LHC SUSY and WIMP dark matter searches confront the string theory
  landscape
  The string theory landscape of vacua solutions provides physicists with some
understanding as to the magnitude of the cosmological constant. Similar
reasoning can be applied to the magnitude of the soft SUSY breaking terms in
supersymmetric models of particle physics: there appears to be a statistical
draw towards large soft terms which is tempered by the anthropic requirement of
the weak scale lying not too far from ~100 GeV. For a mild statistical draw of
m_{soft}^n with n=1 (as expected from SUSY breaking due to a single F term)
then the light Higgs mass is preferred at ~125 GeV while sparticles are all
pulled beyond LHC bounds. We confront a variety of LHC and WIMP dark matter
search limits with the statistical expectations from a fertile patch of string
theory landscape. The end result is that LHC and WIMP dark matter detectors see
exactly that which is expected from the string theory landscape: a Standard
Model-like Higgs boson of mass 125 GeV but as yet no sign of sparticles or WIMP
dark matter. SUSY from the n=1 landscape is most likely to emerge at LHC in the
soft opposite-sign dilepton plus jet plus MET channel. Multi-ton noble liquid
WIMP detectors should be able to completely explore the n=1 landscape parameter
space.
