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Gaplike excitations in the superconducting state of Bi2Sr2CaCu2O8 studied by resonant raman scattering

Author
BUDELMANN, D1 ; SCHULZ, B1 ; RÜBHAUSEN, M1 ; KLEIN, M. V2 ; WILLIAMSEN, M. S3 ; GUPTASARMA, P3
[1] Institut für Angewandte Physik, Universität Hamburg, 20355 Hamburg, Germany
[2] Department of Physics, University of Illinois, Urbana, Illinois 61801, United States
[3] Department of Physics, University of Wisconsin, Milwaukee, Wisconsin 53211, United States
Source

Physical review letters. 2005, Vol 95, Num 5, pp 057003.1-057003.4 ; ref : 28 ref

CODEN
PRLTAO
ISSN
0031-9007
Scientific domain
Optics; Atomic molecular physics; Condensed state physics; Physics; Plasma physics
Publisher
American Physical Society, Ridge, NY
Publication country
United States
Document type
Article
Language
English
Keyword (fr)
Bande interdite supraconductrice Bismuth oxyde Calcium oxyde Cuivre oxyde Diffusion Raman résonance Diffusion inélastique Mode collectif Profil raie Strontium oxyde Supraconducteur haute température Supraconductivité 7425G
Keyword (en)
Superconducting energy gap Bismuth oxides Calcium oxides Copper oxides Resonance Raman scattering Inelastic scattering Collective mode Line shape Strontium oxides High-Tc superconductors Superconductivity
Keyword (es)
Difusión Ramán resonancia Modo colectivo
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 / 001B70D25G Optical properties

Discipline
Physics of condensed state : electronic structure, electrical, magnetic and optical properties
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
17021029

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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