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WO 2016/074683 Al 19 May 2016 (19.05.2016) W P O P C T
(12) INTERNATIONAL APPLICATION PUBLISHED UNDER THE PATENT COOPERATION TREATY (PCT) (19) World Intellectual Property Organization International Bureau (10) International Publication Number (43) International Publication Date WO 2016/074683 Al 19 May 2016 (19.05.2016) W P O P C T (51) International Patent Classification: (81) Designated States (unless otherwise indicated, for every C12N 15/10 (2006.01) kind of national protection available): AE, AG, AL, AM, AO, AT, AU, AZ, BA, BB, BG, BH, BN, BR, BW, BY, (21) International Application Number: BZ, CA, CH, CL, CN, CO, CR, CU, CZ, DE, DK, DM, PCT/DK20 15/050343 DO, DZ, EC, EE, EG, ES, FI, GB, GD, GE, GH, GM, GT, (22) International Filing Date: HN, HR, HU, ID, IL, IN, IR, IS, JP, KE, KG, KN, KP, KR, 11 November 2015 ( 11. 1 1.2015) KZ, LA, LC, LK, LR, LS, LU, LY, MA, MD, ME, MG, MK, MN, MW, MX, MY, MZ, NA, NG, NI, NO, NZ, OM, (25) Filing Language: English PA, PE, PG, PH, PL, PT, QA, RO, RS, RU, RW, SA, SC, (26) Publication Language: English SD, SE, SG, SK, SL, SM, ST, SV, SY, TH, TJ, TM, TN, TR, TT, TZ, UA, UG, US, UZ, VC, VN, ZA, ZM, ZW. (30) Priority Data: PA 2014 00655 11 November 2014 ( 11. 1 1.2014) DK (84) Designated States (unless otherwise indicated, for every 62/077,933 11 November 2014 ( 11. 11.2014) US kind of regional protection available): ARIPO (BW, GH, 62/202,3 18 7 August 2015 (07.08.2015) US GM, KE, LR, LS, MW, MZ, NA, RW, SD, SL, ST, SZ, TZ, UG, ZM, ZW), Eurasian (AM, AZ, BY, KG, KZ, RU, (71) Applicant: LUNDORF PEDERSEN MATERIALS APS TJ, TM), European (AL, AT, BE, BG, CH, CY, CZ, DE, [DK/DK]; Nordvej 16 B, Himmelev, DK-4000 Roskilde DK, EE, ES, FI, FR, GB, GR, HR, HU, IE, IS, IT, LT, LU, (DK). -
The Noble Gases
The Noble Gases The Noble Gases (inert gases, Group 0, Group 18 or the helium group) are notoriously unreactive elements (‘noble’ means unreactive in chemistry) and in their elemental state they exist as monoatomic gases – gases whose ‘molecules’ are single atoms of the element, since the atoms are reluctant to react with anything, including one-another. This inertness is due to the fact that they have stable outer electron shells, with stable octets of electrons (full s and p subshells) except helium, which has a stable full inner shell. The electronic configurations are: Helium (He): 1s2 Neon (Ne): 1s2 2s2 2p6 Argon (Ar): [Ne] 3s2 3p6 Krypton (Kr): [Ar] 3d10 4s2 4p6 Xenon (Xe): [Kr] 4d10 5s2 5p6 Radon (Rn): [Xe] 5d10 6s2 6p6 Nevertheless, this group does have some interesting chemistry and also exhibit interesting physical properties. Reactivity increases down the group. Often helium is included as the first member of the group. Helium (He) Helium is chemically a highly unreactive element. It only forms transient species when electric discharges are passed through a mixture of helium gas and another gaseous element. for example, passing an electric discharge through a mixture of helium and hydrogen forms the transient molecule HHe, which has a very short half-life. HHeF is metastable. Neon (Ne) Neon is chemically the most unreactive element. It forms no true compounds, and no neutral molecules. Ionic molecules are known, e.g. (NeAr)+, (NeH)+, (HeNe)+ and Ne+. Argon (Ar) The unstable argon fluorohydride, HArF, is known. Ar also forms clathrates (see krypton) with water and highly unstable ArH+ and ArF are known. -
Inorganic Chemistry Lesson 16 Periodic Law
Inorganic Chemistry Lesson 16 Periodic Law February 11, 2018 1 How many groups? As you can see, the Table 1 is incomplete: there is a gap between each halogen and the next alkaline metal. Indeed, whereas the mass of adjacent elements differ by 2 or 3 Daltons, the difference between the mass of fluorine (19) and sodium (23), or between bromine (80) and rubidium (85) is unusually high. By the moment Mendeleev made his discovery (in 1869), scientist knew no good candidates to fill this gap. Only in 1894, British physicist Lord Raleigh and chemist Sir William Ramsay separated a strange gas form air. This gas, called argon, was present in atmosphere in small amount (ca 1%). This gas was totally inert, it did not react with any known acid, base, or oxidizer. Later Ramsay discovered other gases with same properties: Neon (Ne), Krypton (Kr), Xenon (Xe), Neon (Ne). Due to their inertness they, as well as independently discovered helium (He) and radon (Ra) are called inert, or noble gases. Initially they were believed to have maximal possible valence of zero. Accordingly, they occupied the column number zero in the early periodic table (before alkaline metals). However, in second half of XX century chemists managed to oxidize xenon and krypton to tetroxides (XeO4 and KrO4, accordingly). These oxides are low boiling liquids that are very prone to explosion. Are noble gas metals, non-metals, or they form a separate group? To answer this question, consider the properties of their oxides. When mixed with water, XeO4 slowly reacts with it yielding perxenic acid: XeO4 + H2O −−→ H4XeO6 which is a very strong acid, instable is a free form. -
Noble Gas Chemistry
Noble Gas Chemistry Noble Gas Chemistry Structure, Bonding, and Gas-Phase Chemistry Felice Grandinetti Author All books published by Wiley-VCH are carefully produced. Nevertheless, authors, Prof. Felice Grandinetti editors, and publisher do not warrant the Dipartimento per la Innovazione nei information contained in these books, sistemi Biologici including this book, to be free of errors. Agroalimentari e Forestali (DIBAF) Readers are advised to keep in mind that Università della Tuscia, L.go statements, data, illustrations, procedural dell’Università details or other items may inadvertently s.n.c., 01100 Viterbo be inaccurate. Italy Library of Congress Card No.: applied for and British Library Cataloguing-in-Publication Data Istituto per le Metodologie Chimiche del A catalogue record for this book is CNR available from the British Library. Via Salaria, Km 29.500 00015 Monterotondo, RM Bibliographic information published by Italy the Deutsche Nationalbibliothek The Deutsche Nationalbibliothek lists Cover: © Rvo233/iStockphoto this publication in the Deutsche Nation- albibliografie; detailed bibliographic dataareavailableontheInternetat <http://dnb.d-nb.de>. © 2018 Wiley-VCH Verlag GmbH & Co. KGaA, Boschstr. 12, 69469 Weinheim, Germany All rights reserved (including those of translation into other languages). No part of this book may be reproduced in any form – by photoprinting, microfilm, or any other means – nor transmitted or translated into a machine language with- out written permission from the publish- ers. Registered names, trademarks, -
The Chemistry of Xenon
THE CHEMISTRY OF XENON' JOHN G. MALM, HENRY SELIG, Chemistry Division, Argonne National Laboratory, Argonne, Illinois JOSHUA JORTNER, AND STUART A. RICE Department of Chemistry and Institute for the Study of Metals, University of Chicago, Chicago, Illinois Received September 9, 1964 CONTENTS I. Introduction.. , . 200 11. The Xenon Fluorides. , , . 200 200 * . 201 203 206 4. XeFe.......................................,... ................. 206 5. XeOFI... .. , , , . , . 208 111. Complexes of Xenon.. ........................... 209 A. Xe(PtF&. ..... ..... .. ... ...... .. ....... 209 210 C. Xenon Difluoride Complexes, . 210 210 210 ............... 210 A. XeF ......................................................................... 210 .............. 210 210 D. XeOFs.. ............ ............................. 211 211 211 211 A. General.. .. .. ... ..... .. .. .. ... ... .. .............. .... ... 211 211 211 D. Xenon Trioxide ............................................................... 212 E. Properties of Aqueous Xe(VII1). ... 212 F. Oxidation Potentials. 213 G. Perxenate Salts.. , , . , . , . 213 H. Xenon Tetroxide.. .................... ........... ............. 213 I. Analysis for Xe(V1) and Xe(V1 Oxidation States., . 213 VI. The Nature of the Chemical Bond in the Xenon Fluorides.. , . , . , . 214 A. The Electron-Correlation Model, . , . , , . , , . , , . 214 B. The Hybridization Model.. ............ ............................. 216 C. Long-Range Xenon-Fluorine Interactions . , . , . , . , . 216 D. The Molecular Orbital Model. -
The Compounds of The; Noble Gases
View Article Online / Journal Homepage / Table of Contents for this issue THE COMPOUNDS OF THE; NOBLE GASES By G. J. MOODY,B.SC., PH.D. and J. D. R. THOMAS,M.SC., F.R.I.C. Welsh College of Advanced Technology, Cardi$ In August of this year, seventy years will have elapsed and an excess of fluorine through a nickel tube at 400°C since the discovery and isolation of the first noble gas, and trapping out the product at -50°C. In this way, namely argon, by Lord Rayleigh and William Ramsay;l formation of xenon(1v) fluoride by the stage but barely two years have passed since the preparation XeF, + F2 --f XeF, . - * (2) of the first compound of a noble gas. Even though claims of compound formation by the can be checked.ll Any xenon(1v) fluoride present as impurity can be separated by flushing the vapours from noble gases have been made since their discovery, the first authentic compound was xenon hexafluoroplati- the system.14 Ultra-violet photolysis of xenon and fluorine in an nate(v), Xe+PtF,-, reported by Bartlett in June, 1962,, all-nickel vessel fitted with sapphire irradiation windows as the result of an idea arising from unrelated researches on the synthesis of dioxygenyl hexafluoroplatinate (v), gives xenon(11) fluoride with only a trace of xenon(1v) 0,+PtF6-.3*4 It was the similarity of the first ionization fluoride.le In addition, ultra-violet irradiation at 20°K of fluorine, xenon and argon mixtures deposited potential of molecular oxygen and of atomic xenon at just over 12 eV, that led to Bartlett's forecast. -
Practice Test Questions 11 Nonmetals Part 2 (Groups 14-17 and Boron)
Practice Test Questions 11 Nonmetals Part 2 (Groups 14-17 and Boron) 1. (a) Give the symbol and name for a halogen. _____ and _____________________ (b) Give the formula and name for an oxoacid. ______ and ____________________________ (c) Give the formula and name for an oxoanion. _______ and _________________________ (d) Give the chemical formula for the halogen that is a liquid at room temperature. ________ (e) Give the symbol for a chalcogen that is also a metalloid. _________ 2. Complete the following table. Formula Name CrPO3 copper(II) nitrite iron(III) sulfate HNO3 copper(II) perchlorate lithium phosphate calcium hydrogen carbonate calcium nitrate Na2SO3 H2SO3 3. Write a balanced chemical equation for each of the reactions described below. Include states of matter. (a) Liquid phosphorus trichloride is prepared from white phosphorus and chlorine gas. (b) Sulfur dioxide and water vapour react in the upper atmosphere (c) Ammonia gas is bubbled into a solution of aqueous acid. (d) Ammonia gas and boron trifluoride gas are mixed and a single solid product forms. (e) Solid P4O10 reacts with liquid H2O. (f) Ozone decays to oxygen. 4. (a) Draw Lewis structures for each of the allotropes of oxygen. (b) On your structures, clearly label any bond angles (redrawing the structure if necessary to show the proper shape) and identify the molecular geometry. 5. Name three allotropes of carbon and briefly describe each. 6. Does nitrogen exhibit allotropy? Does phosphorus? Describe the allotropes formed. 7. What is unusual about the bonding in diborane (B2H6)? Include a diagram in your answer. 8. (a) Draw Lewis structures (and resonance structures, if appropriate) for the following ions: + + IF2 and IF4 Clearly show the formal charge of any atom with a non-zero formal charge. -
Noble Gases an Overview Contents
Noble Gases An Overview Contents 1 Properties 1 1.1 Noble gas ............................................... 1 1.1.1 History ............................................ 1 1.1.2 Physical and atomic properties ................................ 2 1.1.3 Chemical properties ...................................... 3 1.1.4 Occurrence and production .................................. 5 1.1.5 Applications .......................................... 6 1.1.6 Discharge color ........................................ 7 1.1.7 See also ............................................ 7 1.1.8 Notes ............................................. 7 1.1.9 References .......................................... 9 2 Elements 11 2.1 Helium ................................................. 11 2.1.1 History ............................................ 11 2.1.2 Characteristics ........................................ 13 2.1.3 Isotopes ............................................ 16 2.1.4 Compounds .......................................... 17 2.1.5 Occurrence and production .................................. 18 2.1.6 Applications .......................................... 19 2.1.7 Inhalation and safety ..................................... 20 2.1.8 Additional images ....................................... 21 2.1.9 See also ............................................ 21 2.1.10 References .......................................... 21 2.1.11 Bibliography ......................................... 26 2.1.12 External links ......................................... 26 2.2 Neon -
Synthesis and Stability of Xenon Oxides Xe2o5 and Xe3o2 Under Pressure
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Apollo Synthesis and stability of xenon oxides Xe2O5 and Xe3O2 under pressure Agnès Dewaele1, Nicholas Worth2, Chris J. Pickard3,4,5 , Richard J. Needs2, Sakura Pascarelli6, Olivier Mathon6, Mohamed Mezouar6 and Tetsuo Irifune7,8 1CEA, DAM, DIF, F-91297 Arpajon, France 2TCM Group, Cavendish Laboratory, J J Thomson Avenue, University of Cambridge, CB3 0HE, United Kingdom 3Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, United Kingdom 4Department of Materials Science & Metallurgy, University of Cambridge, 27 Charles Babbage Road, Cambridge, CB3 0FS, United Kingdom 5Advanced Institute for Materials Research, Tohoku University 2-1-1 Katahira, Aoba, Sendai, 980-8577, Japan 6European Synchrotron Radiation Facility, BP220, 38043 Grenoble Cedex, France 7Ehime University, 2–5 Bunkyo-cho, Matsuyama 790-8577, Japan 8Earth-Life Science Institute, Tokyo Institute of Technology, Tokyo 152-8500, Japan The noble gases are the most inert atomic group, but their reactivity increases with pressure. Diamond-anvil-cell experiments and ab initio modelling have been used to investigate a possible direct reaction between xenon and oxygen at high pressures. We have synthesized two oxides below 100 GPa, Xe2O5 under oxygen-rich conditions, and Xe3O2 under oxygen-poor conditions. Xe2O5 has been observed using X-ray diffraction methods, its structure identified using ab initio random structure searching, and confirmed using X-ray absorption and Raman spectroscopies. The experiments confirm the recent prediction of Xe3O2 as a stable xenon oxide under high pressure. Xenon atoms adopt mixed oxidation states of 0 and +4 in Xe3O2 and +4 and +6 in Xe2O5. -
Chapter 3 Molecular Shape and Structure
2009년도 제2학기 화 학 2 담당교수: 신국조 Textbook: P. Atkins / L. Jones, Chemical Principles, 4th ed., Freeman (2008) Chapter 15 CHAPTER 15 THE ELEMENTS: THE LAST FOUR MAIN GROUPS GROUP 15/V : THE NITROGEN FAMILY Electronic configuration: ns23np Oxidation states: –3 ~ +5 Different reactivities Stable N2 Burning in air, P Semiconductor, As, Sb Metal, Bi Fig. 15.1 N2(l), Sb, red P, Bi, As 15.1 The Group 15/V Elements ◆ Nitrogen, N o o o m.p.: N2(–196 C) cf. O2(–183 C), Ar(–186 C) Stable triple bond: N≡ N, 944 kJ·mol–1 Bacterial fixation of N2 in nodules on the roots of beans, alfalfa,… Haber-Bosch process Electronegativity: 3.0 – Multiple oxidation states: NH3(–3), HNO3(+5), N3 (azide,–1/3) Fig. 15.2 The pea-plant bacteria. Small atomic radius: π -bond formation from 2p-orbitals, N2O3 ◆ Phosphorus (인,燐), P Large atomic radius Æ π -bond formation from 3p-orbitals Æ single bonds, P4O6 1 2009년도 제2학기 화 학 2 담당교수: 신국조 Textbook: P. Atkins / L. Jones, Chemical Principles, 4th ed., Freeman (2008) Chapter 15 Mineral, apatites, Ca3(PO4)2 ∆ 2 Ca34(PO )2(ss) ++6 SiO2( ) 10 C(s) ⎯⎯→+P4(g) 6 CaSiO3(l) +10 CO(g) White (or Yellow) phosphorus: soft, white, very reactive (burns in air, stored in water), tetrahedral P4 molecules, chemiluminescence (trioxide of phosphorus), 연막탄 Red phosphorus: less reactive, matches, amorphous network (chains of linked P4 tetrahedra) Obtained by heating (240oC) white phosphorus without air (iodine catalyst) Red phosphorus, powder ◆ Arsenic (비소,砒素), As Metalloid GaAs Æ used in lasers in CD players ◆ Antimony, Sb Metalloid Pb/Sb electrodes in lead storage batteries Semiconductors (diodes) ◆ Bismuth, Bi Fig. -
The Noble Gases: Helium, Neon, Argon, Krypton, Xenon and Radon
16 The Noble Gases: Helium, Neon, Argon, Krypton, Xenon and Radon 18.1 Introduction in the spectrum of volcanic gas from Mount Vesuvius, and the terrestrial existence of helium In 1785 H. Cavendish in his classic work on was finally confirmed by W. Ramsay(’) in the the composition of air (p. 406) noted that, after course of his intensive study of atmospheric gases repeatedly sparking a sample of air with an which led to the recognition of a new group in excess of 02, there was a small residue of gas the periodic table. This work was initiated by which he was unable to remove by chemical the physicist, Lord Rayleigh, and was recognized means and which he estimated with astonishing in 1904 by the award of the Nobel Prizes for accuracy to be “not more than &th part of Chemistry and Physics to Ramsay and Rayleigh the whole”. He could not further characterize respectively. this component of air, and its identification as In order to test Prout’s hypothesis (that the argon had to wait for more than a century. atomic weights of all elements are multiples of that of hydrogen) Rayleigh made accurate mea- But first came the discovery of helium, which surements of the densities of common gases and is unique in being the only element discovered found, to his surprise, that the density of nitrogen extraterrestrially before being found on earth. obtained from air by the removal of 02, C02 and During the solar eclipse of 18 August 1868, a new H20 was consistently about 0.5% higher than that yellow line was observed close to the sodium D of nitrogen obtained chemically from ammonia. -
Descriptive P-Block Notes Group 12
- 1 - DESCRIPTIVE P-BLOCK NOTES GROUP 12 Zinc, Cadmium and Mercury – These are being included in this p-block description because the full d-orbitals mean their properties are more p-block in character than Transition Metal. Occurrence – Chalcophiles. Major ores are ZnS, CdS and HgS (only source of Hg). Extraction usually involves roasting to oxide then reduction over C, although HgS + O2 gives Hg + SO2 directly. Elemental Form & Allotropes – They have noticeably lower melting points and boiling points. Mercury is a liquid at room temperature. Hg is also unique in that it is the only element apart from the noble gases that is a monatomic vapour. Zn and Cd are silvery solid with bluish lustre. Liquid Hg has exceptionally high electrical resistivity for a metal. Zn and Cd show distortion of metallic HCP. All these metals have widely separated coplanar atoms giving lower density and tensile strength than Group 11. This is due to the stability of the d electrons now being tightly bound to the nucleus, such that metallic bonding uses only s electrons (weak). Reactivity – Zn and Cd tarnish in air and will combine with O, S, P & X on heating. Mercury also reacts with these (except P). Non-oxidising acids dissolve Zn and Cd, but not Hg. Zn is the only element which dissolves in aqueous alkali. All 3 elements are often used in alloys, e.g. brass and amalgams of mercury. The trend is for Zn and Cd to be very similar in reactivity, while Hg is quite different. Zn and Cd are more electropositive, while Hg is comparatively inert.