Abstract Several interesting Dark Matter (DM) models invoke a dark sector leading to two
types of relic particles, possibly interacting with each other: non-relativistic DM, and …

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 …

The Simons Observatory (SO) is a ground-based cosmic microwave background (CMB)
experiment sited on Cerro Toco in the Atacama Desert in Chile that promises to provide …

The Probe of Inflation and Cosmic Origins (PICO) is an imaging polarimeter that will scan the
sky for 5 years in 21 frequency bands spread between 21 and 799 GHz. It will produce full …

We generalize the formalism for DM capture in celestial bodies to account for arbitrary
mediator mass, and update the existing and projected astrophysical constraints on DM …

Advances in experimental techniques make it possible to map the high redshift Universe in
three dimensions at high fidelity in the near future. This will increase the observed volume by …

In this work we investigate the possibility that dark matter and (massive) neutrinos can
interact via a simple, constant cross section. Building on previous numerical efforts, we …

We use the latest measurements of the Milky Way satellite population from the Dark Energy
Survey and Pan-STARRS1 to infer the most stringent astrophysical bound to date on velocity …

We explore an interacting dark matter (IDM) model that allows for a fraction of dark matter
(DM) to undergo velocity-independent scattering with baryons. In this scenario, structure on …

Critical probes of dark matter come from tests of its elastic scattering with nuclei. The results
are typically assumed to be model independent, meaning that the form of the potential need …