Gi{ORTER COMIAUNICATIONS a STANNITE-KESTERITE
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
MINERALOGY of EPITHERMAL GOLD SULFIDE TELLURIDE ORES of the KAIRAGACH GOLD DEPOSIT, (Uzbekistan)
#07_kovalenker_en_0802:#07_kovalenker_en_0802.qxd 21.05.2009 20:11 Page 45 New data on minerals. M.: 2003. Volume 38 45 UDC 553.43/451.498+553.662(575) MINERALOGY OF EPITHERMAL GOLDSULFIDETELLURIDE ORES OF THE KAIRAGACH GOLD DEPOSIT, (Uzbekistan) Vladimir A. Kovalenker Institute of Geology of Ore Deposits, Petrography, Mineralogy, and Geochemistry (IGEM), RAS, Moscow, [email protected] Olga Yu. Plotinskaya Institute of Geology of Ore Deposits, Petrography, Mineralogy, and Geochemistry (IGEM), RAS, Moscow, [email protected] Rustam I. Koneev Ulugbek National University of Uzbekistan, Tashkent, Republic of Uzbekistan The Kairagach ore deposit is situated on the northern slope of the Kurama Ridge (East Uzbekistan), 3.5 km northeast of the wellknown Kochbulak goldtelluride ore deposit. According to specific mineralogical fea- tures of the ores and hydrothermal alterations, it was assigned to the highsulfidation (or acidsulfate) type of epithermal mineralization. However, in contrast to typical gold deposits of this type with a pronounced AuCu specialization, the ores of the Kairagach deposit are characterized by the AuSnBiSeTe geochemical profile. This paper briefly summarizes original and published data on the Kairagach deposit, including its geological features and ore characteristics, sequence of the mineral formation, and the main mineral assemblages. Occurrence conditions and chemical peculiarities of the essential minerals of the goldsulfideselenidetelluride mineralization are considered. Data on the abundance and compositional vari- ations of native elements (gold, tellurium, and tin), fahlores, Bi and Sb sulfosalts, Cu and Fe sulfostannates, and various selenides and tellurides are presented. It is shown that the unique diversity of the ore mineralization is determined by the variety of state and occur- rence forms (native, isomorphous, sulfide, selenide, and telluride) of their contained chemical elements. -
1393R OMARINIITE, Cu8fe2znge2s12, THE
Title Omariniite, Cu8Fe2ZnGe2S12, the germanium analogue of stannoidite, a new mineral species from Capillitas, Argentina Authors Bindi, L; Putz, H; Paar, WH; Stanley, Christopher Description This is a pre-proof version Date Submitted 2017-09-29 1 1393R 2 3 OMARINIITE, Cu8Fe2ZnGe2S12, THE GERMANIUM-ANALOGUE OF 4 STANNOIDITE, A NEW MINERAL SPECIES FROM CAPILLITAS, 5 ARGENTINA 6 7 1,* 2 3 4 8 LUCA BINDI , HUBERT PUTZ , WERNER H. PAAR , CHRISTOPHER J. STANLEY 9 10 1Dipartimento di Science de la Terra, Università degli Studi di Firenze, Via G. La Pira, 4, I-50121 Firenze, 11 Italy and CNR – Istituto di Geoscienze e Georisorse, Sezione di Firenze, Via G. La Pira 4, I-50121 Firenze, 12 Italy 13 2Friedl ZT GmbH Rohstoff- und Umwelt Consulting, Karl-Lötsch-Strasse 10, A-4840 Vöcklabruck, Austria 14 3Pezoltgasse 46, A-5020 Salzburg, Austria 15 4Natural History Museum, Cromwell Road, London SW7 5BD, United Kingdom 16 *Corresponding Author: [email protected] 17 18 19 20 21 22 ABSTRACT 23 Omariniite, ideally Cu8Fe2ZnGe2S12, represents the Ge-analogue of stannoidite and was 24 found in bornite-chalcocite-rich ores near the La Rosario vein of the Capillitas epithermal 25 deposit, Catamarca Province, Argentina. The mineral is closely associated with three other 26 Ge-bearing minerals (putzite, catamarcaite, rarely zincobriartite) and bornite, chalcocite, 27 digenite, covellite, sphalerite, tennantite, luzonite, wittichenite, thalcusite and traces of 28 mawsonite. The width of the seams rarely exceeds 60 µm, their length can attain several 29 100 µm’s. The mineral is opaque, orange-brown in polished section, has a metallic luster 30 and a brownish-black streak. -
Indium Crystal Chemistry : from Thin-Film Materials * Id
• • • INDIUM CRYSTAL CHEMISTRY : FROM THIN-FILM MATERIALS IN Poster TO NATURAL BULK CHALCOGENIDES * ID 229 * Laboratório Nacional de Energia e Geologia Ma Ondina FIGUEIREDO & Teresa PEREIRA da SILVA LNEG, Geol. Data C., Apt. 7586, 2721-866 Alfragide, & CENIMAT / I3N, Mat. Crystal Chemistry of Indium Sci. Dpt., Fac. Sci. Techn., New Univ. Lisbon, 2829-516 Caparica, Portugal Indium (Z=49) has the electronic structure [Kr] 4d10 5s2 5p1 and frequently assumes the trivalent state, suggesting the inertness of 5s2 electron-pair. Like gallium and unlike tin, indium seldom forms specific minerals, exhibiting a Introduction Table 1 − MORPHOTROPIC DOMAINS of distinctly chalcophile behavior in the Earth’s crust and occurring rather Indium is nowadays widely used in many CHALCOGENIDE MINERALS (Sulphides & Sulphosalts) dispersed within polymetallic sulfide ores (Table 1). technologic fields - electronics, solders, low [chemical range for stable diadochic substitutions in minerals The sulphide roquesite (CuInS2) was the first In-mineral to be described [5], melting-temperature alloys, etc. Discovered in deduced from stable synthetic compounds] followed [6] by indite (Fe In2 S4) and dzhalindite, a tri-hydroxide with In (OH)6 1863 and isolated four years later as a metal, octahedra. The recovery of indium stands mostly on the processing of zinc indium became one of the most relevant scarce Periodic classification of the Elements blende - a cubic mineral typifying tetrahedral sulphides (fig.2) where cations fill metals used in the production of new “high-tech half of the available tetrahedral sites in a cubic closest packing (ccp) of sulfur devices” based on innovative nanotechnologies. anions (S=). The crystal-chemical formula is written Znt[St]c, where t stands Suggestive examples of indium incorporation - S for tetrahedral coordination and c quotes the anion packing [7]. -
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. -
Indium-Bearing Paragenesis from the Nueva Esperanza and Restauradora Veins, Capillitas Mine, Argentina
Journal of Geosciences, 65 (2020), 97–109 DOI: 10.3190/jgeosci.304 Original paper Indium-bearing paragenesis from the Nueva Esperanza and Restauradora veins, Capillitas mine, Argentina María Florencia MÁRQUEZ-ZAVALÍA1,2*, Anna VYMAZALOVÁ3, Miguel Ángel GALLISKI1, Yasushi WATANABE4, Hiroyasu MURAKAMI5 1 IANIGLA, CCT-Mendoza (CONICET), Avda. A. Ruiz Leal s/n, Parque San Martin, CC330, (5500) Mendoza, Argentina; [email protected] 2 Mineralogía y Petrología, FAD, Universidad Nacional de Cuyo, Centro Universitario (5502) Mendoza, Argentina 3 Department of Rock Geochemistry, Czech Geological Survey, Geologická 6, 152 00 Prague 5, Czech Republic 4 Faculty of International Resource Sciences, Mining Museum of Akita University, 28-2 Osawa, Tegata, Akita, 010-8502 Japan 5 Coal Business Planning Group, Coal Business Office, Resources & Power Company, JXTG Nippon Oil & Energy Corporation, 1-2, Otemachi 1-chome, Chiyoda-ku, Tokyo 100-8162 Japan * Corresponding author The Nueva Esperanza and Restauradora are two of the twenty-three veins described at Capillitas mine, an epithermal precious- and base-metal vein deposit located in northern Argentina. Capillitas is genetically linked to other minera- lizations of the Farallón Negro Volcanic Complex, which hosts several deposits. These include two world-class (La Alumbrera and Agua Rica) and some smaller (e.g., Bajo El Durazno) porphyry deposits, and a few epithermal deposits (Farallón Negro, Alto de la Blenda, Cerro Atajo and Capillitas). The main hypogene minerals found at these two ve- ins include pyrite, sphalerite, galena, chalcopyrite, tennantite-(Zn) and tennantite-(Fe). Accessory minerals comprise hübnerite, gold, silver, stannite, stannoidite and mawsonite, and also diverse indium- and tellurium-bearing minerals. -
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. -
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 -
Copper Hyper-Stoichiometry: the Key for the Optimization Of
Copper Hyper-Stoichiometry: The Key for the Optimization of Thermoelectric Properties in Stannoidite Cu8+xFe3–xSn2S12 Ventrapati Pavan Kumar, Tristan Barbier, Vincent Caignaert, Bernard Raveau, Ramzy Daou, Bernard Malaman, Gérard Le Caër, Pierric Lemoine, Emmanuel Guilmeau To cite this version: Ventrapati Pavan Kumar, Tristan Barbier, Vincent Caignaert, Bernard Raveau, Ramzy Daou, et al.. Copper Hyper-Stoichiometry: The Key for the Optimization of Thermoelectric Properties in Stannoidite Cu8+xFe3–xSn2S12. Journal of Physical Chemistry C, American Chemical Society, 2017, 121 (30), pp.16454-16461. 10.1021/acs.jpcc.7b02068. hal-01580457 HAL Id: hal-01580457 https://hal-univ-rennes1.archives-ouvertes.fr/hal-01580457 Submitted on 14 Sep 2017 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Page 1 of 36 The Journal of Physical Chemistry 1 2 3 4 5 6 7 8 Copper Hyper-stoichiometry, the Key for the 9 10 11 12 Optimization of Thermoelectric Properties in 13 14 15 16 Stannoidite Cu 8+ xFe 3-xSn 2S12 17 18 19 20 21 † † † † 22 Ventrapati Pavan Kumar, Tristan Barbier, Vincent Caignaert, Bernard Raveau, Ramzy 23 24 † ‡ # § ,† 25 Daou, Bernard Malaman, Gérard Le Caër, Pierric Lemoine, and Emmanuel Guilmeau * 26 27 28 † 29 Laboratoire CRISMAT, UMR 6508 CNRS/ENSICAEN, 6 bd du Marechal Juin, 14050 Caen 30 31 32 Cedex 4, France 33 34 35 ‡ 36 Institut Jean Lamour, UMR 7198, CNRS, Université de Lorraine, Faculté des Sciences et 37 38 Technologie, B.P. -
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.