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 …

Very compact objects probe extreme gravitational fields and may be the key to understand
outstanding puzzles in fundamental physics. These include the nature of dark matter, the …

We demonstrate in a general and analytic way how high-density information about the
equation of state (EOS) of strongly interacting matter obtained using perturbative quantum …

70 AIM, UMR 7158, CEA/DRF, CNRS, Université Paris Diderot, Irfu/Service d'Astrophysique,
Centre de Saclay, FR-91191 Gif-sur-Yvette, France

We review theories of Asymmetric Dark Matter (ADM), their cosmological implications and
detection. While there are many models of ADM in the literature, our review of existing …

Asymmetric dark matter models are based on the hypothesis that the present-day
abundance of dark matter has the same origin as the abundance of ordinary or" visible" …

In this review article, we discuss the current status of particle dark matter, including
experimental evidence and theoretical motivations. We discuss a wide array of candidates …

Isolated ideal neutron stars (NS) of age> 10 9 yr exhaust thermal and rotational energies
and cool down to temperatures below O (100) K. Accretion of particle dark matter (DM) by …

We present a search for subsolar mass ultracompact objects in data obtained during
Advanced LIGO's second observing run. In contrast to a previous search of Advanced LIGO …

Various extensions of the standard model of elementary particle interactions predict the
existence of new particles such as axions, or “exotic” properties of known particles such as …