We introduce a new paradigm for dark matter (DM) interactions in which the interaction strength is asymptotically safe. In models of this type, the coupling strength is small at low energies but increases at higher energies, and asymptotically approaches a finite constant value. The resulting phenomenology of this "asymptotically safe DM" is quite distinct. One interesting effect of this is to partially offset the low-energy constraints from direct detection experiments without affecting thermal freeze-out processes which occur at higher energies. High-energy collider and indirect annihilation searches are the primary ways to constrain or discover safe dark matter
Dark matter (DM) may belong to a hidden sector (HS) that is only feebly interacting with the standar...
We study the possible signals at LHC of the minimal models of decaying dark matter. Those models are...
I will discuss some phenomenological consequences of extensions of the Standard Model containing a m...
We introduce a new paradigm for dark matter (DM) interactions in which the interaction strength is a...
It is argued that experimental constraints on theories of asymmetric dark matter (ADM) almost certai...
We discuss a class of Dark Matter (DM) models that, although inherently strongly coupled, appear wea...
It is argued that experimental constraints on theories of asymmetric dark matter (ADM) almost certai...
Abstract We explore the Renormalization Group flow of massive uncharged fermions — a candidate for d...
12 pages. Invited talk at DARK 2002, 4th Int. Conf. on Dark Matter in Astro and Particle Physics, Ca...
Dark matter (DM) coupled to light mediators has been invoked to resolve the putative discrepancies ...
The two dark sectors of the universe - dark matter and dark energy - may interact with each other. B...
Abstract. Asymmetric Dark Matter (ADM) models invoke a particle-antiparticle asymme-try, similar to ...
We present kinematically forbidden dark matter annihilations into Standard Model leptons. This mecha...
The two dark sectors of the universe - dark matter and dark energy - may interact with each other. B...
International audienceWe present kinematically forbidden dark matter annihilations into Standard Mod...
Dark matter (DM) may belong to a hidden sector (HS) that is only feebly interacting with the standar...
We study the possible signals at LHC of the minimal models of decaying dark matter. Those models are...
I will discuss some phenomenological consequences of extensions of the Standard Model containing a m...
We introduce a new paradigm for dark matter (DM) interactions in which the interaction strength is a...
It is argued that experimental constraints on theories of asymmetric dark matter (ADM) almost certai...
We discuss a class of Dark Matter (DM) models that, although inherently strongly coupled, appear wea...
It is argued that experimental constraints on theories of asymmetric dark matter (ADM) almost certai...
Abstract We explore the Renormalization Group flow of massive uncharged fermions — a candidate for d...
12 pages. Invited talk at DARK 2002, 4th Int. Conf. on Dark Matter in Astro and Particle Physics, Ca...
Dark matter (DM) coupled to light mediators has been invoked to resolve the putative discrepancies ...
The two dark sectors of the universe - dark matter and dark energy - may interact with each other. B...
Abstract. Asymmetric Dark Matter (ADM) models invoke a particle-antiparticle asymme-try, similar to ...
We present kinematically forbidden dark matter annihilations into Standard Model leptons. This mecha...
The two dark sectors of the universe - dark matter and dark energy - may interact with each other. B...
International audienceWe present kinematically forbidden dark matter annihilations into Standard Mod...
Dark matter (DM) may belong to a hidden sector (HS) that is only feebly interacting with the standar...
We study the possible signals at LHC of the minimal models of decaying dark matter. Those models are...
I will discuss some phenomenological consequences of extensions of the Standard Model containing a m...