The dark matter phenomenon is the realisation that astrophysical and
cosmological observations appear to indicate invisible mass sources.
There are many candidates that could account for dark matter; among
the most prominent proposals are weakly interacting massive particles
(WIMPs), feebly interacting massive particles (FIMPs), and Primordial
Black Holes (PBH). I will start by briefly outlining the case for dark
matter and each of these proposed resolutions. Subsequently, I will
discuss the idea that cosmology may give rise to appreciable
populations of both particle dark matter (WIMPs/FIMPs) and PBH with
the combined mass density providing the observationally inferred value
of the dark matter abundance today. In particular, I will highlight
that dark matter particles will generically form halos around the PBH
leading to enhanced constraints on this scenario from indirect
detection searches.