Discrimination of supersymmetric grand unified models in gaugino mediation
Creators
- 1. Department of Physics and Astronomy, University of Alabama, Tuscaloosa, Alabama 35487 (United States)
- 2. Hanoi University of Science - VNU, 334 Nguyen Trai Road, Hanoi (Viet Nam)
- 3. Hanoi University of Science and Technology, 1 Dai Co Viet Road, Hanoi (Viet Nam)
Description
We consider supersymmetric grand unified theory (GUT) with the gaugino mediated supersymmetry breaking and investigate a possibility to discriminate different GUT models in terms of predicted sparticle mass spectra. Taking two example GUT models, the minimal SU(5) and simple SO(10) models, and imposing a variety of theoretical and experimental constraints, we calculate sparticle masses. Fixing parameters of each model so as to result in the same mass of neutralino as the lightest supersymmetric particle (LSP), giving the observed dark matter relic density, we find sizable mass differences in the left-handed slepton and right-handed down-type squark sectors in two models, which can be a probe to discriminate the GUT models realized at the GUT scale far beyond the reach of collider experiments.
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.83.053001;
- arXiv
- arXiv:1011.1668v2;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 83
- Journal Issue
- 5
- Journal Page Range
- p. 053001-053001.8
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 43055892
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- GRAND UNIFIED THEORY; MASS; MASS DIFFERENCE; MASS SPECTRA; NONLUMINOUS MATTER; PROBES; SPARTICLES; SUPERSYMMETRY; SYMMETRY BREAKING
- Descriptors DEC
- ELEMENTARY PARTICLES; FIELD THEORIES; MATHEMATICAL MODELS; MATTER; PARTICLE MODELS; PARTICLE PROPERTIES; POSTULATED PARTICLES; QUANTUM FIELD THEORY; SPECTRA; SYMMETRY; UNIFIED GAUGE MODELS
Optional Information
- Notes
- (c) 2011 American Institute of Physics