SUSY Phenomenology of KKLT Flux Compactifications

Details SUSY Phenomenology of KKLT Flux Compactifications SUSY Phenomenology of KKLT Flux Compactifications

2005-07-08

arxiv.org/abs/hep-ph/0507110v2

JHEP 0511:034,2005

Physics

High Energy Physics

High Energy Physics - Phenomenology

23 pages, 8 figures; v2: erratum attached

Scientific paper

10.1088/1126-6708/2005/11/034

We study SUSY phenomenology of the KKLT (Kachru-Kallosh-Linde-Trivedi) scenario of string theory compactifications with fluxes. This setup leads to a specific pattern of soft masses and distinct phenomenological properties. In particular, it avoids the cosmological gravitino/moduli problems. Remarkably, the model allows for the correct abundance of SUSY dark matter consistently with all experimental constraints including the bound on the Higgs mass, b-->s gamma, etc. This occurs for both small and large tan beta, and requires the SUSY spectrum above 1 TeV.

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