Bounds on annual modulation signal in dark matter direct detection
I will show constraints on the annual modulation signal in
Dark Matter direct detection experiments which assume only very
general properties of dark matter halo. The derivation of the bound
uses an expansion in the earth velocity and is expressed in terms of
the unmodulated event rate. I will illustrate the bounds by applying
them to the annual modulation signals reported by the DAMA and CoGeNT
experiments in the framework of spin-independent elastic scattering.
While the DAMA signal satisfies our bounds, severe restrictions on the
DM mass can be set for CoGeNT. Finally, I will also review the
constraints on light dark matter interpretation of the CRESST-II
results.
Oct 9 at 4pm in Geo/Phys Room 407