The tin-rich side of the rare earth-tin systems (R=Gd, Tb, Dy, Ho, Er, Tm, Lu and Y)
Identifieur interne : 003769 ( Main/Merge ); précédent : 003768; suivant : 003770The tin-rich side of the rare earth-tin systems (R=Gd, Tb, Dy, Ho, Er, Tm, Lu and Y)
Auteurs : A. Palenzona [Italie] ; P. ManfrinettiSource :
- Journal of alloys and compounds [ 0925-8388 ] ; 1993.
Descripteurs français
- Pascal (Inist)
- Système binaire, Etain alliage, Lanthanide alliage, Gadolinium alliage, Terbium alliage, Dysprosium alliage, Holmium alliage, Erbium alliage, Thulium alliage, Lutétium alliage, Yttrium alliage, Alliage binaire, Analyse thermique différentielle, Diffraction RX, Diagramme phase, Composé intermétallique, Métallographie, Etude expérimentale, Système Gd Sn, Système Sn Tb, Système Dy Sn, Système Ho Sn, Système Er Sn, Système Sn Tm, Système Lu Sn, Système Sn Y.
English descriptors
- KwdEn :
- Binary alloys, Binary systems, Differential thermal analysis, Dysprosium alloys, Erbium alloys, Experimental study, Gadolinium alloys, Holmium alloys, Intermetallic compounds, Lutetium alloys, Metallography, Phase diagrams, Rare earth alloys, Terbium alloys, Thulium alloys, Tin alloys, X-ray diffraction, Yttrium alloys.
Abstract
The tin-rich side of the rare earth-tin systems (R=Gd, Tb, Dy, Ho, Er, Tm, Lu and Y) has been investigated using differential thermal analysis, microscopic analysis, X-ray diffraction and electron microscopy. A complex situation has been found which can be summarized by the presence of compounds with four types of stoichiometry that can be considered as members of the structural series RnSn3n-2:RSn2, R3Sn7, R2Sn5 and RSn3, two of which have structural modifications depending on temperature. The main problem in studying these systems has been the difficulty of attaining equilibrium in these alloys, which had prevented till now the discovery of the existence of these compounds
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Pascal:94-0237702Le document en format XML
<record><TEI><teiHeader><fileDesc><titleStmt><title xml:lang="en" level="a">The tin-rich side of the rare earth-tin systems (R=Gd, Tb, Dy, Ho, Er, Tm, Lu and Y)</title><author><name sortKey="Palenzona, A" sort="Palenzona, A" uniqKey="Palenzona A" first="A." last="Palenzona">A. Palenzona</name><affiliation wicri:level="1"><inist:fA14 i1="01"><s1>Univ. Genova, ist. chimica fisica</s1><s2>16132 Genoa</s2><s3>ITA</s3></inist:fA14><country>Italie</country><wicri:noRegion>16132 Genoa</wicri:noRegion></affiliation></author><author><name sortKey="Manfrinetti, P" sort="Manfrinetti, P" uniqKey="Manfrinetti P" first="P." last="Manfrinetti">P. Manfrinetti</name></author></titleStmt><publicationStmt><idno type="wicri:source">INIST</idno><idno type="inist">94-0237702</idno><date when="1993">1993</date><idno type="stanalyst">PASCAL 94-0237702 INIST</idno><idno type="RBID">Pascal:94-0237702</idno><idno type="wicri:Area/Pascal/Corpus">001835</idno><idno type="wicri:Area/Pascal/Curation">001835</idno><idno type="wicri:Area/Pascal/Checkpoint">001823</idno><idno type="wicri:explorRef" wicri:stream="Pascal" wicri:step="Checkpoint">001823</idno><idno type="wicri:doubleKey">0925-8388:1993:Palenzona A:the:tin:rich</idno><idno type="wicri:Area/Main/Merge">003769</idno></publicationStmt><sourceDesc><biblStruct><analytic><title xml:lang="en" level="a">The tin-rich side of the rare earth-tin systems (R=Gd, Tb, Dy, Ho, Er, Tm, Lu and Y)</title><author><name sortKey="Palenzona, A" sort="Palenzona, A" uniqKey="Palenzona A" first="A." last="Palenzona">A. Palenzona</name><affiliation wicri:level="1"><inist:fA14 i1="01"><s1>Univ. Genova, ist. chimica fisica</s1><s2>16132 Genoa</s2><s3>ITA</s3></inist:fA14><country>Italie</country><wicri:noRegion>16132 Genoa</wicri:noRegion></affiliation></author><author><name sortKey="Manfrinetti, P" sort="Manfrinetti, P" uniqKey="Manfrinetti P" first="P." last="Manfrinetti">P. Manfrinetti</name></author></analytic><series><title level="j" type="main">Journal of alloys and compounds</title><title level="j" type="abbreviated">J. alloys compd.</title><idno type="ISSN">0925-8388</idno><imprint><date when="1993">1993</date></imprint></series></biblStruct></sourceDesc><seriesStmt><title level="j" type="main">Journal of alloys and compounds</title><title level="j" type="abbreviated">J. alloys compd.</title><idno type="ISSN">0925-8388</idno></seriesStmt></fileDesc><profileDesc><textClass><keywords scheme="KwdEn" xml:lang="en"><term>Binary alloys</term><term>Binary systems</term><term>Differential thermal analysis</term><term>Dysprosium alloys</term><term>Erbium alloys</term><term>Experimental study</term><term>Gadolinium alloys</term><term>Holmium alloys</term><term>Intermetallic compounds</term><term>Lutetium alloys</term><term>Metallography</term><term>Phase diagrams</term><term>Rare earth alloys</term><term>Terbium alloys</term><term>Thulium alloys</term><term>Tin alloys</term><term>X-ray diffraction</term><term>Yttrium alloys</term></keywords><keywords scheme="Pascal" xml:lang="fr"><term>Système binaire</term><term>Etain alliage</term><term>Lanthanide alliage</term><term>Gadolinium alliage</term><term>Terbium alliage</term><term>Dysprosium alliage</term><term>Holmium alliage</term><term>Erbium alliage</term><term>Thulium alliage</term><term>Lutétium alliage</term><term>Yttrium alliage</term><term>Alliage binaire</term><term>Analyse thermique différentielle</term><term>Diffraction RX</term><term>Diagramme phase</term><term>Composé intermétallique</term><term>Métallographie</term><term>Etude expérimentale</term><term>Système Gd Sn</term><term>Système Sn Tb</term><term>Système Dy Sn</term><term>Système Ho Sn</term><term>Système Er Sn</term><term>Système Sn Tm</term><term>Système Lu Sn</term><term>Système Sn Y</term></keywords></textClass></profileDesc></teiHeader><front><div type="abstract" xml:lang="en">The tin-rich side of the rare earth-tin systems (R=Gd, Tb, Dy, Ho, Er, Tm, Lu and Y) has been investigated using differential thermal analysis, microscopic analysis, X-ray diffraction and electron microscopy. A complex situation has been found which can be summarized by the presence of compounds with four types of stoichiometry that can be considered as members of the structural series R<sub>n</sub>Sn<sub>3n-2</sub>:RSn<sub>2</sub>, R<sub>3</sub>Sn<sub>7</sub>, R<sub>2</sub>Sn<sub>5</sub> and RSn<sub>3</sub>, two of which have structural modifications depending on temperature. The main problem in studying these systems has been the difficulty of attaining equilibrium in these alloys, which had prevented till now the discovery of the existence of these compounds</div></front></TEI><affiliations><list><country><li>Italie</li></country></list><tree><noCountry><name sortKey="Manfrinetti, P" sort="Manfrinetti, P" uniqKey="Manfrinetti P" first="P." last="Manfrinetti">P. Manfrinetti</name></noCountry><country name="Italie"><noRegion><name sortKey="Palenzona, A" sort="Palenzona, A" uniqKey="Palenzona A" first="A." last="Palenzona">A. Palenzona</name></noRegion></country></tree></affiliations></record>Pour manipuler ce document sous Unix (Dilib)
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