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Direct dark matter detection around the corner? Prospects in the Constrained MSSM

Abstract:

We outline the WIMP dark matter parameter space in the Constrained MSSM by performing a comprehensive statistical analysis that compares with experimental data predicted superpartner masses and other collider observables as well as a cold dark matter abundance. We find that 10(-10) pb less than or similar to sigma(SI)(p) less than or similar to 10(-8) pb for direct WIMP detection (with details slightly dependent on the assumptions made). We conclude that most of the 95% probability region for...

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Publication status:
Published

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Publisher copy:
10.1088/1742-6596/60/1/056

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Institution:
University of Oxford
Department:
Oxford, MPLS, Physics, Astrophysics
Role:
Author
Volume:
60
Pages:
259-263
Publication date:
2007-01-01
DOI:
EISSN:
1742-6596
ISSN:
1742-6588
URN:
uuid:040c060f-63bc-4686-9aee-bbda67abce2c
Source identifiers:
17126
Local pid:
pubs:17126

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