Speaker
FARINALDO queiroz
(International Institute of Physics -Natal)
Description
Dark matter complementarity is commonly thought of in terms of direct, indirect and collider searches. Indeed most dark matter models can be probed that way. However, if dark matter is very light or too heavy, or possesses velocity suppressed interactions, these techniques become not as effective. We will show that using neutron stars to realize a fourfold dark matter complementarity study we can again effectively probe the nature of dark matter.
Primary author
FARINALDO queiroz
(International Institute of Physics -Natal)
