DOCSLIB.ORG

GROWTH and PROPERTIES of BULK Cztsse and Sb2se3 for SOLAR CELLS

Total Page：16

File Type：pdf, Size：1020Kb

Download full-text PDF Read full-text
GROWTH and PROPERTIES of BULK Cztsse and Sb2se3 for SOLAR CELLS GROWTH AND PROPERTIES OF BULK CZTSSe AND Sb2Se3 FOR SOLAR CELLS Theodore Douglas Christopher Hobson Thesis submitted in accordance with the requirements of the UNIVERSITY OF LIVERPOOL For the degree of DOCTOR IN PHILOSOPHY Stephenson Institute for Renewable Energy Department of Physics May 2020 For Holly Abstract This thesis presents investigations into growth techniques to produce bulk polycrystalline and single crystals of the materials Cu2ZnSnS4xSe4(1-x) (CZTSSe) and Sb2Se3, in order to better understand bulk properties of relevance for photovoltaics. For CZTSSe, a technique to grow ~100 μm monograins from a molten NaCl/KCl mix proved successful for compositions 0 ≤ x ≤ 1 in increments of Δx = 0.1, with a more ordered kesterite phase demonstrated compared to directly synthesised feedstock. From this series, Vegard relations were measured as: a (Å) = -0.268(3)x + 5.6949(17) and c (Å) = - 0.516(6)x + 11.345(3) while Raman modes were observed to follow two-mode behaviour as: ωCZTSe -1 -1 (cm ) = (44.6 ± 1.6)x + (194.6 ± 0.8) and ωCZTS (cm ) = (7.1 ± 1.3)x + (329.0 ± 0.8). These relationships are intended to be used as reference data to aid the measurement of sulphur-selenium ratios in CZTSSe thin films. Samples consistent with single crystals of Sb2Se3 with 4 mm diameter and 1 cm length were grown via vertical Bridgman, with the {100} crystal planes evidenced through optical means and XRD. These crystals exhibited low-angle boundary defects consistent with ripplocations. They also demonstrated anisotropies in the polarised Raman spectra, with sample rotation able to resolve the overlapping 187 and 190 cm-1 peaks. The 253 cm-1 peak in the Raman spectra was consistent with reports of Sb2O3. Se-poor and stoichiometric Sb2Se3 single crystals were non-conductive, while Se-rich were p-type, and Sn and Cl were found to induce p-type and n-type doping respectively, with a maximum hole density from Sn-doping of 1015 cm-3 and electron density 17 -3 from Cl of 10 cm . Barrier heights of 0.37 eV for p-Sb2Se3 / In interfaces and 0.56 eV for n-Sb2Se3 / Au interfaces were estimated. Deep level electron traps at 400, 700 and 850 meV were detected in n- type single crystals, thought to result from VSe and VSe defects, while photoluminescence peaks at 0.9, 1.1 and 1.2 eV were assigned to donor-acceptor pair transitions resulting from Sn and Cl impurities. Thermally evaporated thin film Sb2Se3 / CdS solar cells were prepared from n-type, intrinsic and p- type doped source material, all reaching ~1 % efficiency. Of these, the p-type devices decreased in efficiency after ageing in air, while the intrinsic and n-type increased slightly, possibly due to Sb2O3 formation from oxidisation. i Declarations All of the measurements presented in this thesis were carried out by the author apart from the following, separated by institution: Stephenson Institute for Renewable Energy, University of Liverpool: 1. Oliver S Hutter: a. Collaborated with the author on the synthesis of CZTSSe feedstock and growth of crystallised solid solutions series (Sections 4.2.1, 4.2.3, 5.2.1, 5.2.2 and 5.2.3) b. Carried out differential scanning calorimetry of NaCl/KCl mix (fig. 4.1) and CZTSSe feedstock series (fig. 5.2) c. Prepared Sb2Se3 thin films by CSS (Section 4.3.5) and air-annealed them (Section 6.6.5.1) d. Carried out SEM for several samples (figs. 5.1, 6.4 and 7.19) 2. Jonathan D Major: a. Sputtered CdS layer and deposited thermally evaporated Sb2Se3 layers for thin film devices (Sections 4.3.7 and 7.7) b. Carried out deep-level transient spectroscopy measurements (fig. 7.12) 3. Nicole Fleck carried out Raman measurements of the crystallised CZTSSe solid solution series (0 ≤ x ≤ 1) (figs. 5.11 and 5.12a) Other departments at the University of Liverpool: 1. EBSD by Elisabetta Mariani in the Dept. of Earth, Ocean and Ecological Sciences (figs. 6.16a-c) 2. ICP-OES by Stephen Moss in analytical services at the Dept. of Chemistry (Table 5.2, figs. 5.3 and 5.4, Table 6.5) Other institutions: 1. ICP-MS by Chris Ottley and Emily Unsworth in the Department of Earth Sciences at the University of Durham (Table 6.6) 2. Quadrupole SIMS by Guillaume Zoppi in the Dept. of Mathematics, Physics and Electrical Engineering at the University of Northumbria (fig. 6.19) 3. Hall effect by Bhaskar Das in the Chemical Engineering and Materials Science Department at the University of Minnesota (fig. 7.3, Table 7.3) 4. Photoluminescence by Maarja Grossberg, Tavi Raadik and Juri Krustok at the Department of Materials Science at the Tallinn University of Technology (figs. 7.14a and 7.15) ii Acknowledgements I have had the privilege of working with colleagues who are both great scientists and great friends. I have learnt so much from the people around me that I can’t possibly relate all the ways in which they have made this work possible. I’ll simply start by saying it has been a pleasure to collaborate with Oliver Hutter, Nicole Fleck, Huw Shiel, Laurie Philips, Leanne Jones, Tom Featherstone, Matt Smiles, Jack Swallow, Sylvia Mariotti, Isabel Vazquez-Fernandez, Luke Daniels and Holly Edwards to produce work I feel we should all be very proud of. The same goes for my many other collaborators both inside and outside the University of Liverpool. You have all been a joy to work with. However, the work that makes up this thesis would also not have been possible without the invaluable help and assistance of Phil Murgatroyd, Tom Shalvey, Jessica Stoner, Tom Baines, Max Birkett, Annette Pressman, Joe Horne, Peter Yates, Manuel Apollo and Luke Thomas. There’s no way I’ve repaid even half of the help you’ve given me over the years. It’s not just direct collaboration that makes a PhD, and all of my colleagues have been brilliant people to spend time with both inside and outside the lab, making the Stephenson Institute an exciting and friendly place to work. I want to offer additional thanks to Leanne and Nicole for being wonderful desk-mates and making our end of the office the ‘cool corner’, at least in my mind. Having Tom F around to chat was another thing that made be glad to be where I was, and along with Jack Beane, provided a welcome excuse for me to wander around the office. Thanks to Olivia Voyce for always encouraging us to be better people and to Daniel Bromley and Alex Wright for standing up for the rights of students. Thanks to Joe for injecting humour into our lunchtimes and being an unbeatable fountain of trivia, and thanks to Phil for always being there to help me out, whatever the issue. Thanks to Holly for being a great CZTS bestie and to Hatem Amli for brightening up the office. Thanks to Oliver for teaching me a little of what he knows and most of what I know, even if not all the facts were what I’d consider ‘fun’. Thanks to Laurie for being an essential beacon of competence while the rest of us are bumbling around. Thanks to Tom B for introducing me to some iii great music, and to Matt for picking up the dad-joke baton after Tom went over to the dark side. Thanks also to Luke for leading the SIRE football team to victory (the first time) and to Jacob for organising games under lockdown that helped keep me sane. Thanks to Huw for reminding us that there’s more to life than work, Jack S for always having a great sense of humour and Tom S for putting up with all of us. Thanks to Pete, Sylvia and Annette for making me feel welcome when I first started. I also want to thank Bruna Baggio, Angeline Kasina, Kieran Routledge, Mark Forster, Gaia Neri, Stefano Mensa, Charlotte Smith, Liam Banerji, Daniel Cheung and Khezar Saeed for all helping to make the Institute the fun and social place it is. It goes without saying that I need to thank my supervisors Ken Durose and Jon Major for their support and encouragement as much as for their sympathy and patience with me. Thanks are always due to Vince Vasey for keeping the whole lab ticking over and I owe a great thanks to Tim Veal, Dmitry Schkukin, Jon Alaria, Frank Jaeckel, Vin Dhanak and Laurence Hardwick for all their help and for trusting me with their equipment. I want to thank my examiners Liam O’Brien and David Lane for their helpful discussions and feedback. Thanks also need to go to my parents Kate Hobson and Hugh Pearman, my brother Ben, sisters Harriet and Lydia and all my friends in other places. To my oldest friends Joe Drane, Ayla Richardson, Roman Sheppard-Dawson and Sophie Wolfson, I owe a great thanks. I want to thank Holly Gilson for being my wonderful and constant partner in all things. This work was finished during a difficult time for many people, and all I can do is say thank you to all my friends and family, and to wish you all the very best. This work, like me, is better for me having known all of you. iv Contents Abstract ................................................................................................................................................... i Declarations ........................................................................................................................................... ii Acknowledgements .............................................................................................................................. iii 1. Introduction ....................................................................................................................................... 1 1.1 Context for Photovoltaics.............................................................................................................. 1 1.2 Motivation for Researching CZTSSe and Sb2Se3 ......................................................................... 3 1.3 Structure of this Thesis ................................................................................................................. 9 1.4 References ................................................................................................................................... 10 2. Literature Review of CZTSSe and Sb2Se3 in Photovoltaics .......................................................
Load more

Recommended publications
  • CZTS) Phases Rameez Ahmad,1 Marco Brandl,2 Monica Distaso,1 Patrick Herre,1,3 Erdmann Spiecker,3 Rainer Hock 2 and Wolfgang Peukert 1* *[email protected] 1
    CrystEngComm Accepted Manuscript This is an Accepted Manuscript, which has been through the Royal Society of Chemistry peer review process and has been accepted for publication. Accepted Manuscripts are published online shortly after acceptance, before technical editing, formatting and proof reading. Using this free service, authors can make their results available to the community, in citable form, before we publish the edited article. We will replace this Accepted Manuscript with the edited and formatted Advance Article as soon as it is available. You can find more information about Accepted Manuscripts in the Information for Authors. Please note that technical editing may introduce minor changes to the text and/or graphics, which may alter content. The journal’s standard Terms & Conditions and the Ethical guidelines still apply. In no event shall the Royal Society of Chemistry be held responsible for any errors or omissions in this Accepted Manuscript or any consequences arising from the use of any information it contains. www.rsc.org/crystengcomm Page 1 of 24 CrystEngComm A comprehensive study on the mechanism behind formation and depletion of Cu 2ZnSnS 4 (CZTS) phases Rameez Ahmad,1 Marco Brandl,2 Monica Distaso,1 Patrick Herre,1,3 Erdmann Spiecker,3 Rainer Hock 2 and Wolfgang Peukert 1* *[email protected] 1. Institute of Particle Technology, Friedrich-Alexander-Universität Erlangen-Nürnberg (FAU), Cauerstrasse 4, 91058 Erlangen, Germany 2. Chair for Crystallography and Structural physics, Friedrich-Alexander-Universität Erlangen-Nürnberg (FAU), Staudtstr. 3, 91058 Erlangen, Germany 3. Center for Nanoanalysis and Electron Microscopy (CENEM), Friedrich-Alexander-Universität Erlangen- Nürnberg (FAU), Cauerstraße 6, 91058 Erlangen, Germany Manuscript Abstract High efficiency kesterite based solar cells have vigorously raised the research interests in this material.
    [Show full text]
  • Molecular Solution Processing of Metal Chalcogenide Thin Film Solar Cells
    UNIVERSITY OF CALIFORNIA Los Angeles Molecular solution processing of metal chalcogenide thin film solar cells A dissertation submitted in partial satisfaction of the requirements for the degree Doctor of Philosophy in Materials Science and Engineering by Wenbing Yang 2013 Abstract of the Dissertation Molecular solution processing of metal chalcogenide thin film solar cells by Wenbing Yang Doctor of Philosophy in Materials Science and Engineering University of California, Los Angeles, 2013 Professor Yang Yang, Chair The barrier to utilize solar generated electricity mainly comes from their higher cost relative to fossil fuels. However, innovations with new materials and processing techniques can potentially make cost effective photovoltaics. One such strategy is to develop solution processed photovoltaics which avoid the expensive vacuum processing required by traditional solar cells. The dissertation is mainly focused on two absorber material system for thin film solar cells: chalcopyrite CuIn(S,Se) 2 (CISS) and kesterite Cu 2ZnSn(S,Se) 4 organized in chronological order. Chalcopyrite CISS is a very promising material. It has been demonstrated to achieve the highest efficiency among thin film solar cells. Scaled-up industry production at present has reached the giga-watt per year level. The process however mainly relies on vacuum systems which account for a significant percentage of the manufacturing cost. In the first section of this dissertation, hydrazine based solution processed CISS has been explored. The focus of the research involves the procedures to fabricate devices from solution. The topics covered in Chapter 2 include: precursor solution synthesis with a focus on understanding the solution chemistry, CISS absorber formation from precursor, properties modification toward favorable device performance, and device structure innovation toward tandem device.
    [Show full text]
  • Alphabetical List
    LIST L - MINERALS - ALPHABETICAL LIST Specific mineral Group name Specific mineral Group name acanthite sulfides asbolite oxides accessory minerals astrophyllite chain silicates actinolite clinoamphibole atacamite chlorides adamite arsenates augite clinopyroxene adularia alkali feldspar austinite arsenates aegirine clinopyroxene autunite phosphates aegirine-augite clinopyroxene awaruite alloys aenigmatite aenigmatite group axinite group sorosilicates aeschynite niobates azurite carbonates agate silica minerals babingtonite rhodonite group aikinite sulfides baddeleyite oxides akaganeite oxides barbosalite phosphates akermanite melilite group barite sulfates alabandite sulfides barium feldspar feldspar group alabaster barium silicates silicates albite plagioclase barylite sorosilicates alexandrite oxides bassanite sulfates allanite epidote group bastnaesite carbonates and fluorides alloclasite sulfides bavenite chain silicates allophane clay minerals bayerite oxides almandine garnet group beidellite clay minerals alpha quartz silica minerals beraunite phosphates alstonite carbonates berndtite sulfides altaite tellurides berryite sulfosalts alum sulfates berthierine serpentine group aluminum hydroxides oxides bertrandite sorosilicates aluminum oxides oxides beryl ring silicates alumohydrocalcite carbonates betafite niobates and tantalates alunite sulfates betekhtinite sulfides amazonite alkali feldspar beudantite arsenates and sulfates amber organic minerals bideauxite chlorides and fluorides amblygonite phosphates biotite mica group amethyst
    [Show full text]
  • Phase Diagram of the Selenide Kesterite Photovoltaic Materials and NMR Investigation of Cu/Zn Disorder in Cztse
    Electronic Supplementary Material (ESI) for Physical Chemistry Chemical Physics. This journal is © the Owner Societies 2015 Phase diagram of the selenide kesterite photovoltaic materials and NMR investigation of Cu/Zn disorder in CZTSe Léo Choubrac, Alain Lafond, Michaël Paris, Catherine Guillot-Deudon and Stephane Jobic Electronic Supporting Information Experimental Synthesis The compounds were prepared by the solid state reaction of Cu, Zn, Sn, and S powders in the appropriate ratios in evacuated, sealed, fused silica tubes. They were heated at 750 °C (ramp 300 °C/h) for 170 h and then cooled down at 20 °C/h. The obtained powders were then ground and pressed into pellets which were again put into a sealed tube. The second heating sequence was: ramp 300 °C/h; plateau 750 °C; cooling ramp 50 °C/h. For some samples, attention was paid to the cooling mode at the end of the heating process. Samples were heated at 350 °C for 2 days and subsequently ice-quenched (sample A2Q). A part of the obtained samples was reheated at 350 °C for 2 days, slow cooled down to 150°C (2 °C/h), annealed at this temperature for 1 day and finally slow cooled to room temperature. For example, from sample A2 (see Table 1) we got sample A2Q (quenched) and sample A2S (slow cooled). X-ray diffraction The powder X-ray diffraction patterns of the studied samples were measured on a D8-Bruker advance diffractometer ( = 1.540596 Å), equipped with a LynxEye detector, in the 8-100 ° 2 range with a 0.011 ° 2- step and a record time of 0.4 s/step.
    [Show full text]
  • Eijun OHTA* the Toyoha Mine Is Located 40 Km South
    MINING GEOLOGY,39(6),355•`372,1989 Occurrence and Chemistry of Indium-containing Minerals from the Toyoha Mine, Hokkaido, Japan Eijun OHTA* Abstract: Toyoha lead-zinc-silver vein-type deposit in Hokkaido, Japan produces an important amount of indium as well as tin and copper. Bismuth, tungsten, antimony, arsenic, and cobalt are minor but common metals. Indium minerals recognized are; unnamed Zn-In mineral (hereafter abbreviated as ZI) whose composition is at the midst of sphalerite and roquesite, unnamed Ag-In mineral (AI) of AglnS2 composition, roquesite (RQ) and sakuraiite. Observed maximum weight percentages of indium in chalcopyrite, kesterite (KS) and stannite are 1.0, 1.86 and 20.0, respectively. Indium concentration in sphalerite ranges from O.On to a few weight percent in most case, but exceeds ten weight percent at some points. Detailed EPMA analyses have revealed that such high concentration is attributed to a continuous solid solution between sphalerite (SP) and ZI. Continuous solid solutions between RQ90ZI10 and RQ37ZI69, and between KS100ZI0 and KS30ZI70 are also detected. These solid solutions are attributed to coupled substitutions of 2(Zn, Fe) for CuIn, and of (Zn, Fe)In for CuSn. Other substitutions found between chalcopyrite and stannite and between stannite/kesterite and roquesite are of (Fe+2, Zn)Sn for 2Fe+3 and of (Fe+2, Zn)Sn for 2In respectively. Economically most important indium carriers in Toyoha are ZI and indium-bearing sphalerite. Next to sphalerite are kesterite, stannite and the anisotropic chalcopyrite. The occurrence of these minerals indicates that these minerals have been formed by pulsatile mineralization whose peak temperatures were 50 to 100•Ž higher than the hitherto estimated maximum formation temperature, about 300•Ž, of the deposit.
    [Show full text]
  • Synthesis and Structural Characterization of Semiconductors Based on Kesterites
    Synthesis and Structural Characterization of Semiconductors based on Kesterites vorgelegt von Anna Ritscher, Bakk.rer.nat M.Sc. aus Villach, Österreich von der Fakultät II - Mathematik und Naturwissenschaften der Technischen Universität Berlin zur Erlangung des akademischen Grades Doktorin der Naturwissenschaften - Dr.rer.nat. - genehmigte Dissertation Promotionsausschuss: Vorsitzende: Prof. Dr. Regine von Klitzing Gutachter: Prof. Dr. Martin Lerch Gutachter: Prof. Dr. Manfred Mühlberg Tag der wissenschaftlichen Aussprache: 28.10.2016 Berlin, 2016 “There is a theory which states that if ever anyone discovers exactly what the Universe is for and why it is here, it will instantly disappear and be replaced by something even more bizarre and inexplicable. There is another theory mentioned, which states that this has already happened.” Douglas Adams, The Hitchhiker’s Guide to the Galaxy Abstract The here-presented thesis provides detailed investigations on the structural characteris- tics of the chalcogenide Cu2ZnSnS4 (CZTS). This semiconductor material is a promising candidate for absorber layers in solar cells due to its desirable properties for thin film photovoltaic applications. Yet, compared to current used chalcopyrite-based devices, effi- ciencies are significantly lower. This could be attributed to structural effects. Fundamental understanding of the structural characteristics of potential thin film absorber compounds is crucial for proper materials design in the field of solar technology. Therefore, intensive research is necessary to obtain knowledge on so far unexplored structural features or to certify and extend current literature data. The main objective of the here-presented work was to deepen the understanding of the quaternary sulfide 2Cu ZnSnS4. Primary, this implied the full characterization of structural properties of the compound using various diffraction techniques.
    [Show full text]
  • Mineralogy of Sulfides
    This is a repository copy of Mineralogy of sulfides. White Rose Research Online URL for this paper: http://eprints.whiterose.ac.uk/113362/ Version: Published Version Article: Vaughan, D.J. and Corkhill, C.L. orcid.org/0000-0002-7488-3219 (2017) Mineralogy of sulfides. Elements , 13 (2). pp. 81-87. ISSN 1811-5209 https://doi.org/10.2113/gselements.13.2.81 Reuse This article is distributed under the terms of the Creative Commons Attribution (CC BY) licence. This licence allows you to distribute, remix, tweak, and build upon the work, even commercially, as long as you credit the authors for the original work. More information and the full terms of the licence here: https://creativecommons.org/licenses/ Takedown If you consider content in White Rose Research Online to be in breach of UK law, please notify us by emailing [email protected] including the URL of the record and the reason for the withdrawal request. [email protected] https://eprints.whiterose.ac.uk/ Mineralogy of Sulfides David J. Vaughan1 and Claire L. Corkhill2 1811-5209/17/0013-0081$2.50 DOI: 10.2113/gselements.13.2.81 etal sulfides are the most important group of ore minerals. Here, we The literature on sulfide minerals review what is known about their compositions, crystal structures, is extensive, with a number of overview textbooks and Mphase relations and parageneses. Much less is known about their monographs. Comprehensive surface chemistry, their biogeochemistry, or the formation and behaviour of reviews can be found in Ribbe ‘nanoparticle’ sulfides, whether formed abiotically or biogenically.
    [Show full text]
  • Cornish Mineral Reference Manual
    Cornish Mineral Reference Manual Peter Golley and Richard Williams April 1995 First published 1995 by Endsleigh Publications in association with Cornish Hillside Publications © Endsleigh Publications 1995 ISBN 0 9519419 9 2 Endsleigh Publications Endsleigh House 50 Daniell Road Truro, Cornwall TR1 2DA England Printed in Great Britain by Short Run Press Ltd, Exeter. Introduction Cornwall's mining history stretches back 2,000 years; its mineralogy dates from comparatively recent times. In his Alphabetum Minerale (Truro, 1682) Becher wrote that he knew of no place on earth that surpassed Cornwall in the number and variety of its minerals. Hogg's 'Manual of Mineralogy' (Truro 1825) is subtitled 'in wich [sic] is shown how much Cornwall contributes to the illustration of the science', although the manual is not exclusively based on Cornish minerals. It was Garby (TRGSC, 1848) who was the first to offer a systematic list of Cornish species, with locations in his 'Catalogue of Minerals'. Garby was followed twenty-three years later by Collins' A Handbook to the Mineralogy of Cornwall and Devon' (1871; 1892 with addenda, the latter being reprinted by Bradford Barton of Truro in 1969). Collins followed this with a supplement in 1911. (JRIC Vol. xvii, pt.2.). Finally the torch was taken up by Robson in 1944 in the form of his 'Cornish Mineral Index' (TRGSC Vol. xvii), his amendments and additions were published in the same Transactions in 1952. All these sources are well known, but the next to appear is regrettably much less so. it would never the less be only just to mention Purser's 'Minerals and locations in S.W.
    [Show full text]
  • Understanding the Effects of Cd and Ag Doping in Cu2znsns4 Solar Cells
    Article Cite This: Chem. Mater. 2018, 30, 4543−4555 pubs.acs.org/cm ff Understanding the E ects of Cd and Ag Doping in Cu2ZnSnS4 Solar Cells Gopalakrishnan Sai Gautam,† Thomas P. Senftle,†,§ and Emily A. Carter*,‡ † ‡ Department of Mechanical and Aerospace Engineering and School of Engineering and Applied Science, Princeton University, Princeton, New Jersey 08544-5263, United States *S Supporting Information ABSTRACT: Cu2ZnSnS4-based solar cells, which constitute an inex- pensive, beyond-Si photovoltaic technology, often suffer from low open- circuit voltage and efficiency. This drawback is often attributed to disorder in the Cu−Zn sublattice of the kesterite structure. While previous experiments have reported improved performances with isovalent substitution of Cd and Ag for Cu and Zn, respectively, the fundamental driving force for such improvements remains unclear. Here, we use density functional theory to study bulk stability, defect, and surface energetics, as fi well as the electronic structure of these dopants in Cu2ZnSnS4.We nd that Cd and Ag can increase efficiencies, depending on the dopant concentration and Cu content used during synthesis. Most importantly, we find that a low level of Cd doping can suppress disorder in the kesterite phase across all Cu concentrations, while a low level of Ag doping can do so only when Zn- and Sn-rich conditions are employed. A higher Ag content is beneficial as it stabilizes the kesterite structure, whereas a higher Cd content is detrimental as it stabilizes the lower- fi fl gap stannite structure. Cd does not signi cantly in uence the surface energetics of kesterite Cu2ZnSnS4. Ag, on the other hand, decreases the surface energies significantly, which would favor smaller particle sizes.
    [Show full text]
  • An Example of Miocene Epithermal Ag-Zn-Pb-Sn Mineralization in the Andean Tin Belt
    The Cortaderas Zone, Pirquitas Mine, NW Argentina: An Example of Miocene Epithermal Ag-Zn-Pb-Sn Mineralization in the Andean Tin Belt by Evan Thomas Slater A thesis submitted in partial fulfillment of the requirements for the degree of Master of Science (MSc) in Geology The Faculty of Graduate Studies Laurentian University Sudbury, Ontario, Canada © Evan Slater, 2016 THESIS DEFENCE COMMITTEE/COMITÉ DE SOUTENANCE DE THÈSE Laurentian Université/Université Laurentienne Faculty of Graduate Studies/Faculté des études supérieures Title of Thesis Titre de la thèse The Cortaderas Zone, Pirquitas Mine, NW Argentina: An Example of Miocene Epithermal Ag-Zn-Pb-Sn Mineralization in the AnActing Dean Tin Belt Name of Candidate Nom du candidat Slater, Evan Degree Diplôme Master of Science Department/Program Date of Defence Département/Programme Geology Date de la soutenance September 7, 2016 APPROVED/APPROUVÉ Thesis Examiners/Examinateurs de thèse: Dr. Daniel Kontak (Supervisor/Directeur(trice) de thèse) Dr. Andy McDonald (Co-supervisor/Co-directeur(trice) de thèse) Dr. Michael Schindler (Committee member/Membre du comité) Approved for the Faculty of Graduate Studies Approuvé pour la Faculté des études supérieures Dr. Shelley Watson Madame Shelley Watson Dr. Marcos Zentilli Acting Dean, Faculty of Graduate Studies (External Examiner/Examinateur externe) Doyenne intérimaire, Faculté des études supérieures ACCESSIBILITY CLAUSE AND PERMISSION TO USE I, Evan Slater, hereby grant to Laurentian University and/or its agents the non-exclusive license to archive and make accessible my thesis, dissertation, or project report in whole or in part in all forms of media, now or for the duration of my copyright ownership.
    [Show full text]
  • Copper-Lead-Zinc Mineralization at the Hayakawa and Shakako Deposits 343
    J. Min. Peter. Econ. Geol. 85, 341-353, 1990 Copper-lead-zinc mineralization at the Hayakawa and Shakako deposits, Jokoku-Katsuraoka mining area , southwestern Hokkaido, Japan DAIZO ISHIYAMA*, HIROHARU MATSUEDA** and OSAMU MATSUBAYA*** * Institute of Mining Geology , Mining College, Akita University, Akita 010, Japan ** Department of Geology and Mineralogy , Faculty of Science, Hokkaido University, Sapporo 060, Japan *** Research Institute of Natural Resources , Mining College, Akita University, Akita 010, Japan This paper summarizes macrostructures of individual ore bodies, mineral assemblages, mineralization stages, and oxygen isotopic data for quartz from veins and wall rock for copper- lead-zinc mineralization at the Hayakawa and Shakako deposits. Chalcopyrite-pyrite-tetrahedrite-galena-sphalerite-bearing quartz veins (Cu-Pb-Zn quartz veins) and galena-sphalerite-bearing quartz veins (Pb-Zn quartz veins) occur at the Hayakawa and Shakako deposits. The Cu-Pb-Zn quartz veins formed earlier than the Pb-Zn quartz veins. The minerals in the Cu-Pb-Zn quartz veins include chalcopyrite, pyrite, tetrahedrite-tennantite, galena, sphalerite, enargite, bournonite, semseyite, hessite, kesterite, arsenosulvanite, Cu-Fe-Zn- Sn-S mineral, tetradymite, aikinite, quartz and apatite. The minerals in the Pb-Zn quartz veins are galena, sphalerite, pyrite, chalcopyrite, tetrahedrite, electrum and quartz. FeS content of sphalerite decreases from the earlier to later stages of mineralization. Distinct compositional heterogeneity between Sb and As is recognized within a grain of tetrahedrite-tennantite. The ƒÂ18O values for quartz in Cu-Pb-Zn quartz veins at the Hayakawa deposit range from 1.4 to 3.1 per mil. The value for quartz in Cu-Pb-Zn-quartz veins at the Shakako deposit is 1.9 per mil.
    [Show full text]
  • Point Defects, Compositional Fluctuations, and Secondary Phases
    J. Phys.: Energy 2 (2020) 012002 https://doi.org/10.1088/2515-7655/ab4a25 TOPICAL REVIEW Point defects, compositional fluctuations, and secondary phases OPEN ACCESS in non-stoichiometric kesterites RECEIVED 8 April 2019 Susan Schorr1,2 , Galina Gurieva1 , Maxim Guc3,4 , Mirjana Dimitrievska3,5,6, REVISED Alejandro Pérez-Rodríguez3,7, Victor Izquierdo-Roca3, Claudia S Schnohr8 , Juran Kim9, William Jo9 and 23 May 2019 José Manuel Merino10 ACCEPTED FOR PUBLICATION 2 October 2019 1 Department Structure and Dynamics of Energy Materials, Helmholtz-Zentrum Berlin fuer Materialien und Energie, Hahn-Meitner-Platz PUBLISHED 1, 14109 Berlin, Germany 2 10 December 2019 Institute of Geosciences, Freie Universität Berlin, Malteserstr. 74-100, 12449 Berlin, Germany 3 Catalonia Institute for Energy Research (IREC), Jardins de les Dones de Negre 1, 08930 Sant Adrià de Besòs, Spain 4 Institute of Applied Physics, Academiei str. 5, MD 2023 Chisinau, Moldova Original content from this 5 work may be used under NIST Center forNeutron Research, National Institute of Standards and Technology, Gaithersburg, MD 20899-6102, United States of America 6 the terms of the Creative National Renewable Energy Laboratory, Golden, CO 80401, United States of America Commons Attribution 3.0 7 IN2UB, Departament d’Enginyeria Electrònica i Biomèdica, Universitat de Barcelona, C. Martí i Franquès 1, 08028 Barcelona, Spain licence. 8 Felix Bloch Institute for Solid State Physics, Leipzig University, Linnéstraße 5, 04103 Leipzig, Germany Any further distribution of 9 Department of Physics, Ewha Womans University, Seoul 03760, Republic of Korea this work must maintain 10 Faculty of Science, Universidad Autonóma de Madrid, Ciudad Universitaria de Cantoblanco C/Francisco Tomás y Valiente 7, 28049 attribution to the author(s) and the title of Madrid, Spain the work, journal citation E-mail: [email protected] and DOI.
    [Show full text]