Abstract. We study prospects of dark-matter direct-detection searches for probing non-relativistic effective theory for WIMP-baryon scattering. We simulate a large set of noisy recoil-energy spectra for different scattering scenarios (beyond the standard momentum-independent contact interaction), for Generation 2 and futuristic experiments. We analyze these simulations and quantify the probability of successfully identifying the operator govern-ing the scattering, if a WIMP signal is observed. We find that the success rate depends on a combination of factors: the WIMP mass, the mediator mass, the type of interaction, and the experimental energy window. For example, for a 20 GeV WIMP, Generation 2 is only likely to identify the right operato...
AbstractThe search for weakly-interacting massive particle (WIMP) dark matter is multi-pronged. Ulti...
International audienceAfter briefly summarizing the motivations for the A-CDM model, I will argue ra...
The primary observable in dark matter direct detection is the spectrum of scattering events. We simu...
A generic weakly interacting massive particle (WIMP) is one of the most attractive candidates to acc...
Leading candidates for non-baryonic Dark Matter are Weakly Interacting Massive Particles (WIMPs). Th...
Identifying the true theory of dark matter depends crucially on accurately characterizing interactio...
AbstractThe search for weakly-interacting massive particle (WIMP) dark matter is multi-pronged. Ulti...
The search for weakly-interacting massive particle (WIMP) dark matter is multi-pronged. Ulti- mately...
Abstract: Direct searches for WIMPs are sensitive to physics well below the weak scale. In the absen...
The search for weakly-interacting massive particle (WIMP) dark matter is multi-pronged. Ulti- mately...
Weakly interacting massive particles (WIMPs) form a promising solution to the dark matter problem an...
A great number of gravitational anomalies has been detected since the '30s of last century on galact...
Astrophysical observations indicate that about 23% of the energy density of the universe is in the f...
One of the most popular classes of candidates for dark matter are Weakly Interacting Massive Particl...
If the Milky Way’s DM halo is composed of WIMPs, then the WIMP flux on the Earth is of the order of...
AbstractThe search for weakly-interacting massive particle (WIMP) dark matter is multi-pronged. Ulti...
International audienceAfter briefly summarizing the motivations for the A-CDM model, I will argue ra...
The primary observable in dark matter direct detection is the spectrum of scattering events. We simu...
A generic weakly interacting massive particle (WIMP) is one of the most attractive candidates to acc...
Leading candidates for non-baryonic Dark Matter are Weakly Interacting Massive Particles (WIMPs). Th...
Identifying the true theory of dark matter depends crucially on accurately characterizing interactio...
AbstractThe search for weakly-interacting massive particle (WIMP) dark matter is multi-pronged. Ulti...
The search for weakly-interacting massive particle (WIMP) dark matter is multi-pronged. Ulti- mately...
Abstract: Direct searches for WIMPs are sensitive to physics well below the weak scale. In the absen...
The search for weakly-interacting massive particle (WIMP) dark matter is multi-pronged. Ulti- mately...
Weakly interacting massive particles (WIMPs) form a promising solution to the dark matter problem an...
A great number of gravitational anomalies has been detected since the '30s of last century on galact...
Astrophysical observations indicate that about 23% of the energy density of the universe is in the f...
One of the most popular classes of candidates for dark matter are Weakly Interacting Massive Particl...
If the Milky Way’s DM halo is composed of WIMPs, then the WIMP flux on the Earth is of the order of...
AbstractThe search for weakly-interacting massive particle (WIMP) dark matter is multi-pronged. Ulti...
International audienceAfter briefly summarizing the motivations for the A-CDM model, I will argue ra...
The primary observable in dark matter direct detection is the spectrum of scattering events. We simu...