Fri May 9 , 12:30 PM in Miller Room
Roberto Trotta , Oxford University
Astrophysical probes of dark matter
The nature and properties of dark matter are one of the outstanding
questions in cosmology. A well-motivated cold dark matter candidate
is the lightest supersymmetric particle, the neutralino, whose properties
however might remain underconstrained even if supersymmetry is
discovered at the LHC in the next few years.
In this talk I will present results from the most complete analysis of
the Constrained Minimal Supersymmetric Standard Model (CMSSM)
parameter space to date, showing that direct detection experiments
have the potential to discover neutralino dark matter by the end of the
decade if the CMSSM framework is correct. I will highlight the
complementarity between direct dark matter searches, collider
experiments (LHC, Tevatron) and indirect searches for annhilation
signatures (gamma ray and antimatter fluxes) in the search for
supersymmetric particles. I will make the case for the necessity of
a convergent approach, combining astrophysical and collider probes,
to the problem of dark matter.
Host: Harsh Mathur