Published January 25, 2007 | Version v1
Journal article

Possible signals of wino LSP at the Large Hadron Collider

  • 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.