Speaker
Prof.
Howard Baer
(Florida State University)
Description
While most of parameter space of the mSUGRA model is excluded by the constraint on
dark matter relic density, a variety of well-motivated models with non-universal soft
breaking terms can easily accommodate the relic abundance. I survey various models
with non-universal scalar and gauginos masses by the names of NUHM1, NUHM2, NMH,
MWDM, BWCA-DM and compressed SUSY, or LM3DM. Each of these scenarios gives rise to
unique predictions for collider and dark matter detection phenomenology.
Author
Prof.
Howard Baer
(Florida State University)
