R-parity violation in split supersymmetry
- Author
- SUDHIR KUMAR GUPTA1 ; KONAR, Partha2 ; MUKHOPADHYAYA, Biswarup1
[1] Harish-Chandra Research Institute, Chhatnag Road, Jhusi, Allahabad 211019, India
[2] Department of Theoretical Physics, Tata Institute of Fundamental Research, Homi Bhabha Road, Mumbai 400005, India - Source
Physics letters. Section B. 2005, Vol 606, Num 3-4, pp 384-390, 7 p ; ref : 22 ref
- CODEN
- PYLBAJ
- ISSN
- 0370-2693
- Scientific domain
- Theoretical physics
- Publisher
- Elsevier Science, Amsterdam
- Publication country
- Netherlands
- Document type
- Article
- Language
- English
- Keyword (fr)
- Brisure symétrie Désintégration méson Lepton Matière sombre Méson B Nombre baryonique Nombre leptonique Parité Particule supersymétrique Quark Supersymétrie Vertex Violation parité Gaugino Neutralino
- Keyword (en)
- Symmetry breaking Meson decay Leptons Dark matter B mesons Baryon number Lepton number Parity Sparticles Quarks Supersymmetry Vertex Parity violation Gaugino Neutralino
- Keyword (es)
- Vértice Violación paridad Gaugino Neutralino
- Classification
- Pascal
- 001 Exact sciences and technology / 001B Physics / 001B10 The physics of elementary particles and fields / 001B10B Specific theories and interaction models; particle systematics / 001B10B60 Models beyond the standard model / 001B10B60J Supersymmetric models
- Pascal
- 001 Exact sciences and technology / 001B Physics / 001B10 The physics of elementary particles and fields / 001B10D Properties of specific particles / 001B10D80 Other particles (including hypothetical) / 001B10D80L Supersymmetric partners of known particles
- 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)
- Discipline
- Astronomy Physics of elementary particles and fields
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 16450763
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.physletb.2004.12.014 
https://dx.doi.org/10.1016/j.physletb.2004.12.014
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