Enhancement of Line Gamma Ray Signature from Bino-like Dark Matter   Annihilation due to CP Violation
  We study the line gamma ray signature from the Galactic Center originating from Bino-like dark matter pair annihilation, when CP is not conserved. We consider the case that the Bino is nearly degenerate with a sfermion in mass. Although an indirect detection of Bino-like dark matter is difficult in general, the signal of Bino-like dark matter pair annihialtion in this case is enormously enhanced due to the threshold singularity. 
Shigeki Matsumoto, Joe Sato, Yoshio Sato