A. Menshikov

A search for low-mass WIMPs with EDELWEISS-II heat-and-ionization detectors

We report on a search for low-energy (E < 20 keV) WIMP-induced nuclear recoils using data collected in 2009 - 2010 by EDELWEISS from four germanium detectors equipped with thermal sensors and an electrode design (ID) which allows to efficiently reject several sources of background. Using an exposure of 113 kg.d, we find no evidence for an exponential distribution of low-energy nuclear recoils that could be attributed to WIMP elastic scattering. For WIMPs of mass 10 GeV, the observation of one event in the WIMP search region results in a 90% CL limit of 1.0 \times 10^-5 pb on the spin-independent WIMP-nucleon scattering cross-section, which constrains the parameter space associated with the findings reported by the CoGeNT, DAMA and CRESST experiments.

Axion searches with the EDELWEISS-II experiment

We present new constraints on the couplings of axions and more generic axion-like particles using data from the EDELWEISS-II experiment. The EDELWEISS experiment, located at the Underground Laboratory of Modane, primarily aims at the direct detection of WIMPs using germanium bolometers. It is also sensitive to the low-energy electron recoils that would be induced by solar or dark matter axions. Using a total exposure of up to 448 kg.d, we searched for axion-induced electron recoils down to 2.5 keV within four scenarios involving different hypotheses on the origin and couplings of axions. We set a 95% CL limit on the coupling to photons

Background studies for the EDELWEISS dark matter experiment

g_{A\gamma}<2.13\times 10^{-9}

Constraints on low-mass WIMPs from the EDELWEISS-III dark matter search

GeV

Hardware setup for the next generation of 3D Ultrasound Computer Tomography

^{-1}

Development and underground test of radiopure ZnMoO4 scintillating bolometers for the LUMINEU 0 nu 2 beta project

in a mass range not fully covered by axion helioscopes. We also constrain the coupling to electrons,

FPGA-based DAQ system for multi-channel detectors

g_{Ae} < 2.56\times 10^{-11}

Statistical current monitor for the cosmic ray experiment Pierre Auger

, similar to the more indirect solar neutrino bound. Finally we place a limit on

Performance of the EDELWEISS-III experiment for direct dark matter searches

g_{Ae}\times g_{AN}^{\rm eff}<4.70 \times 10^{-17}

LUMINEU: a search for neutrinoless double beta decay based on ZnMoO4 scintillating bolometers

, where