The Physical and Physiological Aspects of Xenon Isotopes in Nuclear Medical Applications
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
1 11. Nuclear Chemistry 11.1 Stable and Unstable Nuclides Very Large
11. Nuclear Chemistry Chemical reactions occur as a result of loosing/gaining and sharing electrons in the valance shell which is far away from the atomic nucleus as we described in previous chapters in chemical bonding. In chemical reactions identity of the elements (atomic) and the makeup of the nuclei (mass due to protons and neutrons) is preserved which is reflected in the Law of Conservation of mass. This idea of atomic nucleus is always stable was shattered as Henri Becquerel discovered radioactivity in uranium compound where uranium nuclei changes or undergo nuclear reactions where nuclei of an element is transformed into nuclei of different element(s) while emitting ionization radiation. Marie Curie also began a study of radioactivity in a different form of uranium ore called pitchblende and she discovered the existence of two more highly radioactive new elements radium and polonium formed as the products during the decay of unstable nuclide of uranium-235. Curie measure that the radiation emanated was proportional to the amount (moles or number of nuclides) of radioactive element present, and she proposed that radiation was a property nucleus of an unstable atom. The area of chemistry that focuses on the nuclear changes is called nuclear chemistry. What changes in a nuclide result from the loss of each of the following? a) An alpha particle. b) A gamma ray. c) An electron. d) A neutron. e) A proton. Answer: a), c), d), e) 11.1 Stable and Unstable Nuclides There are stable and unstable radioactive nuclides. Unstable nuclides emit subatomic particles, with alpha −α, beta −β, gamma −γ, proton-p, neutrons-n being the most common. -
Potential Ivvs.Gelbasedre
US010644304B2 ( 12 ) United States Patent ( 10 ) Patent No.: US 10,644,304 B2 Ein - Eli et al. (45 ) Date of Patent : May 5 , 2020 (54 ) METHOD FOR PASSIVE METAL (58 ) Field of Classification Search ACTIVATION AND USES THEREOF ??? C25D 5/54 ; C25D 3/665 ; C25D 5/34 ; ( 71) Applicant: Technion Research & Development HO1M 4/134 ; HOTM 4/366 ; HO1M 4/628 ; Foundation Limited , Haifa ( IL ) (Continued ) ( 72 ) Inventors : Yair Ein - Eli , Haifa ( IL ) ; Danny (56 ) References Cited Gelman , Haifa ( IL ) ; Boris Shvartsev , Haifa ( IL ) ; Alexander Kraytsberg , U.S. PATENT DOCUMENTS Yokneam ( IL ) 3,635,765 A 1/1972 Greenberg 3,650,834 A 3/1972 Buzzelli ( 73 ) Assignee : Technion Research & Development Foundation Limited , Haifa ( IL ) (Continued ) ( * ) Notice : Subject to any disclaimer , the term of this FOREIGN PATENT DOCUMENTS patent is extended or adjusted under 35 CN 1408031 4/2003 U.S.C. 154 ( b ) by 56 days . EP 1983078 10/2008 (21 ) Appl. No .: 15 /300,359 ( Continued ) ( 22 ) PCT Filed : Mar. 31 , 2015 OTHER PUBLICATIONS (86 ) PCT No .: PCT/ IL2015 /050350 Hagiwara et al. in ( Acidic 1 - ethyl - 3 -methylimidazoliuum fluoride: a new room temperature ionic liquid in Journal of Fluorine Chem $ 371 (c ) ( 1 ), istry vol . 99 ( 1999 ) p . 1-3 ; ( Year: 1999 ). * (2 ) Date : Sep. 29 , 2016 (Continued ) (87 ) PCT Pub . No .: WO2015 / 151099 Primary Examiner — Jonathan G Jelsma PCT Pub . Date : Oct. 8 , 2015 Assistant Examiner Omar M Kekia (65 ) Prior Publication Data (57 ) ABSTRACT US 2017/0179464 A1 Jun . 22 , 2017 Disclosed is a method for activating a surface of metals , Related U.S. Application Data such as self- passivated metals , and of metal -oxide dissolu tion , effected using a fluoroanion -containing composition . -
Noble Gas Bonding Interactions Involving Xenon Oxides and Fluorides
molecules Review Noble Gas Bonding Interactions Involving Xenon Oxides and Fluorides Antonio Frontera Department of Chemistry, Universitat de les Illes Balears, Crta de valldemossa km 7.5, 07122 Palma de Mallorca (Baleares), Spain; [email protected] Academic Editor: Felice Grandinetti Received: 17 July 2020; Accepted: 27 July 2020; Published: 28 July 2020 Abstract: Noble gas (or aerogen) bond (NgB) can be outlined as the attractive interaction between an electron-rich atom or group of atoms and any element of Group-18 acting as an electron acceptor. The IUPAC already recommended systematic nomenclature for the interactions of groups 17 and 16 (halogen and chalcogen bonds, respectively). Investigations dealing with noncovalent interactions involving main group elements (acting as Lewis acids) have rapidly grown in recent years. They are becoming acting players in essential fields such as crystal engineering, supramolecular chemistry, and catalysis. For obvious reasons, the works devoted to the study of noncovalent Ng-bonding interactions are significantly less abundant than halogen, chalcogen, pnictogen, and tetrel bonding. Nevertheless, in this short review, relevant theoretical and experimental investigations on noncovalent interactions involving Xenon are emphasized. Several theoretical works have described the physical nature of NgB and their interplay with other noncovalent interactions, which are discussed herein. Moreover, exploring the Cambridge Structural Database (CSD) and Inorganic Crystal Structure Database (ICSD), it is demonstrated that NgB interactions are crucial in governing the X-ray packing of xenon derivatives. Concretely, special attention is given to xenon fluorides and xenon oxides, since they exhibit a strong tendency to establish NgBs. Keywords: noble gas interactions; noncovalent interactions; crystal packing; xenon 1. -
Chemistry of the Noble Gases*
CHEMISTRY OF THE NOBLE GASES* By Professor K. K. GREE~woon , :.\I.Sc., sc.D .. r".lU.C. University of N ewca.stle 1tpon Tyne The inert gases, or noble gases as they are elements were unsuccessful, and for over now more appropriately called, are a remark 60 years they epitomized chemical inertness. able group of elements. The lightest, helium, Indeed, their electron configuration, s2p6, was recognized in the gases of the sun before became known as 'the stable octet,' and this it was isolated on ea.rth as its name (i]A.tos) fotmed the basis of the fit·st electronic theory implies. The first inert gas was isolated in of valency in 1916. Despite this, many 1895 by Ramsay and Rayleigh; it was named people felt that it should be possible to induce argon (apy6s, inert) and occurs to the extent the inert gases to form compounds, and many of 0·93% in the earth's atmosphere. The of the early experiments directed to this end other gases were all isolated before the turn have recently been reviewed.l of the century and were named neon (v€ov, There were several reasons why chemists new), krypton (KpVn'TOV, hidden), xenon believed that the inert gases might form ~€vov, stmnger) and radon (radioactive chemical compounds under the correct con emanation). Though they occur much less ditions. For example, the ionization poten abundantly than argon they cannot strictly tial of xenon is actually lower than those of be called rare gases; this can be illustrated hydrogen, nitrogen, oxygen, fl uorine and by calculating the volumes occupied a.t s.t.p. -
Mole Ratio Problems
Name: Answer Key Period: ______ Date: __________ Chem B Problems 1 – 6 for HW, the rest for extra practice/review WS 4.6: Mole Ratio Problems Directions: Solve the Following Problems. Show all work on a separate sheet of paper and box your final answer. 1) How many moles of Nitrogen Dioxide will be made from the reaction of 5.5 moles of Dinitrogen Tetraoxide? N2O4(g) → 2 NO2(g) 11 mol NO2 2) How many moles of NH3 will be produced when 13 moles of H2 reacts? N2(g) + 3 H2(g) → 2 NH3(g) 8.7 mol NH3 3) How many moles of NH3 will be produced when 7.0 moles of N2 reacts? N2(g) + 3 H2(g) → 2 NH3(g) 14 mol NH3 4) How many moles of Technetium(VII) Oxide will can be produced from 3.8 moles of Technetium? 4 Tc + 7 O2 → 2 Tc2O7 1.9 mol Tc2O7 5) Given the reaction below, how many moles of Vandium(II) Chloride will form when 3.22 moles of Hydrogen gas reacts? 2 VCl3 + H2 → 2 VCl2 + 2 HCl 6.44 mol VCl2 6) If 12 moles C8H18 burns in excess oxygen, how many moles of Carbon Dioxide will enter the atmosphere and further contribute to global warming? 2 C8H18(l) + 25 O2(g) → 16 CO2(g) + 18 H2O(g) 96 mol CO2 7) If 45.0 moles of CH4 reacts, how many moles of water will be produce? CH4(g) + 2 O2(g) → CO2(g) + 2 H2O(g) 90.0 mol H2O 8) How many moles of lead can be extracted if 50 moles of Carbon are used? 2 PbO + C → 2 Pb + CO2 100 mol Pb 9) For the reaction below, determine how many moles of S2Cl2 formed when 7.80 moles of Sulfur reacts? S8 + 4 Cl2 → 4 S2Cl2 31.2 mol S2Cl2 10) How many moles of Bismuth(III) Sulfate “Bi2(SO4)3” will can be produced if 25.0 moles -
Background and Derivation of ANS-5.4 Standard Fission Product Release Model
NUREG/CR-7003 PNNL-18490 Background and Derivation of ANS-5.4 Standard Fission Product Release Model Office of Nuclear Regulatory Research AVAILABILITY OF REFERENCE MATERIALS IN NRC PUBLICATIONS NRC Reference Material Non-NRC Reference Material As of November 1999, you may electronically access Documents available from public and special technical NUREG-series publications and other NRC records at libraries include all open literature items, such as NRC’s Public Electronic Reading Room at books, journal articles, and transactions, Federal http://www.nrc.gov/reading-rm.html. Register notices, Federal and State legislation, and Publicly released records include, to name a few, congressional reports. Such documents as theses, NUREG-series publications; Federal Register notices; dissertations, foreign reports and translations, and applicant, licensee, and vendor documents and non-NRC conference proceedings may be purchased correspondence; NRC correspondence and internal from their sponsoring organization. memoranda; bulletins and information notices; inspection and investigative reports; licensee event reports; and Commission papers and their attachments. Copies of industry codes and standards used in a substantive manner in the NRC regulatory process are NRC publications in the NUREG series, NRC maintained at— regulations, and Title 10, Energy, in the Code of The NRC Technical Library Federal Regulations may also be purchased from one Two White Flint North of these two sources. 11545 Rockville Pike 1. The Superintendent of Documents Rockville, MD 20852–2738 U.S. Government Printing Office Mail Stop SSOP Washington, DC 20402–0001 These standards are available in the library for Internet: bookstore.gpo.gov reference use by the public. Codes and standards are Telephone: 202-512-1800 usually copyrighted and may be purchased from the Fax: 202-512-2250 originating organization or, if they are American 2. -
The Delimiting/Frontier Lines of the Constituents of Matter∗
The delimiting/frontier lines of the constituents of matter∗ Diógenes Galetti1 and Salomon S. Mizrahi2 1Instituto de Física Teórica, Universidade Estadual Paulista (UNESP), São Paulo, SP, Brasily 2Departamento de Física, CCET, Universidade Federal de São Carlos, São Carlos, SP, Brasilz (Dated: October 23, 2019) Abstract Looking at the chart of nuclides displayed at the URL of the International Atomic Energy Agency (IAEA) [1] – that contains all the known nuclides, the natural and those produced artificially in labs – one verifies the existence of two, not quite regular, delimiting lines between which dwell all the nuclides constituting matter. These lines are established by the highly unstable radionuclides located the most far away from those in the central locus, the valley of stability. Here, making use of the “old” semi-empirical mass formula for stable nuclides together with the energy-time uncertainty relation of quantum mechanics, by a simple calculation we show that the obtained frontier lines, for proton and neutron excesses, present an appreciable agreement with the delimiting lines. For the sake of presenting a somewhat comprehensive panorama of the matter in our Universe and their relation with the frontier lines, we narrate, in brief, what is currently known about the astrophysical nucleogenesis processes. Keywords: chart of nuclides, nucleogenesis, nuclide mass formula, valley/line of stability, energy-time un- certainty relation, nuclide delimiting/frontier lines, drip lines arXiv:1909.07223v2 [nucl-th] 22 Oct 2019 ∗ This manuscript is based on an article that was published in Brazilian portuguese language in the journal Revista Brasileira de Ensino de Física, 2018, 41, e20180160. http://dx.doi.org/10.1590/ 1806-9126-rbef-2018-0160. -
Chemical Names and CAS Numbers Final
Chemical Abstract Chemical Formula Chemical Name Service (CAS) Number C3H8O 1‐propanol C4H7BrO2 2‐bromobutyric acid 80‐58‐0 GeH3COOH 2‐germaacetic acid C4H10 2‐methylpropane 75‐28‐5 C3H8O 2‐propanol 67‐63‐0 C6H10O3 4‐acetylbutyric acid 448671 C4H7BrO2 4‐bromobutyric acid 2623‐87‐2 CH3CHO acetaldehyde CH3CONH2 acetamide C8H9NO2 acetaminophen 103‐90‐2 − C2H3O2 acetate ion − CH3COO acetate ion C2H4O2 acetic acid 64‐19‐7 CH3COOH acetic acid (CH3)2CO acetone CH3COCl acetyl chloride C2H2 acetylene 74‐86‐2 HCCH acetylene C9H8O4 acetylsalicylic acid 50‐78‐2 H2C(CH)CN acrylonitrile C3H7NO2 Ala C3H7NO2 alanine 56‐41‐7 NaAlSi3O3 albite AlSb aluminium antimonide 25152‐52‐7 AlAs aluminium arsenide 22831‐42‐1 AlBO2 aluminium borate 61279‐70‐7 AlBO aluminium boron oxide 12041‐48‐4 AlBr3 aluminium bromide 7727‐15‐3 AlBr3•6H2O aluminium bromide hexahydrate 2149397 AlCl4Cs aluminium caesium tetrachloride 17992‐03‐9 AlCl3 aluminium chloride (anhydrous) 7446‐70‐0 AlCl3•6H2O aluminium chloride hexahydrate 7784‐13‐6 AlClO aluminium chloride oxide 13596‐11‐7 AlB2 aluminium diboride 12041‐50‐8 AlF2 aluminium difluoride 13569‐23‐8 AlF2O aluminium difluoride oxide 38344‐66‐0 AlB12 aluminium dodecaboride 12041‐54‐2 Al2F6 aluminium fluoride 17949‐86‐9 AlF3 aluminium fluoride 7784‐18‐1 Al(CHO2)3 aluminium formate 7360‐53‐4 1 of 75 Chemical Abstract Chemical Formula Chemical Name Service (CAS) Number Al(OH)3 aluminium hydroxide 21645‐51‐2 Al2I6 aluminium iodide 18898‐35‐6 AlI3 aluminium iodide 7784‐23‐8 AlBr aluminium monobromide 22359‐97‐3 AlCl aluminium monochloride -
Xenon Iron Oxides Predicted As Potential Xe Hosts in Earth’S Lower Mantle
ARTICLE https://doi.org/10.1038/s41467-020-19107-y OPEN Xenon iron oxides predicted as potential Xe hosts in Earth’s lower mantle ✉ Feng Peng 1,2,8, Xianqi Song 3,4,8, Chang Liu4,5,6, Quan Li 3,4,5,6 , Maosheng Miao 2, ✉ ✉ Changfeng Chen 7 & Yanming Ma 3,4,5 An enduring geological mystery concerns the missing xenon problem, referring to the abnormally low concentration of xenon compared to other noble gases in Earth’s atmosphere. 1234567890():,; Identifying mantle minerals that can capture and stabilize xenon has been a great challenge in materials physics and xenon chemistry. Here, using an advanced crystal structure search algorithm in conjunction with first-principles calculations we find reactions of xenon with recently discovered iron peroxide FeO2, forming robust xenon-iron oxides Xe2FeO2 and XeFe3O6 with significant Xe-O bonding in a wide range of pressure-temperature conditions corresponding to vast regions in Earth’s lower mantle. Calculated mass density and sound velocities validate Xe-Fe oxides as viable lower-mantle constituents. Meanwhile, Fe oxides do not react with Kr, Ar and Ne. It means that if Xe exists in the lower mantle at the same pressures as FeO2, xenon-iron oxides are predicted as potential Xe hosts in Earth’s lower mantle and could provide the repository for the atmosphere’s missing Xe. These findings establish robust materials basis, formation mechanism, and geological viability of these Xe-Fe oxides, which advance fundamental knowledge for understanding xenon chemistry and physics mechanisms for the possible deep-Earth Xe reservoir. 1 College of Physics and Electronic Information & Henan Key Laboratory of Electromagnetic Transformation and Detection, Luoyang Normal University, 471022 Luoyang, China. -
Coordination Chemistry of Xenon
Coordination Chemistry of Xenon Paul Griffin Literature Seminar 11/14/19 Situated on the far side of the periodic table, the chemical inertness of the noble gases has led to their widespread applications ranging from gas-discharge lamps and ion engines for space travel to medical applications including as MRI contrast agents and radiotherapy.1 Though all practical applications of the noble gases center around Xe (0), understanding the reactivity and bonding of xenon in higher oxidation states is fundamental to investigating chemistry at the far end of the periodic table. The reactivity of the noble gases, in particular xenon, was first uncovered when Bartlett, who had previously prepared dioxygenyl hexafluoroplatinate (V) (O2PtF6), noted similar ionization energies for molecular oxygen and atomic xenon (a difference of 0.1 eV).2 Mixing of xenon with PtF6 vapor led to the formation of an orange-yellow solid led to the synthesis of the first noble gas compound, xenon hexafluoroplatinate (V) (XePtF6). The chemistry of xenon has evolved significantly since its’ discovery to include an assortment of xenon fluorides, oxides, oxylfluorides, organoxenon3, and metalloxenon compounds such as the tetraxenoaurate (II) cation (Figure 1).4 These species have weak covalent bonding between Xe and the oxygen/fluorine moieties.5 The chemistry of xenon is dominated by the 2+, 4+, and 6+ oxidation states, though Xe (VIII) compounds are known in the form of perxenates and xenon tetroxide. These primarily ionic species, particularly the oxides, oxylfluorides, and fluorides, serve as precursors to noncovalent adducts of xenon. Figure 1. Organoxenon and metalloxenon species Recent work has led to the preparation of xenon adducts with noncovalently interacting ligands such as acetonitrile6a, 6b, ketones6c, sulfoxides6c, and crown ethers6d (Figure 2) capable of weakly coordinating to xenon salts to afford stable species at room temperature. -
Basic Answer Key Chapter 7: Chemical
CK-12 Chemistry - Basic Answer Key Chapter 7: Chemical Nomenclature 7.1 Ionic Compounds Lesson Review Questions Questions 1. What is the purpose of an empirical formula? 2. Define binary and ternary ionic compounds. 3. What is the difference between a monatomic and a polyatomic ion? 4. For each of the following ionic compounds, what ions are present and in what ratio? (a) MgBr2 (b) Li2CO3 (c) Fe2(SO4)3 5. Predict the compound that forms when gallium combines with oxygen. What would the name of this compound be? 6. Give the formula for each of the following ionic compounds: (a) ammonium nitrate (d) vanadium(III) oxide (b) cobalt(II) sulfate (e) barium oxide (c) nickel(II) cyanide (f) calcium hypochlorite 7. Name the following ionic compounds: (a) MgBr2 (b) (d) KMnO4 (c) Li2CO3 (d) (NH4)2S (e) KHSO3 (f) CuCl (g) CuCl2 8. Write the correct formulas for the following ionic compounds: a. Barium chloride b. Chromium(III) oxide c. Potassium sulfate d. Zinc phosphate Answer: 1. The empirical formula is the most straightforward way to describe the structure of a molecule, using a chemical formula that gives the lowest whole number ratio between the ions involved. 1 2. Binary ionic compounds are compounds composed of only two elements (like NaCl). Ternary ionic compounds are those composed of more than two elements (like KOH). 3. Monatomic ions form when a single atom gains or loses electrons (Na+). A polyatomic ion is an ion composed of more than one atom (Ammonium ion) 4. Answers: a. Mg2+ and 2 Br- + 2- b. -
Chemistry of Noble Gases
Prepared by: Dr. Ambika Kumar Asst. Prof. in Chemistry B. N. College Bhagalpur Contact No. 7542811733 e-mail ID: [email protected] Unit VI- Chemistry of Noble Gases The noble gases make up a group of chemical elements with similar properties; under standard conditions, they are all odorless, colorless, monatomic gases with very low chemical reactivity. The six naturally occurring noble gases are helium, neon, argon, krypton, xenon, and the radioactive radon. Chemistry of Xenon (Xe) Xenon (Xe), chemical element, a heavy and extremely rare gas of Group 18 (noble gases) of the periodic table. It was the first noble gas found to form true chemical compounds. More than 4.5 times heavier than air, xenon is colourless, odourless, and tasteless. Solid xenon belongs to the face-centred cubic crystal system, which implies that its molecules, which consist of single atoms, behave as spheres packed together as closely as possible. The name xenon is derived from the Greek word xenos, “strange” or “foreign.” Compounds of Xenon Not all the noble gases combine with oxygen and fluorine. Only the heavier noble gases like Xe (larger atomic radius) will react with oxygen and fluorine. Noble gas form compounds with oxygen and fluorine only because they are most electronegative elements. So they can ionise Xenon easily. 1.Xenon Fluorides: Xenon forms three fluorides, XeF2, XeF4 and XeF6. These can be obtained by the direct interaction between xenon and fluorine under appropriate experimental conditions, XeF2, XeF4 and XeF6 are colourless crystalline solids and sublime readily at 298 K. They are powerful fluorinating agents.