Dark matter and collider phenomenology of universal extra dimensions
- Auteur
- HOOPER, Dan1 ; PROFUMO, Stefano2 3
[1] Theoretical Astrophysics Group, Fermilab, Batavia, IL 60510, United States
[2] Division of Physics, Mathematics and Astronomy, California Institute of Technology, Mail Code 106-38, Pasadena, CA 91125, United States
[3] Santa Cruz Institute for Particle Physics, University of California, Santa Cruz CA 95064, United States - Source
Physics reports. 2007, Vol 453, Num 2-4, pp 29-115, 87 p ; ref : 256 ref
- CODEN
- PRPLCM
- ISSN
- 0370-1573
- Domaine scientifique
- Physics; Theoretical physics
- Editeur
- Elsevier Science, Amsterdam
- Pays de publication
- Netherlands
- Type de document
- Article
- Langue
- English
- Mot clé auteur
- 11.10.Kk 12.60.-i 95.35.+d
- Mot clé (fr)
- Abondance Collisionneur linéaire Compactification Cosmologie Etat dégénéré Hadron Matière sombre Modèle particule Modèle référence Modèle standard Métrique plate Observable Parité Règle Feynman Section efficace Supersymétrie Théorie Kaluza Klein Univers primordial
- Mot clé (en)
- Abundance Linear colliders Compactification Cosmology Degenerate state Hadrons Dark matter Particle models Reference model Standard model Flat metric Observables Parity Feynman rule Cross sections Supersymmetry Kaluza-Klein theory Early universe
- Mot clé (es)
- Estado degenerado Modelo referencia Métrico plano Regla Feynman
- Classification
- Discipline
- Theoretical physics
- Provenance
- Inist-CNRS
- Base de données
- PASCAL
- Identifiant INIST
- 19439221
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
10.1016/j.physrep.2007.09.003 
https://dx.doi.org/10.1016/j.physrep.2007.09.003
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