44. Electron‐induced Dissociation Mechanisms Electron Impact A* + B Excitation * – Dipolar + – AB + e Dissociation A + B not possible > 3 eV AB + energy for photons Autodetachment Dissociative Electron Attachment Electron A●+ B– Attachment AB + e– AB–* Associative Attachment < 15 eV AB– + energy Electron Impact Ionization Fragmentation AB+* + 2e– A● + B+* > 10 eV Photochemistry Photochemistry involves “chemical processes which occur from the electronically excited state formed by photon absorption.” – visible (1.8 eV – 3.1 eV) – near‐UV (3.1 – 4.1 eV) no ionization; only excitation – far (deep)‐UV (4.1 – 6.2 eV) – vacuum‐UV (6.2 –12.4 eV) ionization AND excitation B. -
Astrochemical Pathways to Complex Organic and Prebiotic Molecules: Experimental Perspectives for in Situ Solid-State Studies
life Review Astrochemical Pathways to Complex Organic and Prebiotic Molecules: Experimental Perspectives for In Situ Solid-State Studies Daniele Fulvio 1,2,* , Alexey Potapov 3, Jiao He 2 and Thomas Henning 2 1 Istituto Nazionale di Astrofisica, Osservatorio Astronomico di Capodimonte, Salita Moiariello 16, 80131 Naples, Italy 2 Max Planck Institute for Astronomy, Königstuhl 17, D-69117 Heidelberg, Germany; [email protected] (J.H.); [email protected] (T.H.) 3 Laboratory Astrophysics Group of the Max Planck Institute for Astronomy at the Friedrich Schiller University Jena, Institute of Solid State Physics, Helmholtzweg 3, 07743 Jena, Germany; [email protected] * Correspondence: [email protected] Abstract: A deep understanding of the origin of life requires the physical, chemical, and biological study of prebiotic systems and the comprehension of the mechanisms underlying their evolutionary steps. In this context, great attention is paid to the class of interstellar molecules known as “Complex Organic Molecules” (COMs), considered as possible precursors of prebiotic species. Although COMs have already been detected in different astrophysical environments (such as interstellar clouds, protostars, and protoplanetary disks) and in comets, the physical–chemical mechanisms underlying their formation are not yet fully understood. In this framework, a unique contribution comes from laboratory experiments specifically designed to mimic the conditions found in space. We present Citation: Fulvio, D.; Potapov, A.; He, a review of experimental studies on the formation and evolution of COMs in the solid state, i.e., J.; Henning, T. Astrochemical within ices of astrophysical interest, devoting special attention to the in situ detection and analysis Pathways to Complex Organic and techniques commonly used in laboratory astrochemistry.