  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.
