Nitric Oxide 3Rd Edition Pdf, Epub, Ebook
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NBO Applications, 2020
NBO Bibliography 2020 2531 publications – Revised and compiled by Ariel Andrea on Aug. 9, 2021 Aarabi, M.; Gholami, S.; Grabowski, S. J. S-H ... O and O-H ... O Hydrogen Bonds-Comparison of Dimers of Thiocarboxylic and Carboxylic Acids Chemphyschem, (21): 1653-1664 2020. 10.1002/cphc.202000131 Aarthi, K. V.; Rajagopal, H.; Muthu, S.; Jayanthi, V.; Girija, R. Quantum chemical calculations, spectroscopic investigation and molecular docking analysis of 4-chloro- N-methylpyridine-2-carboxamide Journal of Molecular Structure, (1210) 2020. 10.1016/j.molstruc.2020.128053 Abad, N.; Lgaz, H.; Atioglu, Z.; Akkurt, M.; Mague, J. T.; Ali, I. H.; Chung, I. M.; Salghi, R.; Essassi, E.; Ramli, Y. Synthesis, crystal structure, hirshfeld surface analysis, DFT computations and molecular dynamics study of 2-(benzyloxy)-3-phenylquinoxaline Journal of Molecular Structure, (1221) 2020. 10.1016/j.molstruc.2020.128727 Abbenseth, J.; Wtjen, F.; Finger, M.; Schneider, S. The Metaphosphite (PO2-) Anion as a Ligand Angewandte Chemie-International Edition, (59): 23574-23578 2020. 10.1002/anie.202011750 Abbenseth, J.; Goicoechea, J. M. Recent developments in the chemistry of non-trigonal pnictogen pincer compounds: from bonding to catalysis Chemical Science, (11): 9728-9740 2020. 10.1039/d0sc03819a Abbenseth, J.; Schneider, S. A Terminal Chlorophosphinidene Complex Zeitschrift Fur Anorganische Und Allgemeine Chemie, (646): 565-569 2020. 10.1002/zaac.202000010 Abbiche, K.; Acharjee, N.; Salah, M.; Hilali, M.; Laknifli, A.; Komiha, N.; Marakchi, K. Unveiling the mechanism and selectivity of 3+2 cycloaddition reactions of benzonitrile oxide to ethyl trans-cinnamate, ethyl crotonate and trans-2-penten-1-ol through DFT analysis Journal of Molecular Modeling, (26) 2020. -
Ubiquitous Argonium \(Arh+\) in the Diffuse Interstellar Medium: A
A&A 566, A29 (2014) Astronomy DOI: 10.1051/0004-6361/201423727 & c ESO 2014 Astrophysics Ubiquitous argonium (ArH+) in the diffuse interstellar medium: A molecular tracer of almost purely atomic gas P. Schilke1, D. A. Neufeld2, H. S. P. Müller1, C. Comito1, E. A. Bergin3, D. C. Lis4;5, M. Gerin6, J. H. Black7, M. Wolfire8, N. Indriolo2, J. C. Pearson9, K. M. Menten10, B. Winkel10, Á. Sánchez-Monge1, T. Möller1, B. Godard6, and E. Falgarone6 1 I. Physikalisches Institut der Universität zu Köln, Zülpicher Str. 77, 50937 Köln, Germany e-mail: [email protected] 2 The Johns Hopkins University, Baltimore, MD 21218, USA 3 Department of Astronomy, The University of Michigan, 500 Church Street, Ann Arbor, MI 48109-1042, USA 4 California Institute of Technology, Pasadena, CA 91125, USA 5 Sorbonne Universités, Université Pierre et Marie Curie, Paris 6, CNRS, Observatoire de Paris, UMR 8112 LERMA, Paris, France 6 LERMA, CNRS UMR 8112, Observatoire de Paris & École Normale Supérieure, 24 rue Lhomond, 75005 Paris, France 7 Department of Earth and Space Sciences, Chalmers University of Technology, Onsala Space Observatory, 439 92 Onsala, Sweden 8 Astronomy Department, University of Maryland, College Park, MD 20742, USA 9 Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA 10 Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany Received 28 February 2014 / Accepted 29 March 2014 ABSTRACT Aims. We describe the assignment of a previously unidentified interstellar absorption line to ArH+ and discuss its relevance in the + context of hydride absorption in diffuse gas with a low H2 fraction. -
(12) Patent Application Publication (10) Pub. No.: US 2006/0110428A1 De Juan Et Al
US 200601 10428A1 (19) United States (12) Patent Application Publication (10) Pub. No.: US 2006/0110428A1 de Juan et al. (43) Pub. Date: May 25, 2006 (54) METHODS AND DEVICES FOR THE Publication Classification TREATMENT OF OCULAR CONDITIONS (51) Int. Cl. (76) Inventors: Eugene de Juan, LaCanada, CA (US); A6F 2/00 (2006.01) Signe E. Varner, Los Angeles, CA (52) U.S. Cl. .............................................................. 424/427 (US); Laurie R. Lawin, New Brighton, MN (US) (57) ABSTRACT Correspondence Address: Featured is a method for instilling one or more bioactive SCOTT PRIBNOW agents into ocular tissue within an eye of a patient for the Kagan Binder, PLLC treatment of an ocular condition, the method comprising Suite 200 concurrently using at least two of the following bioactive 221 Main Street North agent delivery methods (A)-(C): Stillwater, MN 55082 (US) (A) implanting a Sustained release delivery device com (21) Appl. No.: 11/175,850 prising one or more bioactive agents in a posterior region of the eye so that it delivers the one or more (22) Filed: Jul. 5, 2005 bioactive agents into the vitreous humor of the eye; (B) instilling (e.g., injecting or implanting) one or more Related U.S. Application Data bioactive agents Subretinally; and (60) Provisional application No. 60/585,236, filed on Jul. (C) instilling (e.g., injecting or delivering by ocular ion 2, 2004. Provisional application No. 60/669,701, filed tophoresis) one or more bioactive agents into the Vit on Apr. 8, 2005. reous humor of the eye. Patent Application Publication May 25, 2006 Sheet 1 of 22 US 2006/0110428A1 R 2 2 C.6 Fig. -
Understanding the Bonding of Second Period Diatomic Molecules Spdf Vs MCAS
Understanding the Bonding of Second Period Diatomic Molecules Spdf vs MCAS By Joel M Williams (text and images © 2013) The html version with updates and higher resolution images is at the author’s website (click here) Abstract The current spdf and MO modeling of chemical molecules are well-established, but do so by continuing to assume that non-classical physics is operating. The MCAS electron orbital model is an alternate particulate model based on classical physics. This paper describes its application to the diatomic molecules of the second period of the periodic table. In doing so, it addresses their molecular electrostatics, bond strengths, and electron affinities. Particular attention is given to the anomalies of the carbon diatom. Questions are raised about the sensibleness of the spdf model’s spatial ability to contain two electrons on an axis between diatoms and its ability to form π-bonds from parallel p-orbitals located over the nuclei of each atom. Nitrogen, carbon monoxide, oxygen, and fluorine all have the same inter-nuclei bonding: all “triple bonds” of varying strength caused by different numbers of anti-bonding electrons. The spdf model was devised for single atoms by physicists and mathematicians. Kowtowing to them, chemists produce hybrid orbitals to explain how atoms could actually form molecules. Drawing these hybrids and meshing them on paper might look great, but, constrained to measured interatomic physical dimensions and electrostatic interactions, bonding based on the spdf-hybrids (sp, sp2, sp3) is illogical. To have even one electron occupy the “bond” region between the nuclei of diatomic molecules, at the expense of reduced coverage elsewhere, does not make sense for stable molecules. -
Discharge Plasmas of Molecular Gases
/ J ¥4~r~~~: 'o j~ ~7 ~,~U;~I u t= ~]f~LL*~ ~~~~~~; 4. Isotope Separation in Discharge Plasmas of Molecular Gases EZOUBTCHENKO, Alexandre N.t, AKATSUKA Hiroshi and SUZUKI Masaaki Research Laboratory for Nuclear Reactors, Tokyo Institute of Technology, Tokyo 152-8550, Japan (Received 25 December 1997) Abstract We review the theoretical principles and the experimental methods of isotope separation achieved through the use of discharge plasmas of molecular gases. Isotope separation has been accomplished in various plasma chemical reactions. It is experimentally and theoretically shown that a state of non- equilibrium in the plasmas, especially in the vibrational distribution functions, is essential for the isotope redistribution in the reagents and products. Examples of the reactions, together with the isotope separ- ation factors known up to the present time, are shown to separate isotopic species of carbon, nitrogen and oxygen molecules in the plasma phase, generated by glow discharge and microwave discharge. Keywords: isotope separation, vibrational nonequilibrium, glow discharge, microwave discharge, plasma chemistry 4.1 Introduction isotopic species will be redistributed between the rea- Plasmas generated by electric discharge of molecu- gents and the products. We can elaborate a new lar gases under moderate pressures (10 Torr < p < method of the plasma isotope separation for light ele- 200 Torr) are usually in a state of nonequilibrium. We ments . can define various temperatures according to the kine- There were a few experimental studies of isotope tics of various particles in such plasmas, for example, separation phenomena in the nonequilibrium electric electron temperature ( T*), gas translational temperature discharge. Semiokhin et al. measured C02 enrichment ( To), gas rotational temperature ( TR) and vibrational in i3C02 and 12C160180 with a separation factor a ~ temperature ( Tv), where the relationships T* > Tv ;~ 1.01 in the C02 Silent (barrier) discharge in the pres- TR- To usually hold. -
©2018 Alexander Hook ALL RIGHTS RESERVED
©2018 Alexander Hook ALL RIGHTS RESERVED A DFT STUDY OF HYDROGEN ABSTRACTION FROM LIGHT ALKANES: Pt ALLOY DEHYDROGENATION CATALYSTS AND TIO2 STEAM REFORMING CATALYSTS By ALEXANDER HOOK A dissertation submitted to the School of Graduate Studies Rutgers, The State University of New Jersey In partial fulfillment of the requirements For the degree of Doctor of Philosophy Graduate Program in Chemical and Biochemical Engineering Written under the direction of Fuat E. Celik And approved by __________________________ __________________________ __________________________ __________________________ New Brunswick, New Jersey May, 2018 ABSTRACT OF THE DISSERTATION A DFT STUDY OF HYDROGEN ABSTRACTION FROM LIGHT ALKANES: Pt ALLOY DEHYDROGENATION CATALYSTS AND TiO2 STEAM REFORMING CATALYSTS By ALEC HOOK Dissertation Director: Fuat E. Celik Sustainable energy production is one of the biggest challenges of the 21st century. This includes effective utilization of carbon-neutral energy resources as well as clean end-use application that do not emit CO2 and other pollutants. Hydrogen gas can potentially solve the latter problem, as a clean burning fuel with very high thermodynamic energy conversion efficiency in fuel cells. In this work we will be discussing two methods of obtaining hydrogen. The first is as a byproduct of light alkane dehydrogenation where we obtain a high value olefin along with hydrogen gas. The second is in methane steam reforming where hydrogen is the primary product. Chapter 1 begins by introducing the reader to the current state of the energy industry. Afterwards there is an overview of what density functional theory (DFT) is and how this computational technique can elucidate and complement laboratory experiments. It will also contain the general parameters and methodology of the VASP software package that runs the DFT calculations. -
A Dicationic Iminophosphane Ying Kai Loh, Chitra Gurnani, Rakesh Ganguly, and Dragoslav Vidović*
A Dicationic Iminophosphane Ying Kai Loh, Chitra Gurnani, Rakesh Ganguly, and Dragoslav Vidović* Department of Chemistry and Biological Chemistry, Nanyang Technological University, 21 Nanyang Link, Singapore, 637371. Supporting Information Placeholder ABSTRACT: A novel dicationic system containing a PN frag- ment has been synthesized and structurally characterized. Accord- ing to the solid state analysis and theoretical investigation the dica- tionic iminophosphane resonance from is the most appropriate de- scription for the dication. However, the contribution from the phos- phorus mononitride resonance form is not negligible. Neutral two-eletron donor carbenes have proven to be quite versatile ligands for isolation of a wide variety of novel main group 1-4 species. Examples include diatomic allotropes (L-E2-L; L = car- bene, E = B, Si, Ge, P, As, etc)1a of boron, silicon, germanium, phosphorus, arsenic, etc.2-4 Nevertheless, these interesting mole- cules, among numerous other main group species, sparked a debate about the most appropriate way to describe bonding in these com- Figure 1. Recently isolated neutral (A) and radical cationic (B) 5,6 pounds. In particular, the arguments have been focused on phosphorus mononitrides, and general structure for carbones (C). whether the carbene moieties form typical covalent bonds or the Dipp = 2,6-diisopropylphenyl. use of dative bond analogy is also valid. The latest evidence showed that the L-E bonds for L-B2-L are quite strong suggesting a sub- stantial covalent character.6 However, Frenking argued that dative The overall synthesis of the target dication is summarized in bonds could be also very strong by the combination of -donation Scheme 1. -
Directed Gas Phase Formation of Silicon Dioxide and Implications for the Formation of Interstellar Silicates
ARTICLE DOI: 10.1038/s41467-018-03172-5 OPEN Directed gas phase formation of silicon dioxide and implications for the formation of interstellar silicates Tao Yang 1,2, Aaron M. Thomas1, Beni B. Dangi1,3, Ralf I. Kaiser 1, Alexander M. Mebel 4 & Tom J. Millar 5 1234567890():,; Interstellar silicates play a key role in star formation and in the origin of solar systems, but their synthetic routes have remained largely elusive so far. Here we demonstrate in a combined crossed molecular beam and computational study that silicon dioxide (SiO2) along with silicon monoxide (SiO) can be synthesized via the reaction of the silylidyne radical (SiH) with molecular oxygen (O2) under single collision conditions. This mechanism may provide a low-temperature path—in addition to high-temperature routes to silicon oxides in circum- stellar envelopes—possibly enabling the formation and growth of silicates in the interstellar medium necessary to offset the fast silicate destruction. 1 Department of Chemistry, University of Hawai’iatMānoa, Honolulu, HI 96822, USA. 2 State Key Laboratory of Precision Spectroscopy, East China Normal University, Shanghai, 200062, China. 3 Department of Chemistry, Florida Agricultural and Mechanical University, Tallahassee, FL 32307, USA. 4 Department of Chemistry and Biochemistry, Florida International University, Miami, FL 33199, USA. 5 Astrophysics Research Centre, School of Mathematics and Physics, Queen’s University Belfast, Belfast, BT7 1NN, UK. Correspondence and requests for materials should be addressed to R.I.K. (email: [email protected]) or to A.M.M. (email: mebela@fiu.edu) or to T.J.M. (email: [email protected]) NATURE COMMUNICATIONS | (2018) 9:774 | DOI: 10.1038/s41467-018-03172-5 | www.nature.com/naturecommunications 1 ARTICLE NATURE COMMUNICATIONS | DOI: 10.1038/s41467-018-03172-5 — 28 + 28 + he origin of interstellar silicate grains nanoparticles ( SiO2 ), and 44 ( SiO ). -
(12) United States Patent (10) Patent No.: US 6,264,917 B1 Klaveness Et Al
USOO6264,917B1 (12) United States Patent (10) Patent No.: US 6,264,917 B1 Klaveness et al. (45) Date of Patent: Jul. 24, 2001 (54) TARGETED ULTRASOUND CONTRAST 5,733,572 3/1998 Unger et al.. AGENTS 5,780,010 7/1998 Lanza et al. 5,846,517 12/1998 Unger .................................. 424/9.52 (75) Inventors: Jo Klaveness; Pál Rongved; Dagfinn 5,849,727 12/1998 Porter et al. ......................... 514/156 Lovhaug, all of Oslo (NO) 5,910,300 6/1999 Tournier et al. .................... 424/9.34 FOREIGN PATENT DOCUMENTS (73) Assignee: Nycomed Imaging AS, Oslo (NO) 2 145 SOS 4/1994 (CA). (*) Notice: Subject to any disclaimer, the term of this 19 626 530 1/1998 (DE). patent is extended or adjusted under 35 O 727 225 8/1996 (EP). U.S.C. 154(b) by 0 days. WO91/15244 10/1991 (WO). WO 93/20802 10/1993 (WO). WO 94/07539 4/1994 (WO). (21) Appl. No.: 08/958,993 WO 94/28873 12/1994 (WO). WO 94/28874 12/1994 (WO). (22) Filed: Oct. 28, 1997 WO95/03356 2/1995 (WO). WO95/03357 2/1995 (WO). Related U.S. Application Data WO95/07072 3/1995 (WO). (60) Provisional application No. 60/049.264, filed on Jun. 7, WO95/15118 6/1995 (WO). 1997, provisional application No. 60/049,265, filed on Jun. WO 96/39149 12/1996 (WO). 7, 1997, and provisional application No. 60/049.268, filed WO 96/40277 12/1996 (WO). on Jun. 7, 1997. WO 96/40285 12/1996 (WO). (30) Foreign Application Priority Data WO 96/41647 12/1996 (WO). -
H2CS) and Its Thiohydroxycarbene Isomer (HCSH
A chemical dynamics study on the gas phase formation of thioformaldehyde (H2CS) and its thiohydroxycarbene isomer (HCSH) Srinivas Doddipatlaa, Chao Hea, Ralf I. Kaisera,1, Yuheng Luoa, Rui Suna,1, Galiya R. Galimovab, Alexander M. Mebelb,1, and Tom J. Millarc,1 aDepartment of Chemistry, University of Hawai’iatManoa, Honolulu, HI 96822; bDepartment of Chemistry and Biochemistry, Florida International University, Miami, FL 33199; and cSchool of Mathematics and Physics, Queen’s University Belfast, Belfast BT7 1NN, Northern Ireland, United Kingdom Edited by Stephen J. Benkovic, The Pennsylvania State University, University Park, PA, and approved August 4, 2020 (received for review March 13, 2020) Complex organosulfur molecules are ubiquitous in interstellar molecular sulfur dioxide (SO2) (21) and sulfur (S8) (22). The second phase clouds, but their fundamental formation mechanisms have remained commences with the formation of the central protostars. Tempera- largely elusive. These processes are of critical importance in initiating a tures increase up to 300 K, and sublimation of the (sulfur-bearing) series of elementary chemical reactions, leading eventually to organo- molecules from the grains takes over (20). The subsequent gas-phase sulfur molecules—among them potential precursors to iron-sulfide chemistry exploits complex reaction networks of ion–molecule and grains and to astrobiologically important molecules, such as the amino neutral–neutral reactions (17) with models postulating that the very acid cysteine. Here, we reveal through laboratory experiments, first sulfur–carbon bonds are formed via reactions involving methyl electronic-structure theory, quasi-classical trajectory studies, and astro- radicals (CH3)andcarbene(CH2) with atomic sulfur (S) leading to chemical modeling that the organosulfur chemistry can be initiated in carbonyl monosulfide and thioformaldehyde, respectively (18). -
Injection of Meteoric Phosphorus Into Planetary Atmospheres
Planetary and Space Science 187 (2020) 104926 Contents lists available at ScienceDirect Planetary and Space Science journal homepage: www.elsevier.com/locate/pss Injection of meteoric phosphorus into planetary atmospheres Juan Diego Carrillo-Sanchez a, David L. Bones a, Kevin M. Douglas a, George J. Flynn b, Sue Wirick c, Bruce Fegley Jr. d, Tohru Araki e, Burkhard Kaulich e, John M.C. Plane a,* a School of Chemistry, University of Leeds, Woodhouse Lane, Leeds, LS2 9JT, UK b State University of New York at Plattsburgh, Department of Physics, 101 Broad Street, Plattsburg, NY, 12901, USA c Focused Beam Enterprises, Westhampton, NY, 11977, USA d Planetary Chemistry Laboratory, Department of Earth & Planetary Sciences and McDonnell Center for the Space Sciences, Washington University, St Louis, MO, 63130, USA e Diamond Light Source Ltd, Harwell Science & Innovation Campus, Didcot, OX11 0DE, UK ARTICLE INFO ABSTRACT Keywords: This study explores the delivery of phosphorus to the upper atmospheres of Earth, Mars, and Venus via the Cosmic dust ablation of cosmic dust particles. Micron-size meteoritic particles were flash heated to temperatures as high as Planetary atmospheres 2900 K in a Meteor Ablation Simulator (MASI), and the ablation of PO and Ca recorded simultaneously by laser Ablation induced fluorescence. Apatite grains were also ablated as a reference. The speciation of P in anhydrous chondritic Phosphorus thermodynamics porous Interplanetary Dust Particles was made by K-edge X-ray absorption near edge structure (XANES) spec- Zodiacal cloud troscopy, demonstrating that P mainly occurs in phosphate-like domains. A thermodynamic model of P in a sil- icate melt was then developed for inclusion in the Leeds Chemical Ablation Model (CABMOD). -
Ubiquitous Argonium, Arh+, in the Diffuse Interstellar Medium
Ubiquitous Argonium, ArH+, in the Interstellar Medium P. Schilke, Holger S. P. Müller, C. Comito, Á. Sánchez-Monge, D. A. Neufeld, N. Indriolo, E. A. Bergin, D. C. Lis, M. Gerin, J. H. Black, M. G. Wolfire, J. C. Pearson, K. M. Menten, B. Winkel V.6, 13th International HITRAN Conference, CfA, Cambridge, MA, USA, June 23–25, 2014 What is Argonium? ArH+, 1Σ+, isoelectronic to HCl + + Formation: Ar + H2 → ArH + H + + Destruction (e.g.): ArH + H2 → Ar + H3 Isotopic ratio: 36Ar : 38Ar : 40Ar terrestrial: 84.2 : 15.8 : 25018.8 (from decay of 40K) solar/ISM: ~84.6 : ~15.4 : 0.025 36ArH+ toward Crab Nebula SNR: J = 1 – 0 & 2 – 1 in emission (w. OH+ N = 1 – 0); SPIRE/Herschel M. J. Barlow et al., Science 342 (2013) 1343 On the Spectroscopy of ArH+ 40ArH+; rotational spectroscopy: K. B. Laughlin et al., PRL 58 (1987) 996: J" = 0 J. M. Brown et al., JMSp 128 (1988) 587: J" = 1 – 6 D. J. Liu et al., JCP 87 (1987) 2442: J" = 20 – 24; v ≤ 4 (MIR) 40ArD+; rotational spectroscopy: W. C. Bowman et al., JCP 79 (1983) 2093: J" = 0 (+ 36ArD+ & 38ArD+ H. Odashima et al., JMSp 195 (1999) 356: J" = 2 – 14 rovibrational spectroscopy: J. W. Brault & S. P. Davis, Phys. Sript. 25 (1982) 268: 40ArH+ J. W. C. Johns, JMSp 106 (1984) 124: 40ArH+, 40ArD+ R. R. Filueira & C. E. Blom, JMSp 127 (1988) 279: 36ArH+, 38ArH+ M. Cueto et al., ApJ 783 (2014) L5: 36ArH+, 38ArH+ ArH+ toward Sagittarius B2(M) – HIFI Line Survey Absorption toward Sgr B2(M) massive star-forming regions as background sources with approximate origins Sagittarius B2(M) Interstellar Chemistry of ArH+ I + + + + Ar + H2 → ArH + H exothermic (endo.