Lower limits on R-parity-violating couplings in supersymmetric models with light squarks
Creators
- 1. High Energy Physics Division, Argonne National Laboratory, Argonne, Illinois 60439 (United States)
- 2. Theoretical Physics Department, Fermi National Accelerator Laboratory, Batavia, Illinois 60510-0500 (United States)
Description
We interpret the results of searches for strongly interacting massive particles to place absolute lower limits on R-parity-violating couplings for squarks with mass (mq-tilde) below 100 GeV. Recent searches for anomalous isotopes require that there be a baryon-number-violating or lepton-number-violating coupling larger than 10-22-10-21 if mq-tilde>18 GeV. Using data from searches for stable particles at the CERN Large Electron Positron Collider (LEP) we demonstrate that this lower limit increases by 14 orders of magnitude, to an R-parity-violating coupling larger than 10-8-10-7 for any squarks of mass less than 90 GeV. In the presence of an R-parity-violating coupling of this magnitude, neutralinos cannot explain the dark matter density in the Universe
Additional details
Identifiers
- DOI
- 10.1103/PhysRevLett.92.201801;
- arXiv
- arXiv:hep-ph/0310001v2;
Publishing Information
- Journal Title
- Physical Review Letters
- Journal Volume
- 92
- Journal Issue
- 20
- Journal Page Range
- p. 201801-201801.4
- ISSN
- 0031-9007
- CODEN
- PRLTAO
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 36019240
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- BARYON NUMBER; CERN; CONSERVATION LAWS; COSMOLOGY; COUPLING; COUPLING CONSTANTS; GEV RANGE 10-100; LEP STORAGE RINGS; LEPTON NUMBER; NONLUMINOUS MATTER; PARITY; QUANTUM FIELD THEORY; SPARTICLES; SUPERSYMMETRY; UNIVERSE
- Descriptors DEC
- ACCELERATORS; CYCLIC ACCELERATORS; ELEMENTARY PARTICLES; ENERGY RANGE; FIELD THEORIES; GEV RANGE; INTERNATIONAL ORGANIZATIONS; MATTER; PARTICLE PROPERTIES; POSTULATED PARTICLES; STORAGE RINGS; SYMMETRY; SYNCHROTRONS
Optional Information
- Notes
- (c) 2004 The American Physical Society