|
Résumé |
Minimal self-consistent scenarios with light (sub-GeV) dark matter are usually
accompanied by a correspondingly light "dark sector". The presence of the
latter leads to bright detection prospects at fixed target experiments and
colliders and potentially strong astrophysical bounds. We will illustrate this
point by exploring explicitly a typical simple fermion dark matter setup,
examining in particular the key role of the dark sector in the interplay
between accelerator searches and astrophysical signatures.
|
