Waterts Second Glass Transition
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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. -
Indiana Glaciers.PM6
How the Ice Age Shaped Indiana Jerry Wilson Published by Wilstar Media, www.wilstar.com Indianapolis, Indiana 1 Previiously published as The Topography of Indiana: Ice Age Legacy, © 1988 by Jerry Wilson. Second Edition Copyright © 2008 by Jerry Wilson ALL RIGHTS RESERVED 2 For Aaron and Shana and In Memory of Donna 3 Introduction During the time that I have been a science teacher I have tried to enlist in my students the desire to understand and the ability to reason. Logical reasoning is the surest way to overcome the unknown. The best aid to reasoning effectively is having the knowledge and an understanding of the things that have previ- ously been determined or discovered by others. Having an understanding of the reasons things are the way they are and how they got that way can help an individual to utilize his or her resources more effectively. I want my students to realize that changes that have taken place on the earth in the past have had an effect on them. Why are some towns in Indiana subject to flooding, whereas others are not? Why are cemeteries built on old beach fronts in Northwest Indiana? Why would it be easier to dig a basement in Valparaiso than in Bloomington? These things are a direct result of the glaciers that advanced southward over Indiana during the last Ice Age. The history of the land upon which we live is fascinating. Why are there large granite boulders nested in some of the fields of northern Indiana since Indiana has no granite bedrock? They are known as glacial erratics, or dropstones, and were formed in Canada or the upper Midwest hundreds of millions of years ago. -
Genesis and Geographical Aspects of Glaciers - Vladimir M
HYDROLOGICAL CYCLE – Vol. IV - Genesis and Geographical Aspects of Glaciers - Vladimir M. Kotlyakov GENESIS AND GEOGRAPHICAL ASPECTS OF GLACIERS Vladimir M. Kotlyakov Institute of Geography, Russian Academy of Sciences, Moscow, Russia Keywords: Chionosphere, cryosphere, equilibrium line, firn line, glacial climate, glacier, glacierization, glaciosphere, ice, seasonal snow line, snow line, snow-patch Contents 1. Introduction 2. Properties of natural ice 3. Cryosphere, glaciosphere, chionosphere 4. Snow-patches and glaciers 5. Basic boundary levels of snow and ice 6. Measures of glacierization 7. Occurrence of glaciers 8. Present-day glacierization of the Arctic Glossary Bibliography Biographical Sketch Summary There exist ten crystal variants of ice and one amorphous form in Nature, however only one form ice-1 is distributed on the Earth. Ten other ice variants steadily exist only under a certain combinations of pressure, specific volume and temperature of medium, and those are not typical for our planet. The ice density is less than that of water by 9%, and owing to this water reservoirs are never totally frozen., Thus life is sustained in them during the winter time. As a rule, ice is much cleaner than water, and specific gas-ice compounds called as crystalline hydrates are found in ice. Among the different spheres surrounding our globe there are cryosphere (sphere of the cold), glaciosphere (sphere of snow and ice) and chionosphere (that part of the troposphere where the annual amount of solid precipitation exceeds their losses). The chionosphere envelopes the Earth with a shell 3 to 5 km in thickness. In the present epoch, snow and ice cover 14.2% of the planet’s surface and more than half of the land surface. -
Case Fil Copy
NASA TECHNICAL NASA TM X-3511 MEMORANDUM CO >< CASE FIL COPY REPORTS OF PLANETARY GEOLOGY PROGRAM, 1976-1977 Compiled by Raymond Arvidson and Russell Wahmann Office of Space Science NASA Headquarters NATIONAL AERONAUTICS AND SPACE ADMINISTRATION • WASHINGTON, D. C. • MAY 1977 1. Report No. 2. Government Accession No. 3. Recipient's Catalog No. TMX3511 4. Title and Subtitle 5. Report Date May 1977 6. Performing Organization Code REPORTS OF PLANETARY GEOLOGY PROGRAM, 1976-1977 SL 7. Author(s) 8. Performing Organization Report No. Compiled by Raymond Arvidson and Russell Wahmann 10. Work Unit No. 9. Performing Organization Name and Address Office of Space Science 11. Contract or Grant No. Lunar and Planetary Programs Planetary Geology Program 13. Type of Report and Period Covered 12. Sponsoring Agency Name and Address Technical Memorandum National Aeronautics and Space Administration 14. Sponsoring Agency Code Washington, D.C. 20546 15. Supplementary Notes 16. Abstract A compilation of abstracts of reports which summarizes work conducted by Principal Investigators. Full reports of these abstracts were presented to the annual meeting of Planetary Geology Principal Investigators and their associates at Washington University, St. Louis, Missouri, May 23-26, 1977. 17. Key Words (Suggested by Author(s)) 18. Distribution Statement Planetary geology Solar system evolution Unclassified—Unlimited Planetary geological mapping Instrument development 19. Security Qassif. (of this report) 20. Security Classif. (of this page) 21. No. of Pages 22. Price* Unclassified Unclassified 294 $9.25 * For sale by the National Technical Information Service, Springfield, Virginia 22161 FOREWORD This is a compilation of abstracts of reports from Principal Investigators of NASA's Office of Space Science, Division of Lunar and Planetary Programs Planetary Geology Program. -
Searching for Crystal-Ice Domains in Amorphous Ices
PHYSICAL REVIEW MATERIALS 2, 075601 (2018) Searching for crystal-ice domains in amorphous ices Fausto Martelli,1,2,* Nicolas Giovambattista,3,4 Salvatore Torquato,2 and Roberto Car2 1IBM Research, Hartree Centre, Daresbury WA4 4AD, United Kingdom 2Department of Chemistry, Princeton University, Princeton, New Jersey 08544, USA 3Department of Physics, Brooklyn College of the City University of New York, Brooklyn, New York 11210, USA 4The Graduate Center of the City University of New York, New York, New York 10016, USA (Received 7 May 2018; published 2 July 2018) Weemploy classical molecular dynamics simulations to investigate the molecular-level structure of water during the isothermal compression of hexagonal ice (Ih) and low-density amorphous (LDA) ice at low temperatures. In both cases, the system transforms to high-density amorphous ice (HDA) via a first-order-like phase transition. We employ a sensitive local order metric (LOM) [F. Martelli et al., Phys. Rev. B 97, 064105 (2018)] that can discriminate among different crystalline and noncrystalline ice structures and is based on the positions of the oxygen atoms in the first- and/or second-hydration shell. Our results confirm that LDA and HDA are indeed amorphous, i.e., they lack polydispersed ice domains. Interestingly, HDA contains a small number of domains that are reminiscent of the unit cell of ice IV,although the hydrogen-bond network (HBN) of these domains differs from the HBN of ice IV. The presence of ice-IV-like domains provides some support to the hypothesis that HDA could be the result of a detour on the HBN rearrangement along the Ih-to-ice-IV pressure-induced transformation. -
Evasive Ice X and Heavy Fermion Ice XII: Facts and Fiction About High
Physica B 265 (1999) 113—120 Evasive ice X and heavy fermion ice XII: facts and fiction about high-pressure ices W.B. Holzapfel* Fachbereich Physik, Universita( t-GH Paderborn, D-33095 Paderborn, Germany Abstract Recent theoretical and experimental results on the structure and dynamics of ice in wide regions of pressure and temperature are compared with earlier models and predictions to illustrate the evasive nature of ice X, which was originally introduced as completely ordered form of ice with short single centred hydrogen bonds isostructural CuO. Due to the lack of experimental information on the proton ordering in the pressure and temperature region for the possible occurrence of ice X, effects of thermal and quantum delocalization are discussed with respect to the shape of the phase diagram and other structural models consistent with present optical and X-ray data for this region. Theoretical evidences for an additional orthorhombic modification (ice XI) at higher pressures are confronted with various reasons supporting a delocalization of the protons in the form of a heavy fermion system with very unique physical properties characterizing this fictitious new phase of ice XII. ( 1999 Elsevier Science B.V. All rights reserved. Keywords: Ices; Hydrogen bonds; Phase diagram; Equation of states 1. Introduction tunnelling [2]. Detailed Raman studies on HO and DO ice VIII to pressures in the range of The first in situ X-ray studies on HO and DO 50 GPa [3] revealed the expected softening in the ice VII under pressures up to 20 GPa [1] together molecular stretching modes and led to the deter- with a simple twin Morse potential (TMP) model mination of a critical O—H—O bond length of " for protons or deuterons in hydrogen bonds [2] R# 232 pm, where the central barrier of the effec- allowed almost 26 years ago first speculations tive double-well potential should disappear [4]. -
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. -
Properties of Ices at 0 K: a Test of Water Models J
THE JOURNAL OF CHEMICAL PHYSICS 127, 154518 ͑2007͒ Properties of ices at 0 K: A test of water models J. L. Aragones, E. G. Noya, J. L. F. Abascal, and C. Vega Departamento de Química Física, Facultad de Ciencias Químicas, Universidad Complutense, 28040 Madrid, Spain ͑Received 9 July 2007; accepted 27 July 2007; published online 19 October 2007͒ The properties of ices Ih, II, III, V, and VI at zero temperature and pressure are determined by computer simulation for several rigid water models ͑SPC/E, TIP5P, TIP4P/Ice, and TIP4P/2005͒. The energies of the different ices at zero temperature and pressure ͑relative to the ice II energy͒ are compared to the experimental results of Whalley ͓J. Chem. Phys. 81, 4087 ͑1984͔͒. TIP4P/Ice and TIP4P/2005 provide a qualitatively correct description of the relative energies of the ices at these conditions. In fact, only these two models provide the correct ordering in energies. For the SPC/E and TIP5P models, ice II is the most stable phase at zero temperature and pressure whereas for TIP4P/Ice and TIP4P/2005 ice Ih is the most stable polymorph. These results are in agreement with the relative stabilities found at higher temperatures. The solid-solid phase transitions at 0 K are determined. The predicted pressures are in good agreement with those obtained from free energy calculations. © 2007 American Institute of Physics. ͓DOI: 10.1063/1.2774986͔ I. INTRODUCTION 20th century, starting with the pioneering work of Tammann and Bridgman16–21 up to the recent discovery of ices XII, Taking into account the importance of water, it is not XIII, and XIV.22,23 Compared to the liquid, the study of ices surprising that thousands of simulation studies of water have by computer simulation has been more limited. -
Ice Molecular Model Kit © Copyright 2015 Ryler Enterprises, Inc
Super Models Ice Molecular Model Kit © Copyright 2015 Ryler Enterprises, Inc. Recommended for ages 10-adult ! Caution: Atom centers and vinyl tubing are a choking hazard. Do not eat or chew model parts. Kit Contents: 50 red 4-peg oxygen atom centers (2 spares) 100 white hydrogen 2-peg atom centers (2 spares) 74 clear, .87”hydrogen bonds (2 spares) 100 white, .87” covalent bonds (2 spares) Related Kits Available: Chemistry of Water Phone: 806-438-6865 E-mail: [email protected] Website: www.rylerenterprises.com Address: 5701 1st Street, Lubbock, TX 79416 The contents of this instruction manual may be reprinted for personal use only. Any and all of the material in this PDF is the sole property of Ryler Enterprises, Inc. Permission to reprint any or all of the contents of this manual for resale must be submitted to Ryler Enterprises, Inc. General Information Ice, of course, ordinarily refers to water in the solid phase. In the terminology of astronomy, an ice can be the solid form of any element or compound which is usually a liquid or gas. This kit is designed to investigate the structure of ice formed by water. Fig. 1 Two water molecules bonded by a hydrogen bond. Water ice is very common throughout the universe. According to NASA, within our solar system ice is The symbol δ means partial, so when a plus sign is found in comets, asteroids, and several moons of added, the combination means partial positive the outer planets, and it has been located in charge. The opposite obtains when a negative sign interstellar space as well. -
Ice, Ice, Bambino September 8, 2020 1 / 45 Chemistry: 18 Shades of Ice
ICE Chemistry It gets bigger when it freezes! Biology Inupiaq (Alaska) have 100 Stuff lives in it in ice cores! Astrobiology names for ice! Enceladus? Climatology Albedo and Negative feedback Snowball Earth Astrophysics Clear at optical and also radio frequencies Ice as a good cosmic-ray target Cosmic-ray collisions with ice molecules visible from km-scale distances Dave Besson Ice, Ice, Bambino September 8, 2020 1 / 45 Chemistry: 18 Shades of Ice Terrestrial (familiar) ice: ”Ice 1h” 1996: Ice XII discovered 2006: Ice XIII and Ice XIV 2009: Ice XV found extremely high pressures and 143 C. At P>1.55×1012Pa (10M atm) ice!metal Ice, water, and water vapor coexist at the ‘triple point’: 273.16 K (0.01 C) at P=611.657 Pa. 1◦ ≡1/273.16 of difference b/w triple point and absolute zero (this defn will change in May 2019) Dave Besson Ice, Ice, Bambino September 8, 2020 2 / 45 Oddly, ρice < ρwater The fact that ice remains on top of water is what prevents lakes and rivers from freezing upwards from below! Dave Besson Ice, Ice, Bambino September 8, 2020 3 / 45 Socio-Cultural impact: Refrigeration, Curling, Marvel’s Iceman (2015-17) Refrigeration: 400 BC: Persian engineers carve ice in winter and store in 5000 m3 insulated (via ‘sarooj’ - sand, clay, egg whites, lime, goat hair, and ash) caverns in desert during summer Dave Besson Ice, Ice, Bambino September 8, 2020 4 / 45 Why is ice clear (blue) Dave Besson Ice, Ice, Bambino September 8, 2020 5 / 45 and snow white? and implications for climate.. -
The Water Polymorphism and the Liquid–Liquid Transition from Transport Data
Article The Water Polymorphism and the Liquid–Liquid Transition from Transport Data Francesco Mallamace 1,2,* , Domenico Mallamace 3 , Giuseppe Mensitieri 4 , Sow-Hsin Chen 1 , Paola Lanzafame 3 and Georgia Papanikolaou 3 1 Department of Nuclear Science and Engineering, Massachusetts Institute of Technology, Cambridge, MA 02139, USA; [email protected] 2 CNR ISC, UOS Roma Sapienza, Physics Department, Sapienza University of Rome, 00185 Roma, Italy 3 Departments of ChiBioFarAm Section of Industrial Chemistry, University of Messina, CASPE-INSTM, V.le F. Stagno d’Alcontres 31, 98166 Messina, Italy; [email protected] (D.M.); [email protected] (P.L.); [email protected] (G.P.) 4 Department of Chemical, Materials and Industrial Production Engineering, University of Naples Federico II, P.le Tecchio 80, 80125 Napoli, Italy; [email protected] * Correspondence: [email protected]; Tel.: +39-340-233-5213 Abstract: NMR spectroscopic literature data are used, in a wide temperature-pressure range (180–350 K and 0.1–400 MPa), to study the water polymorphism and the validity of the liquid–liquid transition (LLT) hypothesis. We have considered the self-diffusion coefficient DS and the reorientational correlation time tq (obtained from spin-lattice T1 relaxation times), measured, respectively, in bulk and emulsion liquid water from the stable to well inside the metastable supercooled region. As an effect of the hydrogen bond (HB) networking, the isobars of both these transport functions evolve with T by changing by several orders of magnitude, whereas their pressure dependence Citation: Mallamace, F.; Mallamace, become more and more pronounced at lower temperatures. Both these transport functions were D.; Mensitieri, G.; Chen, S.-H.; Lanzafame, P.; Papanikolaou, G. -
Mechanical Characterization Via Full Atomistic Simulation: Applications to Nanocrystallized Ice
Mechanical Characterization via Full Atomistic Simulation: Applications to Nanocrystallized Ice A thesis presented By Arvand M.H. Navabi to The Department of Civil and Environmental Engineering in partial fulfillment of the requirements for the degree of Master of Science in the field of Civil Engineering Northeastern University Boston, Massachusetts August, 2016 Submitted to Prof. Steven W. Cranford Acknowledgements I acknowledge generous support from my thesis advisor Dr. Steven W. Cranford whose encouragement and availability was crucial to this thesis and also my parents for allowing me to realize my own potential. The simulations were made possible by LAMMPS open source program. Visualization has been carried out using the VMD visualization package. 3 Abstract This work employs molecular dynamic (MD) approaches to characterize the mechanical properties of nanocrystalline materials via a full atomistic simulation using the ab initio derived ReaxFF potential. Herein, we demonstrate methods to efficiently simulate key mechanical properties (ultimate strength, stiffness, etc.) in a timely and computationally inexpensive manner. As an illustrative example, the work implements the described methodology to perform full atomistic simulation on ice as a material platform, which — due to its complex behavior and phase transitions upon pressure, heat exchange, energy transfer etc. — has long been avoided or it has been unsuccessful to ascertain its mechanical properties from a molecular perspective. This study will in detail explain full atomistic MD methods and the particulars required to correctly simulate crystalline material systems. Tools such as the ReaxFF potential and open-source software package LAMMPS will be described alongside their fundamental theories and suggested input methods to simulate further materials, encompassing both periodic and finite crystalline models.