Non-Abelian gauge potentials for ultracold atoms with degenerate dark states
- Author
- RUSECKAS, J1 2 ; JUZELIUNAS, G1 ; ÖHBERG, P3 ; FLEISCHHAUER, M2
[1] Institute of Theoretical Physics and Astronomy of Vilnius University, A. Goštauto 12, 01108 Vilnius, Lithuania
[2] Fachbereich Physik, Technische Universität Kaiserslautern, 67663 Kaiserslautern, Germany
[3] Department of Physics, University of Strathclyde, Glasgow G4 0NG, United Kingdom - Source
Physical review letters. 2005, Vol 95, Num 1, pp 010404.1-010404.4 ; ref : 31 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)
- Atome n niveaux Atome ultrafroid Etat dégénéré Faisceau laser Interaction rayonnement matière Théorie non abélienne 0365V
- Keyword (en)
- Multilevel atom Ultracold atom Degenerate state Laser beams Radiation matter interactions Non abelian theory
- Keyword (es)
- Atomo n niveles Estado degenerado Teoría no abeliana
- Classification
- Pascal
- 001 Exact sciences and technology / 001B Physics / 001B00 General / 001B00C Classical and quantum physics: mechanics and fields / 001B00C65 Quantum mechanics / 001B00C65B Foundations, theory of measurement, miscellaneous theories (including aharonov-bohm effect, bell inequalities, berry's phase)
- Discipline
- Theoretical physics
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 16956499
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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DOI
10.1103/PhysRevLett.95.010404 
https://dx.doi.org/10.1103/PhysRevLett.95.010404
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