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Ab initio prediction of superconductivity in molecular metallic hydrogen under high pressure

Author
LIJUN ZHANG1 ; YINGLI NIU1 ; QUAN LI1 ; TIAN CUI1 ; YI WANG1 ; YANMING MA1 ; ZHI HE1 ; GUANGTIAN ZOU1
[1] National Lab of Superhard Materials, Jilin University, Changchun 130012, China
Source

Solid state communications. 2007, Vol 141, Num 11, pp 610-614, 5 p

CODEN
SSCOA4
ISSN
0038-1098
Scientific domain
Crystallography; Electronics; Metallurgy, welding; Condensed state physics
Publisher
Elsevier, Oxford
Publication country
United Kingdom
Document type
Article
Language
English
Author keyword
61.50.Ah 63.20.Dj A. Superconductors 71.38.+i 74.70.Ad C. Crystal structure and symmetry D. Electron-phonon interactions D. Phonons
Keyword (fr)
Calcul ab initio Conduction métallique Densité état électron Effet pression Haute pression Hydrogène Interaction électron phonon Mode mou Niveau Fermi Recouvrement raie spectrale Supraconductivité Théorie BCS Théorie réponse linéaire 7462F
Keyword (en)
Ab initio calculations Metallic conduction Electronic density of states Pressure effects High pressure Hydrogen Electron-phonon interactions Soft modes Fermi level Spectral line overlapping Superconductivity BCS theory Linear response theory
Keyword (es)
Conducción metálica Recubrimiento raya espectral Teoría repuesta lineal
Classification
Pascal
001 Exact sciences and technology / 001B Physics / 001B70 Condensed matter: electronic structure, electrical, magnetic, and optical properties / 001B70D Superconductivity / 001B70D62 Transition temperature variations / 001B70D62F Pressure effects

Discipline
Physics of condensed state : electronic structure, electrical, magnetic and optical properties
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
18581477

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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