Neutrino superfluidity
- Author
- KAPUSTA, J. I1
[1] School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, United States - Source
Physical review letters. 2004, Vol 93, Num 25, pp 251801.1-251801.3 ; ref : 7 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)
- Boson Higgs Echange particule Groupe U(1) Longueur cohérence Neutrino Paire Cooper Particule élémentaire Superfluidité Température critique Théorie SU(2)
- Keyword (en)
- Higgs bosons Particle exchange U-1 groups Coherence length Neutrinos Cooper pairs Elementary particles Superfluidity Critical temperature SU(2) theory
- Keyword (es)
- Intercambio partícula
- Classification
- Pascal
- 001 Exact sciences and technology / 001B Physics / 001B10 The physics of elementary particles and fields / 001B10D Properties of specific particles / 001B10D60 Leptons / 001B10D60P Neutrino mass and mixing
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03A Fundamental astronomy and astrophysics. Instrumentation, techniques, and astronomical observations / 001E03A35 Dark matter (stellar, interstellar, galactic, and cosmological)
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03C Stars / 001E03C60 Late stages of stellar evolution (including black holes) / 001E03C60J Neutron stars
- Discipline
- Astronomy Physics of elementary particles and fields
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 16378144
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.93.251801 
https://dx.doi.org/10.1103/PhysRevLett.93.251801
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