Structural Polymorphism in “Kesterite” Cu2znsns4
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Mineral Processing
Mineral Processing Foundations of theory and practice of minerallurgy 1st English edition JAN DRZYMALA, C. Eng., Ph.D., D.Sc. Member of the Polish Mineral Processing Society Wroclaw University of Technology 2007 Translation: J. Drzymala, A. Swatek Reviewer: A. Luszczkiewicz Published as supplied by the author ©Copyright by Jan Drzymala, Wroclaw 2007 Computer typesetting: Danuta Szyszka Cover design: Danuta Szyszka Cover photo: Sebastian Bożek Oficyna Wydawnicza Politechniki Wrocławskiej Wybrzeze Wyspianskiego 27 50-370 Wroclaw Any part of this publication can be used in any form by any means provided that the usage is acknowledged by the citation: Drzymala, J., Mineral Processing, Foundations of theory and practice of minerallurgy, Oficyna Wydawnicza PWr., 2007, www.ig.pwr.wroc.pl/minproc ISBN 978-83-7493-362-9 Contents Introduction ....................................................................................................................9 Part I Introduction to mineral processing .....................................................................13 1. From the Big Bang to mineral processing................................................................14 1.1. The formation of matter ...................................................................................14 1.2. Elementary particles.........................................................................................16 1.3. Molecules .........................................................................................................18 1.4. Solids................................................................................................................19 -
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. -
Stannoidite Cu8(Fe, Zn)3Sn2s12 C 2001-2005 Mineral Data Publishing, Version 1 Crystal Data: Orthorhombic
Stannoidite Cu8(Fe, Zn)3Sn2S12 c 2001-2005 Mineral Data Publishing, version 1 Crystal Data: Orthorhombic. Point Group: 222. Massive, in veinlets, to 1 mm. Physical Properties: Fracture: Uneven to subconchoidal. Hardness = ∼4 VHN = 181–274 (100 g load). D(meas.) = n.d. D(calc.) = [4.68] Optical Properties: Opaque. Color: Brass-brown; in polished section, pinkish brown. Streak: Dark brown-gray. Luster: Metallic. Pleochroism: Distinct, pale salmon-brown to brown. Anisotropism: Strong; dark orange-red to yellow-gray. R1–R2: (400) 17.5–18.9, (420) 17.4–19.2, (440) 18.2–20.3, (460) 19.5–21.7, (480) 20.8–23.0, (500) 21.8–24.2, (520) 22.8–25.3, (540) 23.7–26.3, (560) 24.6–27.1, (580) 25.4–27.8, (600) 26.2–28.4, (620) 27.1–29.1, (640) 27.8–29.5, (660) 28.7–30.0, (680) 29.6–30.5, (700) 30.3–30.8 Cell Data: Space Group: I222. a = 10.767 b = 5.411 c = 16.118 Z = [2] X-ray Powder Pattern: Konjo mine, Japan. 3.11 (100), 1.906 (70), 1.621 (20b), 2.70 (16), 4.83 (10), 5.40 (5), 4.13 (4) Chemistry: (1) (2) (1) (2) Cu 37.2 38.2 Zn 1.2 0.8 Ag 0.1 Sn 16.5 18.7 Fe 12.5 11.9 S 31.2 29.9 Total 98.7 99.5 (1) Konjo mine, Japan; by electron microprobe, corresponding to (Cu7.22Ag0.01)Σ=7.23 (Fe2.76Zn0.23)Σ=2.99Sn1.71S12.00. -
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 University of Manitoba
THE OCCURRH\ICE OF TTN AT THE DtcKsroNE No. 2 oRBODY, NORTHmN IfANTTOBA by Marti:: Gray }4crcice Trliruli-peg, Manitoba Iftarcln, l97l+ A Thesis Submitted to the Faculty of Graduate SbudÍes and Research The University of Manitoba I:i Part,ial Fït]-fillrnent of the Requirements for the Degree of Master of Science ABSIRACT The Dickstone No. 2 Orebody, a sna1l massive sulphide deposít situated i¡r northern Ïvlanitoba, contain" lirl i¡ amou::ts averaging O"O8/" or 1o6 pounds per ton. ' Most of the tin occurs-as the oxide cassiterite. The cassiterite shows a considerable size range from (.OOI fiÍn. to 0o6 tmno, with approxÍ:nately 99% of a-ll cassiterite present Ín graÍns larger than Oo1 nm. acrossc_ The larger cassiterite grains e:dribit subhedral crystal forms, Some of which show the e'ffects of abrasion. Quafr'zt calcite and ' pyrite are most closely associated with the cassiterite u A microprobe study of the'cassiterites shows that the most connnon trace elem.e=nts are jndium, siJver, neod¡rmium, tur:gsten, iodine and lutetium. Ca1cíum, anti-rnony, and ytterbium occur moderately, whi-le titan-iran, iron, zi:rrc, tantalurn and iridium occur infrequently. Another tin-bearing rnineral was encour:teredo .Llthough not posÍtively identified, this mjneral ís a calcium-titanium silicate, possibly sphene" l-l_ ACKNOTìILEDGEMH\TS The uriter would like to thank Dro H. Du Bo lniilson for his help and supervision durirrg the preparation of this thesi-s. Aclcrow- ledgements are al-so exbended to Mro Ku RamJ-al- whose guidance dwi:rg the electron rnícroprobe phase of this study proved invaluable. -
Tungsten Minerals and Deposits
DEPARTMENT OF THE INTERIOR FRANKLIN K. LANE, Secretary UNITED STATES GEOLOGICAL SURVEY GEORGE OTIS SMITH, Director Bulletin 652 4"^ TUNGSTEN MINERALS AND DEPOSITS BY FRANK L. HESS WASHINGTON GOVERNMENT PRINTING OFFICE 1917 ADDITIONAL COPIES OF THIS PUBLICATION MAY BE PROCURED FROM THE SUPERINTENDENT OF DOCUMENTS GOVERNMENT PRINTING OFFICE WASHINGTON, D. C. AT 25 CENTS PER COPY CONTENTS. Page. Introduction.............................................................. , 7 Inquiries concerning tungsten......................................... 7 Survey publications on tungsten........................................ 7 Scope of this report.................................................... 9 Technical terms...................................................... 9 Tungsten................................................................. H Characteristics and properties........................................... n Uses................................................................. 15 Forms in which tungsten is found...................................... 18 Tungsten minerals........................................................ 19 Chemical and physical features......................................... 19 The wolframites...................................................... 21 Composition...................................................... 21 Ferberite......................................................... 22 Physical features.............................................. 22 Minerals of similar appearance................................. -
VEIN and GREISEN SN and W DEPOSITS (MODELS 15A-C; Cox and Bagby, 1986; Reed, 1986A,B) by James E. Elliott, Robert J. Kamilli, Wi
VEIN AND GREISEN SN AND W DEPOSITS (MODELS 15a-c; Cox and Bagby, 1986; Reed, 1986a,b) by James E. Elliott, Robert J. Kamilli, William R. Miller, and K. Eric Livo SUMMARY OF RELEVANT GEOLOGIC, GEOENVIRONMENTAL, AND GEOPHYSICAL INFORMATION Deposit geology Vein deposits consist of simple to complex fissure filling or replacement quartz veins, including discrete single veins, swarms or systems of veins, or vein stockworks, that contain mainly wolframite series minerals (huebnerite-ferberite) and (or) cassiterite as ore minerals (fig. 1). Other common minerals are scheelite, molybdenite, bismuthinite, base- etal sulfide minerals, tetrahedrite, pyrite, arsenopyrite, stannite, native bismuth, bismuthinite, fluorite, muscovite, biotite, feldspar, beryl, tourmaline, topaz, and chlorite (fig. 2). Complex uranium, thorium, rare earth element oxide minerals and phosphate minerals may be present in minor amounts. Greisen deposits consist of disseminated cassiterite and cassiterite-bearing veinlets, stockworks, lenses, pipes, and breccia (fig. 3) in gangue composed of quartz, mica, fluorite, and topaz. Veins and greisen deposits are found within or near highly evolved, rare-metal enriched plutonic rocks, especially near contacts with surrounding country rock; settings in or adjacent to cupolas of granitic batholiths are particularly favorable. Figure 1. Generalized longitudinal section through the Xihuashan and Piaotang tungsten deposits in the Dayu district, China. Other vein systems are indicated by heavy lines. I, upper limits of ore zones; II, lower limits of ore zones. Patterned area is granite batholith. Unpatterned area is sedimentary and metamorphic rocks (from Elliott, 1992). Figure 2. Maps and sections of tungsten vein deposits illustrating mineral and alteration zoning. A, Chicote Grande deposit, Bolivia; B, Xihuashan, China (from Cox and Bagby, 1986). -
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. -
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 -
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. -
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. -
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.