Searching for Dark Matter in Unification Models A Hint from Indirect Sensitivities towards.pdf
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Searching for Dark Matter in Unification Models A Hint from Indirect Sensitivities towards
hep-ph/0610272
UMN–TH–2518/06
FTPI–MINN–06/31
September 2006
Searching for Dark Matter in Unification
Models: A Hint from Indirect Sensitivities
6
0 towards Future Signals in
0
2 Direct Detection and B-decays1
t
c
O Keith A. Olive
0
2 William I Fine Theoretical Physics Institute,
University of Minnesota, Minneapolis, MN 55455, USA
1
v
2 Abstract. A comparison is made between accelerator and direct detection constraints in con-
7 strained versions of the minimal supersymmetric standard model. Models considered are based on
2 mSUGRA, where scalar and gaugino masses are unified at the GUT scale. In addition, the mSUGRA
0 relation between the (unified) A and B parameters is assumed, as is the relation between m0 and
1 the gravitino mass. Also considered are models where the latter two conditions are dropped (the
6 CMSSM), and a less constrained version where the Higgs soft masses are not unified at the GUT
0 scale (the NUHM).
/
h Keywords: Dark Matter; Supersymmetry
p- PACS: 11.30Pb, 13.25.Hw, 95.35.+d, 98.80.-k
p
e
h UNIFICATION MODELS
:
v
i
X As constraints from accelerator searches and direct detection experiments improve, and
r in anticipation of the
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