Published December 1, 2011
| Version v1
Journal article
Non-standard neutrino interactions at colliders
Creators
- 1. Department of Physics and Astronomy, York University, Toronto, ON (Canada)
- 2. IPNL, Universite de Lyon, Universite Lyon 1, CNRS/IN2P3, 4 rue E. Fermi 69622 Villeurbanne cedex (France)
Description
Many extensions of the Standard Model lead to nonstandard neutrino interactions (NSI), which can affect the interpretation of current and future neutrino data. We explore an alternative approach to the study of these dimension-eight four-fermion interactions (of coefficient 4εGF/√(2)), by bringing into play collider data. In models where coefficients of potential dimension-six operators are suppressed by cancellations, LEP2 can provide interesting bounds on NSI operators (ε < or approx. 10-2-10-3). If NSI are contact interactions at LHC energies, they induce an effective interaction qqW+W-eα+eβ- (according to the Equivalence Theorem), to which the LHC at 14 TeV and with 100 fb-1 of data has excellent sensitivity (ε < or approx. 3x10-3).
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.84.113011;
- arXiv
- arXiv:1108.5320v1;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 84
- Journal Issue
- 11
- Journal Page Range
- p. 113011-113011.11
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 43080289
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- CANCELLATION; CERN LHC; FERMI INTERACTIONS; NEUTRINOS; SENSITIVITY; STANDARD MODEL; TEV RANGE 10-100
- Descriptors DEC
- ACCELERATORS; BASIC INTERACTIONS; CYCLIC ACCELERATORS; ELEMENTARY PARTICLES; ENERGY RANGE; FERMIONS; FIELD THEORIES; GRAND UNIFIED THEORY; INTERACTIONS; LEPTONS; MASSLESS PARTICLES; MATHEMATICAL MODELS; PARTICLE MODELS; QUANTUM FIELD THEORY; STORAGE RINGS; SYNCHROTRONS; TEV RANGE; UNIFIED GAUGE MODELS; WEAK INTERACTIONS
Optional Information
- Notes
- (c) 2011 American Institute of Physics