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Shubnikov-de Haas oscillations in n-CuInSe2

Author
ARUSHANOV, E; ESSALEH, L; GALIBERT, J; LEOTIN, J; ARSENE, M. A; PEYRADE, J. P; ASKENAZY, S
INSA, serv. national champs magnétiques pulsés, lab. physique solides, Toulouse, France
Source

Applied physics letters. 1992, Vol 61, Num 8, pp 958-960 ; ref : 14 ref

CODEN
APPLAB
ISSN
0003-6951
Scientific domain
Crystallography; Electronics; Optics; Condensed state physics
Publisher
American Institute of Physics, Melville, NY
Publication country
United States
Document type
Article
Language
English
Keyword (fr)
Basse température Champ magnétique Composé minéral Cuivre Indium Séléniure Mixte Effet Shubnikov de Haas Etude expérimentale Etude théorique Facteur g Masse effective Surface Fermi Température Très basse température Métal transition Composé
Keyword (en)
Low temperature Magnetic field Inorganic compound Copper Indium Selenides Mixed Shubnikov de Haas effect Experimental study Theoretical study g factor Effective mass Fermi surface Temperature Very low temperature Transition metal Compounds
Keyword (es)
Baja temperatura Campo magnético Compuesto inorgánico Cobre Indio Seleniuro Mixto Efecto Shubnikov de Haas Estudio experimental Estudio teórico Factor g Masa efectiva Superficie Fermi Temperatura Temperatura muy baja Metal transición Compuesto
Classification
Pascal
001 Exact sciences and technology / 001B Physics / 001B70 Condensed matter: electronic structure, electrical, magnetic, and optical properties / 001B70A Electron states / 001B70A18 Fermi surface: calculations and measurements; effective mass, g factor

Discipline
Physics of condensed state : electronic structure, electrical, magnetic and optical properties
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
5477572

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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