One can expect accessible lower bounds for dark matter detection rate due to restrictions on masses of the SUSY-partners. To explore this correlation one needs a new-generation large-mass detector. The absolute lower bound for detection rate can naturally be due to spin-dependent interaction. Aimed at detecting dark matter with sensitivity higher than $10^{-5}$ event/day/kg an experiment should have a non-zero-spin target. Perhaps, the best is to create a GENIUS-like detector with both Ge-73 (high spin) and Ge-76 nuclei
An energy threshold of (220 +/- 10) eV was achieved at an efficiency of 50% with a four-channel ultr...
We analyze the rate of detection of minimal supersymmetric neutralino dark matter in germanium, sapp...
We compare the rate for scattering of neutralinos from nuclei with the flux of muons induced by ener...
The recent WMAP data have confirmed that exotic dark matter together with the vacuum energy (cosmolo...
The Weakly Interacting Massive Particles (WIMPs) are among the main candidates for the relic dark ma...
We briefly review some theoretical issues involved in the direct detection of supersymmetric (SUSY) ...
International audienceWe examine the predictions for both the spin dependent and spin independentdir...
We performed a combined analysis of the parameter space of the Minimal Supersymmetric Standard Model...
A new set of supersymmetric benchmark scenarios has recently been proposed in the context of the con...
The present thesis, in the context of the direct detection of dark matter, focuses on the search for...
International audienceThe EDELWEISS Collaboration has performed a search for dark matter particles w...
All attempts to directly detect particle dark matter (DM) scattering on nuclei suffer from the parti...
Direct dark matter detection is considered in the Next-to-Minimal Supersymmetric Standard Model (NMS...
Predictions for the direct detection rates in a variety of models with dark natter candidates are su...
We calculate dark matter scattering rates in the minimal supersymmetric extension of the standard mo...
An energy threshold of (220 +/- 10) eV was achieved at an efficiency of 50% with a four-channel ultr...
We analyze the rate of detection of minimal supersymmetric neutralino dark matter in germanium, sapp...
We compare the rate for scattering of neutralinos from nuclei with the flux of muons induced by ener...
The recent WMAP data have confirmed that exotic dark matter together with the vacuum energy (cosmolo...
The Weakly Interacting Massive Particles (WIMPs) are among the main candidates for the relic dark ma...
We briefly review some theoretical issues involved in the direct detection of supersymmetric (SUSY) ...
International audienceWe examine the predictions for both the spin dependent and spin independentdir...
We performed a combined analysis of the parameter space of the Minimal Supersymmetric Standard Model...
A new set of supersymmetric benchmark scenarios has recently been proposed in the context of the con...
The present thesis, in the context of the direct detection of dark matter, focuses on the search for...
International audienceThe EDELWEISS Collaboration has performed a search for dark matter particles w...
All attempts to directly detect particle dark matter (DM) scattering on nuclei suffer from the parti...
Direct dark matter detection is considered in the Next-to-Minimal Supersymmetric Standard Model (NMS...
Predictions for the direct detection rates in a variety of models with dark natter candidates are su...
We calculate dark matter scattering rates in the minimal supersymmetric extension of the standard mo...
An energy threshold of (220 +/- 10) eV was achieved at an efficiency of 50% with a four-channel ultr...
We analyze the rate of detection of minimal supersymmetric neutralino dark matter in germanium, sapp...
We compare the rate for scattering of neutralinos from nuclei with the flux of muons induced by ener...