987 resultados para Bismuth sulfide


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Exploring high-performance anode materials is currently one of the most urgent issues towards practical sodium-ion batteries (SIBs). In this work, Bi2S3 is demonstrated to be a high-capacity anode for SIBs for the first time. The specific capacity of Bi2S3 nanorods achieves up to 658 and 264 mAh g-1 at a current density of 100 and 2000 mA g-1, respectively. A full cell with Na3V2(PO4)3-based cathode is also assembled as a proof of concept and delivers 340 mAh g-1 at 100 mA g-1. The sodium storage mechanism of Bi2S3 is investigated by ex-situ XRD coupled with high-resolution TEM (HRTEM), and it is found that sodium storage is achieved by a combined conversion-intercalation mechanism.

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One new homoleptic Bi(dtc)(3)] (1) (dtc = 4-hydroxypiperdine dithiocarbamate) has been synthesized and characterized by microanalysis, IR, UV-Vis, H-1 and C-13 spectroscopy and X-ray crystallography. The photoluminescence spectrum for the compound in DMSO solution was recorded. The crystal structure of 1 displayed distorted octahedral geometry around the Bi(III) center bonded through sulfur atoms of the dithiocarbamate ligands. TGA indicates that the compound decomposes to a Bi and Bi-S phase system. The Bi and Bi-S obtained from decomposition of the compound have been characterized by pXRD, EDAX and SEM. Solvothermal decomposition of 1 in the absence and presence of two different capping agents yielded three morphologically different Bi2S3 systems which were deployed as counter-electrode in dye-sensitized solar cells (DSSCs). (C) 2015 Elsevier B.V. All rights reserved.

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Beneficial effects of carbon grafting into the iron active material for rechargeable alkaline-iron-electrodes with and without Bi2S3 additive is probed by in situ X-ray diffraction in conjunction with Extended X-ray Absorption Fine Structure (EXAFS) and electrochemistry. EXAFS data unravel that the composition of pristine active material (PAM) for iron electrodes comprises 87% of magnetite and 13% of alpha-iron while carbon-grafted active material comprises 60% of magnetite and 40% of alpha-iron. In situ XRD patterns are recorded using a specially designed electrochemical cell. XRD data reflect that magnetite present in PAM iron electrode, without bismuth sulfide additive, is not reduced during charging while PAM iron electrode with bismuth sulfide additive is partially reduced to alpha-Fe/Fe(OH)(2). Interestingly, carbon-grafted-iron electrodes with bismuth sulfide exhibit complete conversion of active material to alpha-Fe/Fe(OH)2. The ameliorating effect of carbon grafting is substantiated by kinetic parameters obtained from steady-state potentiostatic polarization and Tafel plots. The mechanism for iron-electrode charge - discharge reactions are discussed in the light of the potential - pH diagrams for Fe - H2O, S - H2O and FeSads - H2O systems and it is surmised that carbon grafting into iron active material promotes its electrochemical utilization. (C) The Author(s) 2015. Published by ECS. All rights reserved.

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Single crystalline Bi2S3 With various morphologies (wires, rods, and flowers) has been successfully prepared via a simple polyol solution process and characterized by X-ray diffraction (XRD), field emission scanning electron microscopy (FESEM), and transmission electron microscopy (TEM) techniques. The morphologies of Bi2S3 crystals are highly dependent on the experimental parameters, including the reaction temperature, reactant ratio, sulfur source, and additive. The adjustment of these parameters can lead to an obvious shape evolution of products, and the growth mechanism has been proposed.

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Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

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Angesichts der sich abzeichnenden Erschöpfung fossiler Ressourcen ist die Erforschung alternativer Energiequellen derzeit eines der meistbeachteten Forschungsgebiete. Durch ihr enormes Potential ist die Photovoltaik besonders im Fokus der Wissenschaft. Um großflächige Beschichtungsverfahren nutzen zu können, wird seit einigen Jahren auf dem Gebiet der Dünnschichtphotovoltaik intensiv geforscht. Jedoch sind die gegenwärtigen Solarzellenkonzepte allesamt durch die Verwendung giftiger (Cd, As) oder seltener Elemente (In, Ga) oder durch eine komplexe Phasenbildung in ihrem Potential beschränkt. Die Entwicklung alternativer Konzepte erscheint daher naheliegend.rnAufgrund dessen wurde in einem BMBF-geförderten Verbundprojekt die Abscheidung von Dünnschichten des binären Halbleiters Bi2S3 mittels physikalischer Gasphasenabscheidung mit dem Ziel der Etablierung als quasi-intrinsischer Absorber in Solarzellenstrukturen mit p-i-n-Schichtfolge hin untersucht.rnDurch sein von einem hochgradig anisotropen Bindungscharakter geprägtes Kristallwachstum war die Abscheidung glatter, einphasiger und für die Integration in eine Multischichtstruktur geeigneter Schichten mit Schichtdicken von einigen 100 nm eine der wichtigsten Herausforderungen. Die Auswirkungen der beiden Parameter Abscheidungstemperatur und Stöchiometrie wurden hinsichtlich ihrer Auswirkungen auf die relevanten Kenngrößen (wie Morphologie, Dotierungsdichte und Photolumineszenz) untersucht. Es gelang, erfolgreich polykristalline Schichten mit geeigneter Rauigkeit und einer Dotierungsdichte von n ≈ 2 1015cm-3 auf anwendungsrelevanten Substraten abzuscheiden, wobei eine besonders starke Abhängigkeit von der Gasphasenzusammensetzung ermittelt werden. Es konnten weiterhin die ersten Messungen der elektronischen Zustandsdichte unter Verwendung von Hochenergie-Photoemissionsspektroskopie durchgeführt werden, die insbesondere den Einfluss variabler Materialzusammensetzungen offenbarten.rnZum Nachweis der Eignung des Materials als Absorberschicht standen innerhalb des Projektes mit SnS, Cu2O und PbS prinzipiell geeignete p-Kontaktmaterialien zur Verfügung. Es konnten trotz der Verwendung besonders sauberer Abscheidungsmethoden im Vakuum keine funktionstüchtigen Solarzellen mit Bi2S3 deponiert werden. Jedoch war es unter Verwendung von Photoemissionspektroskopie möglich, die relevanten Grenzflächen zu spektroskopieren und die Ursachen für die Beobachtungen zu identifizieren. Zudem konnte erfolgreich die Notwendigkeit von Puffermaterialien bei der Bi2S3-Abscheidung nachgewiesen werden, um Oberflächenreaktionen zu unterbinden und die Transporteigenschaften an der Grenzfläche zu verbessern.rn

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The Raman spectrum of atelestite Bi2O(OH)(AsO4), a hydroxy-arsenate mineral containing bismuth, has been studied in terms of spectra-structure relations. The studied spectrum is compared with the Raman spectrum of atelestite downloaded from the RRUFF database. The sharp intense band at 834 cm-1 is assigned to the 1 AsO43- (A1) symmetric stretching mode and the three bands at 767, 782 and 802 cm-1 to the 3 AsO43- antisymmetric stretching modes. The bands at 310, 324, 353, 370, 395, 450, 480 and 623 cm-1 are assigned to the corresponding ν4 and ν2 bending modes and Bi-O-Bi (vibration of bridging oxygen) and Bi-O (vibration of non-bridging oxygen) stretching vibrations. Lattice modes are observed at 172, 199 and 218 cm-1. A broad low intensity band at 3095 cm-1 is attributed to the hydrogen bonded OH units in the atelestite structure. A weak band at 1082 cm-1 is assigned to  (Bi-OH) vibration.

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Samples of a large (~60 µm) chondritic porous (CP) aggregate collected from the stratosphere have been analysed in detail by analytical electron microscopy (AEM). Previous studies of CP aggregates have shown that they are extraterrestrial in origin1–3 and may be related to cometary debris4. CP aggregates are dissimilar to C1 and C2 carbonaceous chondrite matrices and many have not been significantly altered by thermal or radiation processes since their assembly5. We report here a high concentration of Bi2O3 grains within the large CP aggregate designated W7029* A (~60 µm) and suggest they formed by rapid heating (~300 °C) of elemental Bi grains within the aggregate during atmospheric entry. We examine the possibilities for terrestrial Bi contamination of CP aggregate W7029* A but judge them unlikely. Enrichment of elemental Bi within components of extraterrestrial materials is consistent with a nebula condensation model6 and implies that Bi within CP aggregate W7029* A may have formed at a late stage of the condensation process.

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Platey grains of cubic Bi2O3, α-Bi2O3, and Bi2O2.75 nanograins were associated with chondritic porous interplanetary dust particles W7029C1, W7029E5, and 2011C2 that were collected in the stratosphere at 17-19 km altitude. Similar Bi oxide nanograins were present in the upper stratosphere during May 1985. These grains are linked to the plumes of several major volcanic eruptions during the early 1980s that injected material into the stratosphere. The mass of sulfur from these eruptions is a proxy for the mass of stratospheric Bi from which we derive the particle number densities (p m -3) for "average Bi2O3 nanograins" due to this volcanic activity and those necessary to contaminate the extraterrestrial chondritic porous interplanetary dust particles via collisional sticking. The match between both values supports the idea that Bi2O3 nanograins of volcanic origin could contaminate interplanetary dust particles in the Earth's stratosphere. Copyright 1997 by the American Geophysical Union.

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The mechanisms and the reaction products for the oxidation of sulfide ions in the presence of pyrite have been established. When the leach solution contains free sulfide ions, oxidation occurs via electron transfer from the sulfide ion to dissolved oxygen on the pyrite mineral surface, with polysulfides being formed as an intermediate oxidation product. In the absence of cyanide, the polysulfides are further oxidised to thiosulfate, whilst with cyanide present, thiocyanate and sulfite are also formed from the reaction of polysulfides with cyanide and dissolved oxygen. Polysulfide chain length has been shown to affect the final reaction products of polysulfide oxidation by dissolved oxygen. The rate of pyrite catalysed sulfide ion oxidation was found to be slower in cyanide solutions compared to cyanide free solutions. Mixed potential measurements indicated that the reduction of oxygen at the pyrite surface is hindered in the presence of cyanide. The presence of sulfide ions was also found to activate the pyrite surface, increasing its rate of oxidation by oxygen. This effect was particularly evident in the presence of cyanide; in the presence of sulfide the increase in total sulfur from pyrite oxidation was 2.3 mM in 7 h, compared to an increase of <1 mM in the absence of sulfide over 24 h.