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AC susceptibility study of Bi1.66Pb0.34Sr2Ca2-xMgxCu3Oy (x = 0, 0.2 and 0.4) superconductor systems

Author
KAMELI, P1 ; SALAMATI, H1 ; ABDOLHOSSEINI, I1
[1] Department of Physics, Isfahan University of Technology, Isfahan, Iran, Islamic Republic of
Source

Journal of alloys and compounds. 2008, Vol 458, Num 1-2, pp 61-65, 5 p ; ref : 30 ref

ISSN
0925-8388
Scientific domain
Inorganic chemistry; Crystallography; Metallurgy, welding; Condensed state physics
Publisher
Elsevier, Lausanne
Publication country
Switzerland
Document type
Article
Language
English
Author keyword
AC susceptibility High-Tc superconductors Intergranular properties Mg substitution
Keyword (fr)
Bismuth Calcium Cuivre Magnésium Plomb Strontium Oxyde Mixte Composition chimique Densité courant critique Effet température Electronégativité Joint grain Liaison faible Modèle état critique Réaction état solide Supraconducteur haute température Susceptibilité magnétique Bi1.66Pb0.34Sr2Ca2-xMgxCuOy
Keyword (en)
Bismuth Calcium Copper Magnesium Lead Strontium Oxides Mixed Chemical composition Critical current density Temperature effects Electronegativity Grain boundaries Weak links Critical state model Solid state reaction High-Tc superconductors Magnetic susceptibility
Keyword (es)
Mixto Densidad corriente crítica Reacción estado sólido
Classification
Pascal
001 Exact sciences and technology / 001B Physics / 001B70 Condensed matter: electronic structure, electrical, magnetic, and optical properties / 001B70D Superconductivity / 001B70D25 Properties of type I and type II superconductors / 001B70D25S Critical currents

Discipline
Physics of condensed state : electronic structure, electrical, magnetic and optical properties
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
20348843

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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