Orateur
Geraldine Servant
(CERN)
Description
In some classes of WIMP models, the Higgs boson could be copiously produced in association
with a photon from dark matter annihilations in the center of our galaxy. The resulting photon spectrum
possesses a line whose energy reflects the mass of the Higgs and of the WIMP and whose intensity
depends on the WIMP spin and statistics. I will discuss how gamma-ray telescopes such as Fermi
could provide information on the Higgs and dark matter complementary to that obtained at the LHC.
Author
Geraldine Servant
(CERN)
