WDs and neutron stars are far-reaching and multi-faceted laboratories in the hunt for dark
matter. We review detection prospects of wave-like, particulate, macroscopic and black hole …

It is commonly assumed that the energy density of the Universe was dominated by radiation
between reheating after inflation and the onset of matter domination 54,000 years later …

While astrophysical and cosmological probes provide a remarkably precise and consistent
picture of the quantity and general properties of dark matter, its fundamental nature remains …

We consider mechanisms for producing a significant population of primordial black holes
(PBHs) within string inspired single field models of inflation. The production of PBHs …

In many cosmologies dark matter clusters on subkiloparsec scales and forms compact
subhalos, in which the majority of Galactic dark matter could reside. Null results in direct …

Pulsars act as accurate clocks, sensitive to gravitational redshift and acceleration induced by
transiting clumps of matter. We study the sensitivity of pulsar timing arrays (PTAs) to single …

Gravitational dark matter (DM) is the simplest possible scenario that has recently gained
interest in the early Universe cosmology. In this scenario, DM is assumed to be produced …

There is a large and growing interest in observations of small-scale structure in dark matter.
We propose a new way to probe dark matter structures in the∼ 10–10 8 M⊙ range. This …

A thermally decoupled hidden sector of particles, with a mass gap, generically enters a
phase of cannibalism in the early Universe. The Standard Model sector becomes …

A bstract Models of Dark Matter (DM) can leave unique imprints on the Universe's small
scale structure by boosting density perturbations on small scales. We study the capability of …