Abstract
In supersymmetric models with gravity-mediated SUSY
breaking, universality of soft SUSY breaking sfermion masses m0
is motivated by the need to suppress unwanted flavor changing
processes. The same motivation, however, does not apply to soft
breaking Higgs masses, which may in general have independent masses
from matter scalars at the GUT scale. We explore phenomenological
implications of both the one-parameter and two-parameter
non-universal Higgs mass models (NUHM1 and NUHM2), and examine the
parameter ranges compatible with ΩCDMh2, BF(b→sγ) and (g−2)μ constraints. We have demonstrated that in
contrast to the mSUGRA model, in both NUHM1 and NUHM2 models, the
dark matter A-annihilation funnel can be reached at low values of
tan β, while the higgsino dark matter annihilation regions can
be reached for low values of m0. We show that there may be
observable rates for indirect and direct detection of neutralino
cold dark matter in phenomenologically aceptable ranges of parameter
space. We also examine implications of the NUHM models for the
Fermilab Tevatron, the CERN LHC and a (s)1/2 = 0.5−1 TeV e+e−
linear collider. Novel possibilities include: very light R,
R squark and
L slepton masses as
well as light charginos and neutralinos and H, A and H±
Higgs bosons.