Published April 15, 2002
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SUSY dark matter and non-universal gaugino masses
Description
In this talk the authors investigate the dark matter prospects for supersymmetric models with non-universal gaugino masses. They motivate the use of non-universal gaugino masses from several directions, including problems, with the current favorite scenario, the cMSSM. They then display new corridors of parameter space that allow an acceptable dark matter relic density once gaugino mass universality is relaxed. They finish with a specific string-derived model that allows this universality relaxation and then use the dark matter constraint to make specific statements about the hidden sector of the model
Availability note (English)
Available from INIS in electronic form; Also available from OSTI as DE00796097; PURL: https://www.osti.gov/servlets/purl/796097-1iFhB2/native/
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Additional details
Identifiers
Publishing Information
- Imprint Pagination
- 5 p.
- Report number
- LBNL--50109
Conference
- Title
- Sources and Detection of Dark Matter and Dark Energy in the Universe
- Dates
- 20-22 Feb 2002
- Place
- Marina del Rey, CA (United States)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 33046565
- Subject category
- S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- COSMOLOGICAL MODELS; DETECTION; NONLUMINOUS MATTER; STRING MODELS; SUPERSYMMETRY; UNIVERSE
- Descriptors DEC
- COMPOSITE MODELS; EXTENDED PARTICLE MODEL; MATHEMATICAL MODELS; MATTER; PARTICLE MODELS; QUARK MODEL; SYMMETRY
Optional Information
- Contract/Grant/Project number
- AC03-76SF00098
- Funding organization
- USDOE Director, Office of Science. Office of High Energy and Nuclear Physics. Division of High Energy Physics (United States)
- Secondary number(s)
- UCB-PTH--02/15