Colloidally stable selenium@copper selenide core@shell nanoparticles as selenium source for manufacturing of copper-indium-selenide solar cells
Identifieur interne : 000179 ( Main/Repository ); précédent : 000178; suivant : 000180Colloidally stable selenium@copper selenide core@shell nanoparticles as selenium source for manufacturing of copper-indium-selenide solar cells
Auteurs : RBID : Pascal:14-0087058Descripteurs français
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Abstract
Selenium nanoparticles with diameters of 100-400 nm are prepared via hydrazine-driven reduction of selenious acid. The as-prepared amorphous, red selenium (a-Se) particles were neither a stable phase nor were they colloidally stable. Due to phase transition to crystalline (trigonal), grey selenium (t-Se) at or even below room temperature, the particles merged rapidly and recrystallized as micronsized crystal needles. As a consequence, such Se particles were not suited for layer deposition and as a precursor to manufacture thin-film CIS (copper indium selenide/CulnSe2) solar cells. To overcome this restriction, Se@CuSe core@shell particles are presented here. For these Se@CuSe core@shell nanoparticles, the phase transition a-Se → t-Se is shifted to temperatures higher than 100°C. Moreover, a spherical shape of the particles is retained even after phase transition. Composition and structure of the Se@CuSe core@shell nanostructure are evidenced by electron microscopy (SEM/STEM), DLS, XRD, FT-IR and line-scan EDXS. As a conceptual study, the newly formed Se@CuSe core@shell nanostructures with CuSe acting as a protecting layer to increase the phase-transition temperature and to improve the colloidal stability were used as a selenium precursor for manufacturing of thin-film CIS solar cells and already lead to conversion efficiencies up to 3%.
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<author><name>HAILONG DONG</name>
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<author><name sortKey="Quintilla, Aina" uniqKey="Quintilla A">Aina Quintilla</name>
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<s2>70565 Stuttgart</s2>
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<author><name sortKey="Cemernjak, Marco" uniqKey="Cemernjak M">Marco Cemernjak</name>
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<author><name sortKey="Popescu, Radian" uniqKey="Popescu R">Radian Popescu</name>
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<author><name sortKey="Gerthsen, Dagmar" uniqKey="Gerthsen D">Dagmar Gerthsen</name>
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<author><name sortKey="Feldmann, Claus" uniqKey="Feldmann C">Claus Feldmann</name>
<affiliation wicri:level="3"><inist:fA14 i1="01"><s1>Institut für Anorganische Chemie, Karlsruhe Institute of Technology (KIT), Engesserstrasse 15</s1>
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<s3>DEU</s3>
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<region type="district" nuts="2">District de Karlsruhe</region>
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<term>Copper selenides</term>
<term>Indium</term>
<term>Manufacturing</term>
<term>Selenium</term>
<term>Solar cell</term>
<term>Solar radiation</term>
<term>Structure</term>
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<keywords scheme="Pascal" xml:lang="fr"><term>Sélénium</term>
<term>Particule enrobée</term>
<term>Fabrication</term>
<term>Indium</term>
<term>Rayonnement solaire</term>
<term>Structure</term>
<term>Cellule solaire</term>
<term>Séléniure de cuivre</term>
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<front><div type="abstract" xml:lang="en">Selenium nanoparticles with diameters of 100-400 nm are prepared via hydrazine-driven reduction of selenious acid. The as-prepared amorphous, red selenium (a-Se) particles were neither a stable phase nor were they colloidally stable. Due to phase transition to crystalline (trigonal), grey selenium (t-Se) at or even below room temperature, the particles merged rapidly and recrystallized as micronsized crystal needles. As a consequence, such Se particles were not suited for layer deposition and as a precursor to manufacture thin-film CIS (copper indium selenide/CulnSe<sub>2</sub>
) solar cells. To overcome this restriction, Se@CuSe core@shell particles are presented here. For these Se@CuSe core@shell nanoparticles, the phase transition a-Se → t-Se is shifted to temperatures higher than 100°C. Moreover, a spherical shape of the particles is retained even after phase transition. Composition and structure of the Se@CuSe core@shell nanostructure are evidenced by electron microscopy (SEM/STEM), DLS, XRD, FT-IR and line-scan EDXS. As a conceptual study, the newly formed Se@CuSe core@shell nanostructures with CuSe acting as a protecting layer to increase the phase-transition temperature and to improve the colloidal stability were used as a selenium precursor for manufacturing of thin-film CIS solar cells and already lead to conversion efficiencies up to 3%.</div>
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<sZ>1 aut.</sZ>
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) solar cells. To overcome this restriction, Se@CuSe core@shell particles are presented here. For these Se@CuSe core@shell nanoparticles, the phase transition a-Se → t-Se is shifted to temperatures higher than 100°C. Moreover, a spherical shape of the particles is retained even after phase transition. Composition and structure of the Se@CuSe core@shell nanostructure are evidenced by electron microscopy (SEM/STEM), DLS, XRD, FT-IR and line-scan EDXS. As a conceptual study, the newly formed Se@CuSe core@shell nanostructures with CuSe acting as a protecting layer to increase the phase-transition temperature and to improve the colloidal stability were used as a selenium precursor for manufacturing of thin-film CIS solar cells and already lead to conversion efficiencies up to 3%.</s0>
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