Cherenkov Telescope Array will test whether pulsars generate the Galactic Center gamma-ray excess
Cherenkov Telescope Array will test whether pulsars generate the Galactic Center gamma-ray excess
The GeV-scale gamma-ray excess observed from the region surrounding the Galactic Center has been interpreted as either the products of annihilating dark matter particles, or as the emission from a large population of faint and centrally-located millisecond pulsars. If pulsars are responsible for this signal, they should also produce detectable …