International audienceWe discuss the consequences of the accretion of dark matter (DM) particles on compact stars such as white dwarfs and neutron stars. We show that in large regions of the DM parameter space, these objects are sensitive probes of the presence of DM and can be used to set constraints both on the DM density and on the physical properties of DM particles
Abstract. We report recent results on the impact of asymmetric dark matter (DM) particles on low-mas...
International audienceThe existence of cosmological dark matter is in the bedrock of the modern cosm...
The white dwarf luminosity function, which provides information about their cooling, has been measur...
We discuss the consequences of the accretion of dark matter (DM) particles on compact stars such as ...
Probing the existence of hypothetical particles beyond the Standard model often deals with extreme p...
There is by now compelling evidence that most of the matter in the universe is in the form of dark m...
We study the effects of feebly or nonannihilating weakly interacting dark matter (DM) particles on s...
We study the impact of asymmetric bosonic dark matter on neutron star properties, including possible...
International audienceWe study the effects of feebly or nonannihilating weakly interacting dark matt...
In the ΛCDM model, ≈ 26% of the matter-energy content of the Universe is in the form of an unidentif...
In the context of the standard model of particle physics, there is a definite upper limit to the den...
Trabajo presentado en el Seminar at AstroCoffee ITP-FIAS (Astrophysics@GU), celebrado en Frankfurt o...
White dwarfs (WDs) are the most promising captors of dark matter (DM) particles in the crests that a...
We present a study of neutron star models that contain dark matter (DM) in the core. The DM is assum...
Although many independent astrophysical and cosmological observations imply the existenceof a new da...
Abstract. We report recent results on the impact of asymmetric dark matter (DM) particles on low-mas...
International audienceThe existence of cosmological dark matter is in the bedrock of the modern cosm...
The white dwarf luminosity function, which provides information about their cooling, has been measur...
We discuss the consequences of the accretion of dark matter (DM) particles on compact stars such as ...
Probing the existence of hypothetical particles beyond the Standard model often deals with extreme p...
There is by now compelling evidence that most of the matter in the universe is in the form of dark m...
We study the effects of feebly or nonannihilating weakly interacting dark matter (DM) particles on s...
We study the impact of asymmetric bosonic dark matter on neutron star properties, including possible...
International audienceWe study the effects of feebly or nonannihilating weakly interacting dark matt...
In the ΛCDM model, ≈ 26% of the matter-energy content of the Universe is in the form of an unidentif...
In the context of the standard model of particle physics, there is a definite upper limit to the den...
Trabajo presentado en el Seminar at AstroCoffee ITP-FIAS (Astrophysics@GU), celebrado en Frankfurt o...
White dwarfs (WDs) are the most promising captors of dark matter (DM) particles in the crests that a...
We present a study of neutron star models that contain dark matter (DM) in the core. The DM is assum...
Although many independent astrophysical and cosmological observations imply the existenceof a new da...
Abstract. We report recent results on the impact of asymmetric dark matter (DM) particles on low-mas...
International audienceThe existence of cosmological dark matter is in the bedrock of the modern cosm...
The white dwarf luminosity function, which provides information about their cooling, has been measur...