Ice XV: a New Thermodynamically Stable Phase of Ice
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Proton Ordering and Reactivity of Ice
1 Proton ordering and reactivity of ice Zamaan Raza Department of Chemistry University College London Thesis submitted for the degree of Doctor of Philosophy September 2012 2 I, Zamaan Raza, confirm that the work presented in this thesis is my own. Where information has been derived from other sources, I confirm that this has been indicated in the thesis. 3 For Chryselle, without whom I would never have made it this far. 4 I would like to thank my supervisors, Dr Ben Slater and Prof Angelos Michaelides for their patient guidance and help, particularly in light of the fact that I was woefully unprepared when I started. I would also like to express my gratitude to Dr Florian Schiffmann for his indispens- able advice on CP2K and quantum chemistry, Dr Alexei Sokol for various discussions on quantum mechanics, Dr Dario Alfé for his incredibly expensive DMC calculations, Drs Jiri Klimeš and Erlend Davidson for advice on VASP, Matt Watkins for help with CP2K, Christoph Salzmann for discussions on ice, Dr Stefan Bromley for allowing me to work with him in Barcelona and Drs Aron Walsh, Stephen Shevlin, Matthew Farrow and David Scanlon for general help, advice and tolerance. Thanks and also apologies to Stephen Cox, with whom I have collaborated, but have been unable to contribute as much as I should have. Doing a PhD is an isolating experience (more so in the Kathleen Lonsdale building), so I would like to thank my fellow students and friends for making it tolerable: Richard, Tiffany, and Chryselle. Finally, I would like to acknowledge UCL for my funding via a DTA and computing time on Legion, the Materials Chemistry Consortium (MCC) for computing time on HECToR and HPC-Europa2 for the opportunity to work in Barcelona. -
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. -
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. -
Electromagnetism Based Atmospheric Ice Sensing Technique - a Conceptual Review
Int. Jnl. of Multiphysics Volume 6 · Number 4 · 2012 341 Electromagnetism based atmospheric ice sensing technique - A conceptual review Umair N. Mughal*, Muhammad S. Virk and M. Y. Mustafa High North Technology Center Department of Technology, Narvik University College, Narvik, Norway ABSTRACT Electromagnetic and vibrational properties of ice can be used to measure certain parameters such as ice thickness, type and icing rate. In this paper we present a review of the dielectric based measurement techniques for matter and the dielectric/spectroscopic properties of ice. Atmospheric Ice is a complex material with a variable dielectric constant, but precise calculation of this constant may form the basis for measurement of its other properties such as thickness and strength using some electromagnetic methods. Using time domain or frequency domain spectroscopic techniques, by measuring both the reflection and transmission characteristics of atmospheric ice in a particular frequency range, the desired parameters can be determined. Keywords: Atmospheric Ice, Sensor, Polar Molecule, Quantum Excitation, Spectroscopy, Dielectric 1. INTRODUCTION 1.1. ATMOSPHERIC ICING Atmospheric icing is the term used to describe the accretion of ice on structures or objects under certain conditions. This accretion can take place either due to freezing precipitation or freezing fog. It is primarily freezing fog that causes this accumulation which occurs mainly on mountaintops [16]. It depends mainly on the shape of the object, wind speed, temperature, liquid water content (amount of liquid water in a given volume of air) and droplet size distribution (conventionally known as the median volume diameter). The major effects of atmospheric icing on structure are the static ice loads, wind action on iced structure and dynamic effects. -
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, 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. -
© Cambridge University Press Cambridge
Cambridge University Press 978-0-521-80620-6 - Creep and Fracture of Ice Erland M. Schulson and Paul Duval Index More information Index 100-year wave force, 336 friction and fracture, 289, 376 60° dislocations, 17, 82, 88 indentation failure, 345 microstructure, 45, 70, 237, 255, 273 abrasion, 337 multiscale fracture and frictional accommodation processes of basal slip, 165 sliding, 386 acoustic emission, 78, 90, 108 nested envelopes, 377 across-column cleavage cracks, 278 pressure–area relationship, 349, 352 across-column confinement, 282 S2 growth texture, 246, 273 across-column cracks, 282, 306, SHEBA faults, 371 across-column loading, 275 SHEBA stress states, 377 across-column strength, 246, 249, 275 Arctic Ocean, 1, 45, 190, 361 activation energy, 71, 84, 95, 111, 118, 131 aspect ratio, 344 activation volume, 114, 182 atmospheric ice, 219, 221, 241, 243 activity of pyramidal slip systems, 158 atmospheric icing, 31 activity of slip systems, 168 atmospheric impurities, 113 adiabatic heating, 291, 348 atomic packing factor, 9 adiabatic softening, 291 audible report, 240 affine self-consistent model, 160 avalanches, 206 air bubbles, 38 air-hydrate crystals, 37 bands, 89 albedo, 363 basal activity, 162 aligned first-year sea ice, 246 basal dislocations, 77 along-column confinement, 282 basal planes, 214, along-column confining stress, 282, basal screw dislocations, 77, 87 along-column strength, 244, 275 basal shear bands, 163 ammonia dihydrate, 181 basal slip, 18, 77, 127, 228 ammonia–water system, 186 basal slip lines, 77 amorphous forms -
The Everlasting Hunt for New Ice Phases ✉ Thomas C
COMMENT https://doi.org/10.1038/s41467-021-23403-6 OPEN The everlasting hunt for new ice phases ✉ Thomas C. Hansen 1 Water ice exists in hugely different environments, artificially or naturally occurring ones across the universe. The phase diagram of crystalline phases of ice is still under construction: a high-pressure phase, ice XIX, has just been 1234567890():,; reported but its structure remains ambiguous. Water is the molecule that makes our planet so special and gives it its nickname, the blue planet. Liquid water is the medium for any form of life on Earth and is considered to be a sine qua non- condition for life on any place in our universe. Ice, the solid phase of water, has always been in the focus of science. It was maybe even ice, that was a necessary substrate for first life on Earth to emerge1; Therefore, it is normal to be very curious about all possible structures of water ices under different conditions—twenty crystalline and further amorphous forms are now known to exist (Fig. 1). ’ Ice Ih, hexagonal ice, is the only form relevant to the Earth s environmental conditions, as even the thickest ice slabs do not provide the necessary pressure to pass it into high-pressure poly- 2 3,4 morphs. However, so-called cubic ice, ice Ic, only very recently isolated in pure form , plays a role at very low temperatures in the higher atmosphere in the nucleation of ice5; ice VI, the lowest high-pressure ice phase at room temperature has been spectroscopically found in dia- mond inclusions6, and ice VII has been speculated to be present on Earth in cold subduction zones7. -
Gibbs Energy of Ices III, V and VI: Wholistic Thermodynamics and Elasticity of the Water Phase Diagram to 2300 Mpa. 1. Abstract
Gibbs energy of ices III, V and VI: wholistic thermodynamics and elasticity of the water phase diagram to 2300 MPa. B. Journaux*1, J.M. Brown1, A. Pakhomova2, I. E. Collings3,4, S. Petitgirard5, P. Espinoza1, J. Ott1,6, F. Cova3,7, G. Garbarino3, M. Hanfland3 1. Abstract: Gibbs energy representations for ice III, V and VI are reported. These were constructed using new measurements of volumes at high pressure over a range of low temperatures combined with calculated vibrational energies grounded in statistical physics. The collection of representations including ice Ih and water (released as the open source “SeaFreeze” framework) allow accurate determinations of thermodynamics properties (phase boundaries, density, heat capacity, bulk modulus, thermal expansivity, chemical potentials) and seismic wave velocities over the entire range of conditions encountered in hydrospheres in our solar system (220-500K to 2300 MPa). These comprehensive representations allow exploration of the rich spectrum of thermodynamic behavior in the H2O system. Although the results are broadly applicable in science and engineering, their use in habitability analysis in water-rich planetary bodies of our solar system and beyond is particularly relevant. 2. Introduction Water is a fundamentally important molecule in scientific fields ranging from biology to engineering, earth and environmental sciences, chemistry or astrophysics. As a common molecular species in our cosmic neighborhood, water ice polymorphs at high pressures in planetary interiors could be the most abundant “mineral group” in the Universe (Hanslmeier 2011). A focus on potentially habitable icy moons and ocean exoplanets hydrospheres (Sotin and Tobie 2004; Vance and Brown 2013; Journaux et al. -
X-Ray Study of Ice and Water on Surfaces and in Aqueous Solutions
X-RAY STUDY OF ICE AND WATER ON SURFACES AND IN AQUEOUS SOLUTIONS A DISSERTATION SUBMITTED TO THE DEPARTMENT OF CHEMISTRY AND THE COMMITTEE ON GRADUATE STUDIES OF STANFORD UNIVERSITY IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF DOCTOR OF PHILOSOPHY Iradwikanari Waluyo March 2011 © 2011 by Iradwikanari Waluyo. All Rights Reserved. Re-distributed by Stanford University under license with the author. This dissertation is online at: http://purl.stanford.edu/dt235bn2603 ii I certify that I have read this dissertation and that, in my opinion, it is fully adequate in scope and quality as a dissertation for the degree of Doctor of Philosophy. Anders Nilsson, Primary Adviser I certify that I have read this dissertation and that, in my opinion, it is fully adequate in scope and quality as a dissertation for the degree of Doctor of Philosophy. Hans Andersen I certify that I have read this dissertation and that, in my opinion, it is fully adequate in scope and quality as a dissertation for the degree of Doctor of Philosophy. Christopher Chidsey Approved for the Stanford University Committee on Graduate Studies. Patricia J. Gumport, Vice Provost Graduate Education This signature page was generated electronically upon submission of this dissertation in electronic format. An original signed hard copy of the signature page is on file in University Archives. iii Abstract Since antiquity, water has been considered as the most important substance on Earth. In fact, the abundance of liquid water on this planet allowed for the emergence and evolution of life. At the molecular level, the structure of an individual water molecule may seem simple; however, the intermolecular interaction between water molecules in the form of hydrogen bonding gives rise to water’s various properties that can be considered anomalous when compared to other liquids.