Published January 25, 2007
| Version v1
Journal article
Possible signals of wino LSP at the Large Hadron Collider
Creators
- 1. Stanford Linear Accelerator Center, Stanford University, Stanford, CA 94309 (United States)
- 2. Department of Physics, Tohoku University, Sendai (Japan)
- 3. Research Center for the Early Universe, University of Tokyo, Tokyo 113-0033 (Japan)
- 4. Department of Physics, University of Tokyo, Tokyo 113-0033 (Japan)
Description
We consider a class of anomaly-mediated supersymmetry breaking models where gauginos acquire masses mostly from anomaly mediation while masses of other superparticles are from Kahler interactions, which are as large as gravitino mass ∼O(10-100)TeV. In this class of models, the neutral wino becomes the lightest superparticle in a wide parameter region. The mass splitting between charged and neutral winos are very small and experimental discovery of such winos is highly non-trivial. We discuss how we should look for wino-induced signals at Large Hadron Collider
Additional details
Identifiers
- DOI
- 10.1016/j.physletb.2006.11.061;
- arXiv
- arXiv:hep-ph/0610277v1;
- PII
- S0370-2693(06)01515-2;
Publishing Information
- Journal Title
- Physics Letters. Section B
- Journal Volume
- 644
- Journal Issue
- 5-6
- Journal Page Range
- p. 355-360
- ISSN
- 0370-2693
- CODEN
- PYLBAJ
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 39014307
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- CERN LHC; MASS; SIGNALS; SYMMETRY BREAKING; TEV RANGE 10-100
- Descriptors DEC
- ACCELERATORS; CYCLIC ACCELERATORS; ENERGY RANGE; STORAGE RINGS; SYNCHROTRONS; TEV RANGE
Optional Information
- Copyright
- Copyright (c) 2006 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.