High Pressure and Low Temperature
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Ice Ic” Werner F
Extent and relevance of stacking disorder in “ice Ic” Werner F. Kuhsa,1, Christian Sippela,b, Andrzej Falentya, and Thomas C. Hansenb aGeoZentrumGöttingen Abteilung Kristallographie (GZG Abt. Kristallographie), Universität Göttingen, 37077 Göttingen, Germany; and bInstitut Laue-Langevin, 38000 Grenoble, France Edited by Russell J. Hemley, Carnegie Institution of Washington, Washington, DC, and approved November 15, 2012 (received for review June 16, 2012) “ ” “ ” A solid water phase commonly known as cubic ice or ice Ic is perfectly cubic ice Ic, as manifested in the diffraction pattern, in frequently encountered in various transitions between the solid, terms of stacking faults. Other authors took up the idea and liquid, and gaseous phases of the water substance. It may form, attempted to quantify the stacking disorder (7, 8). The most e.g., by water freezing or vapor deposition in the Earth’s atmo- general approach to stacking disorder so far has been proposed by sphere or in extraterrestrial environments, and plays a central role Hansen et al. (9, 10), who defined hexagonal (H) and cubic in various cryopreservation techniques; its formation is observed stacking (K) and considered interactions beyond next-nearest over a wide temperature range from about 120 K up to the melt- H-orK sequences. We shall discuss which interaction range ing point of ice. There was multiple and compelling evidence in the needs to be considered for a proper description of the various past that this phase is not truly cubic but composed of disordered forms of “ice Ic” encountered. cubic and hexagonal stacking sequences. The complexity of the König identified what he called cubic ice 70 y ago (11) by stacking disorder, however, appears to have been largely over- condensing water vapor to a cold support in the electron mi- looked in most of the literature. -
A Primer on Ice
A Primer on Ice L. Ridgway Scott University of Chicago Release 0.3 DO NOT DISTRIBUTE February 22, 2012 Contents 1 Introduction to ice 1 1.1 Lattices in R3 ....................................... 2 1.2 Crystals in R3 ....................................... 3 1.3 Comparingcrystals ............................... ..... 4 1.3.1 Quotientgraph ................................. 4 1.3.2 Radialdistributionfunction . ....... 5 1.3.3 Localgraphstructure. .... 6 2 Ice I structures 9 2.1 IceIh........................................... 9 2.2 IceIc........................................... 12 2.3 SecondviewoftheIccrystalstructure . .......... 14 2.4 AlternatingIh/Iclayeredstructures . ........... 16 3 Ice II structure 17 Draft: February 22, 2012, do not distribute i CONTENTS CONTENTS Draft: February 22, 2012, do not distribute ii Chapter 1 Introduction to ice Water forms many different crystal structures in its solid form. These provide insight into the potential structures of ice even in its liquid phase, and they can be used to calibrate pair potentials used for simulation of water [9, 14, 15]. In crowded biological environments, water may behave more like ice that bulk water. The different ice structures have different dielectric properties [16]. There are many crystal structures of ice that are topologically tetrahedral [1], that is, each water molecule makes four hydrogen bonds with other water molecules, even though the basic structure of water is trigonal [3]. Two of these crystal structures (Ih and Ic) are based on the same exact local tetrahedral structure, as shown in Figure 1.1. Thus a subtle understanding of structure is required to differentiate them. We refer to the tetrahedral structure depicted in Figure 1.1 as an exact tetrahedral structure. In this case, one water molecule is in the center of a square cube (of side length two), and it is hydrogen bonded to four water molecules at four corners of the cube. -
Arxiv:2004.08465V2 [Cond-Mat.Stat-Mech] 11 May 2020
Phase equilibrium of liquid water and hexagonal ice from enhanced sampling molecular dynamics simulations Pablo M. Piaggi1 and Roberto Car2 1)Department of Chemistry, Princeton University, Princeton, NJ 08544, USA a) 2)Department of Chemistry and Department of Physics, Princeton University, Princeton, NJ 08544, USA (Dated: 13 May 2020) We study the phase equilibrium between liquid water and ice Ih modeled by the TIP4P/Ice interatomic potential using enhanced sampling molecular dynamics simulations. Our approach is based on the calculation of ice Ih-liquid free energy differences from simulations that visit reversibly both phases. The reversible interconversion is achieved by introducing a static bias potential as a function of an order parameter. The order parameter was tailored to crystallize the hexagonal diamond structure of oxygen in ice Ih. We analyze the effect of the system size on the ice Ih-liquid free energy differences and we obtain a melting temperature of 270 K in the thermodynamic limit. This result is in agreement with estimates from thermodynamic integration (272 K) and coexistence simulations (270 K). Since the order parameter does not include information about the coordinates of the protons, the spontaneously formed solid configurations contain proton disorder as expected for ice Ih. I. INTRODUCTION ture forms in an orientation compatible with the simulation box9. The study of phase equilibria using computer simulations is of central importance to understand the behavior of a given model. However, finding the thermodynamic condition at II. CRYSTAL STRUCTURE OF ICE Ih which two or more phases coexist is particularly hard in the presence of first order phase transitions. -
Planets of the Solar System
Chapter Planets of the 27 Solar System Chapter OutlineOutline 1 ● Formation of the Solar System The Nebular Hypothesis Formation of the Planets Formation of Solid Earth Formation of Earth’s Atmosphere Formation of Earth’s Oceans 2 ● Models of the Solar System Early Models Kepler’s Laws Newton’s Explanation of Kepler’s Laws 3 ● The Inner Planets Mercury Venus Earth Mars 4 ● The Outer Planets Gas Giants Jupiter Saturn Uranus Neptune Objects Beyond Neptune Why It Matters Exoplanets UnderstandingU d t di theth formationf ti and the characteristics of our solar system and its planets can help scientists plan missions to study planets and solar systems around other stars in the universe. 746 Chapter 27 hhq10sena_psscho.inddq10sena_psscho.indd 774646 PDF 88/15/08/15/08 88:43:46:43:46 AAMM Inquiry Lab Planetary Distances 20 min Turn to Appendix E and find the table entitled Question to Get You Started “Solar System Data.” Use the data from the How would the distance of a planet from the sun “semimajor axis” row of planetary distances to affect the time it takes for the planet to complete devise an appropriate scale to model the distances one orbit? between planets. Then find an indoor or outdoor space that will accommodate the farthest distance. Mark some index cards with the name of each planet, use a measuring tape to measure the distances according to your scale, and place each index card at its correct location. 747 hhq10sena_psscho.inddq10sena_psscho.indd 774747 22/26/09/26/09 111:42:301:42:30 AAMM These reading tools will help you learn the material in this chapter. -
Deuterium – Tritium Pulse Propulsion with Hydrogen As Propellant and the Entire Space-Craft As a Gigavolt Capacitor for Ignition
Deuterium – Tritium pulse propulsion with hydrogen as propellant and the entire space-craft as a gigavolt capacitor for ignition. By F. Winterberg University of Nevada, Reno Abstract A deuterium-tritium (DT) nuclear pulse propulsion concept for fast interplanetary transport is proposed utilizing almost all the energy for thrust and without the need for a large radiator: 1. By letting the thermonuclear micro-explosion take place in the center of a liquid hydrogen sphere with the radius of the sphere large enough to slow down and absorb the neutrons of the DT fusion reaction, heating the hydrogen to a fully ionized plasma at a temperature of ~ 105 K. 2. By using the entire spacecraft as a magnetically insulated gigavolt capacitor, igniting the DT micro-explosion with an intense GeV ion beam discharging the gigavolt capacitor, possible if the space craft has the topology of a torus. 1. Introduction The idea to use the 80% of the neutron energy released in the DT fusion reaction for nuclear micro-bomb rocket propulsion, by surrounding the micro-explosion with a thick layer of liquid hydrogen heated up to 105 K thereby becoming part of the exhaust, was first proposed by the author in 1971 [1]. Unlike the Orion pusher plate concept, the fire ball of the fully ionized hydrogen plasma can here be reflected by a magnetic mirror. The 80% of the energy released into 14MeV neutrons cannot be reflected by a magnetic mirror for thermonuclear micro-bomb propulsion. This was the reason why for the Project Daedalus interstellar probe study of the British Interplanetary Society [2], the neutron poor deuterium-helium 3 (DHe3) reaction was chosen. -
Investigation of the Use of Deuterium and Oxygen in Illicit Fentanyl Analysis Author(S): John F
The author(s) shown below used Federal funding provided by the U.S. Department of Justice to prepare the following resource: Document Title: Investigation of the Use of Deuterium and Oxygen in Illicit Fentanyl Analysis Author(s): John F. Casale, Mike Lott, Jennifer R. Mallette Document Number: 255103 Date Received: August 2020 Award Number: NIJ-ONDCP IAA: 2017 DEA contract research task This resource has not been published by the U.S. Department of Justice. This resource is being made publically available through the Office of Justice Programs’ National Criminal Justice Reference Service. Opinions or points of view expressed are those of the author(s) and do not necessarily reflect the official position or policies of the U.S. Department of Justice. Investigation of the Use of Deuterium and Oxygen in Illicit Fentanyl Analysis John F. Casalea, Mike Lottb, and Jennifer R. Mallettea aU.S. Drug Enforcement Administration Special Testing and Research Laboratory Dulles, VA bIsoForensics, Inc. Salt Lake City, UT 84108 This work was conducted through an Inter-Agency Agreement dated June 28, 2017, between the Office of National Drug Control Policy (ONDCP) and the National Institute of Justice (NIJ), under DEA Contract number 15DDHQ18P00000344 with funding from the NIJ, Office of Justice Programs, U.S. Department of Justice. The opinions, findings, and conclusions or recommendations expressed in this publication/program/exhibition are those of the authors, and do not necessarily reflect those of the Department of Justice or ONDCP. This resource was prepared by the author(s) using Federal funds provided by the U.S. Department of Justice. -
Isotopic Fractionation of Carbon, Deuterium, and Nitrogen: a Full Chemical Study?
A&A 576, A99 (2015) Astronomy DOI: 10.1051/0004-6361/201425113 & c ESO 2015 Astrophysics Isotopic fractionation of carbon, deuterium, and nitrogen: a full chemical study? E. Roueff1;2, J. C. Loison3, and K. M. Hickson3 1 LERMA, Observatoire de Paris, PSL Research University, CNRS, UMR8112, Place Janssen, 92190 Meudon Cedex, France e-mail: [email protected] 2 Sorbonne Universités, UPMC Univ. Paris 6, 4 Place Jussieu, 75005 Paris, France 3 ISM, Université de Bordeaux – CNRS, UMR 5255, 351 cours de la Libération, 33405 Talence Cedex, France e-mail: [email protected] Received 6 October 2014 / Accepted 5 January 2015 ABSTRACT Context. The increased sensitivity and high spectral resolution of millimeter telescopes allow the detection of an increasing number of isotopically substituted molecules in the interstellar medium. The 14N/15N ratio is difficult to measure directly for molecules con- taining carbon. Aims. Using a time-dependent gas-phase chemical model, we check the underlying hypothesis that the 13C/12C ratio of nitriles and isonitriles is equal to the elemental value. Methods. We built a chemical network that contains D, 13C, and 15N molecular species after a careful check of the possible fraction- ation reactions at work in the gas phase. Results. Model results obtained for two different physical conditions that correspond to a moderately dense cloud in an early evolu- tionary stage and a dense, depleted prestellar core tend to show that ammonia and its singly deuterated form are somewhat enriched 15 14 15 + in N, which agrees with observations. The N/ N ratio in N2H is found to be close to the elemental value, in contrast to previous 15 + models that obtain a significant enrichment, because we found that the fractionation reaction between N and N2H has a barrier in + 15 + + 15 + the entrance channel. -
Modeling the Ice VI to VII Phase Transition
Modeling the Ice VI to VII Phase Transition Dawn M. King 2009 NSF/REU PROJECT Physics Department University of Notre Dame Advisor: Dr. Kathie E. Newman July 31, 2009 Abstract Ice (solid water) is found in a number of different structures as a function of temperature and pressure. This project focuses on two forms: Ice VI (space group P 42=nmc) and Ice VII (space group Pn3m). An interesting feature of the structural phase transition from VI to VII is that both structures are \self clathrate," which means that each structure has two sublattices which interpenetrate each other but do not directly bond with each other. The goal is to understand the mechanism behind the phase transition; that is, is there a way these structures distort to become the other, or does the transition occur through the breaking of bonds followed by a migration of the water molecules to the new positions? In this project we model the transition first utilizing three dimensional visualization of each structure, then we mathematically develop a common coordinate system for the two structures. The last step will be to create a phenomenological Ising-like spin model of the system to capture the energetics of the transition. It is hoped the spin model can eventually be studied using either molecular dynamics or Monte Carlo simulations. 1 Overview of Ice The known existence of many solid states of water provides insight into the complexity of condensed matter in the universe. The familiarity of ice and the existence of many structures deem ice to be interesting in the development of techniques to understand phase transitions. -
11Th International Conference on the Physics and Chemistry of Ice, PCI
11th International Conference on the Physics and Chemistry of Ice (PCI-2006) Bremerhaven, Germany, 23-28 July 2006 Abstracts _______________________________________________ Edited by Frank Wilhelms and Werner F. Kuhs Ber. Polarforsch. Meeresforsch. 549 (2007) ISSN 1618-3193 Frank Wilhelms, Alfred-Wegener-Institut für Polar- und Meeresforschung, Columbusstrasse, D-27568 Bremerhaven, Germany Werner F. Kuhs, Universität Göttingen, GZG, Abt. Kristallographie Goldschmidtstr. 1, D-37077 Göttingen, Germany Preface The 11th International Conference on the Physics and Chemistry of Ice (PCI- 2006) took place in Bremerhaven, Germany, 23-28 July 2006. It was jointly organized by the University of Göttingen and the Alfred-Wegener-Institute (AWI), the main German institution for polar research. The attendance was higher than ever with 157 scientists from 20 nations highlighting the ever increasing interest in the various frozen forms of water. As the preceding conferences PCI-2006 was organized under the auspices of an International Scientific Committee. This committee was led for many years by John W. Glen and is chaired since 2002 by Stephen H. Kirby. Professor John W. Glen was honoured during PCI-2006 for his seminal contributions to the field of ice physics and his four decades of dedicated leadership of the International Conferences on the Physics and Chemistry of Ice. The members of the International Scientific Committee preparing PCI-2006 were J.Paul Devlin, John W. Glen, Takeo Hondoh, Stephen H. Kirby, Werner F. Kuhs, Norikazu Maeno, Victor F. Petrenko, Patricia L.M. Plummer, and John S. Tse; the final program was the responsibility of Werner F. Kuhs. The oral presentations were given in the premises of the Deutsches Schiffahrtsmuseum (DSM) a few meters away from the Alfred-Wegener-Institute. -
2Growth, Structure and Properties of Sea
Growth, Structure and Properties 2 of Sea Ice Chris Petrich and Hajo Eicken 2.1 Introduction The substantial reduction in summer Arctic sea ice extent observed in 2007 and 2008 and its potential ecological and geopolitical impacts generated a lot of attention by the media and the general public. The remote-sensing data documenting such recent changes in ice coverage are collected at coarse spatial scales (Chapter 6) and typically cannot resolve details fi ner than about 10 km in lateral extent. However, many of the processes that make sea ice such an important aspect of the polar oceans occur at much smaller scales, ranging from the submillimetre to the metre scale. An understanding of how large-scale behaviour of sea ice monitored by satellite relates to and depends on the processes driving ice growth and decay requires an understanding of the evolution of ice structure and properties at these fi ner scales, and is the subject of this chapter. As demonstrated by many chapters in this book, the macroscopic properties of sea ice are often of most interest in studies of the interaction between sea ice and its environment. They are defi ned as the continuum properties averaged over a specifi c volume (Representative Elementary Volume) or mass of sea ice. The macroscopic properties are determined by the microscopic structure of the ice, i.e. the distribution, size and morphology of ice crystals and inclusions. The challenge is to see both the forest, i.e. the role of sea ice in the environment, and the trees, i.e. the way in which the constituents of sea ice control key properties and processes. -
A 4565 Myr Old Andesite from an Extinct Chondritic Protoplanet
A 4565 Myr old andesite from an extinct chondritic protoplanet. Jean-Alix Barrata*, Marc Chaussidonb, Akira Yamaguchic, Pierre Beckd, Johan Villeneuvee, David J. Byrnee, Michael W. Broadleye, Bernard Martye a Univ Brest, Institut Universitaire Européen de la Mer (IUEM), UMR 6539, Place Nicolas Copernic, F- 29280 Plouzané, France ;b Université de Paris, Institut de pHysique du globe de Paris, CNRS, F-75005 Paris;c National Institute of Polar ResearcH, Tokyo, 190-8518, Japan ;dUniversite Grenoble Alpes, CNRS, Institut de Planetologie et d’Astrophysique de Grenoble (IPAG), Saint-Martin d’Heres, France;e Université de Lorraine, CNRS, CRPG, F-54000 Nancy, France. *Corresponding autHor Jean-Alix Barrat Email: [email protected] Abstract The age of iron meteorites implies that accretion of protoplanets began during the first millions of years of the solar system. Due to the Heat generated by 26Al decay, many early protoplanets were fully differentiated, with an igneous crust produced during the cooling of a magma ocean, and the segregation at depth of a metallic core. The formation and nature of the primordial crust generated during the early stages of melting is poorly understood, due in part to the scarcity of available samples. The newly discovered meteorite Erg CHecH 002 (EC 002) originates from one sucH primitive igneous crust, and has an andesite bulk composition. It derives from the partial melting of a non-carbonaceous chondritic reservoir, witH no depletion in alkalis relative to the sun’s photosphere, and at a high melting rate of around 25%. Moreover, EC 002 is to date, the oldest known piece of an igneous crust witH a 26Al-26Mg crystallization age of 4565.0 Myr. -
And Tissue Perfusion Employing 2H20 As a Freely Diffusible Tracer (Rat Liver/Surface Coil/Spin-Lattice Relaxation/Heavy Water) JOSEPH J
Proc. Natl. Acad. Sci. USA Vol. 84, pp. 4099-4102, June 1987 Biophysics Deuterium nuclear magnetic resonance measurements of blood flow and tissue perfusion employing 2H20 as a freely diffusible tracer (rat liver/surface coil/spin-lattice relaxation/heavy water) JOSEPH J. H. ACKERMAN*t, COLEEN S. EwY*, NANCY N. BECKER*, AND ROBERT A. SHALWITZtt *Department of Pediatrics, Washington University School of Medicine, St. Louis, MO 63110; and *Department of Chemistry, Washington University, St. Louis, MO 63130 Communicated by William D. Phillips, January 28, 1987 ABSTRACT The use of deuterium oxide (21120) is pro- We propose herein the analogous use of 2H20 as a posed as a freely diffusible nuclear magnetic resonance (NMR) diffusible blood-flow and tissue-perfusion tracer where deu- blood flow and tissue perfusion tracer of potential clinical terium NMR is used to monitor label intensity as a function utility. Deuterium is a stable, nonradiative isotope commer- of time. Deuterium is a nonradiative, naturally abundant cially available as 2H20 at enrichment levels of essentially (0.0156%), quadrupole nuclide with only 0.01 the sensitivity 100%-i.e., 110 molar equivalent deuterium. This high con- of 'H. Nevertheless, the combination of an efficient centration, together with the short relaxation time of the spin quadrupole relaxation mechanism and the commercial avail- 1 (quadrupole) deuterium nuclide, provides substantial sensi- ability of 2H20, essentially 100% enriched to ca. 110 molar tivity for NMR spectroscopy. As a result, when 2H20 is equivalent deuterium, can provide substantial NMR signal- administered in a bolus fashion to a specific tissue or organ in to-noise in the intact subject.