2013/05/13 by В. Козлов, Kozlov, V. Y.
Physics and Astronomy · #Cosmology and Nongalactic Astrophysics (astro-ph.CO) #Dark Matter and Cosmic Phenomena #FOS: Physical sciences #Instrumentation and Detectors (physics.ins-det) #Instrumentation and Methods for Astrophysics (astro-ph.IM) #Particle Detector Development and Performance #Superconducting and THz Device Technology
paper · pdf · doi:10.48550/arxiv.1305.2808
openalex publication_date 2013/05/13 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
The Edelweiss experiment uses Ge-bolometers with an improved background rejection (interleaved electrode design) to search for WIMP dark matter. The setup is located in the underground laboratory, Laboratoire Souterrain de Modane (LSM, France). In 2009-2010 the collaboration successfully operated ten 400-g bolometers together with an active muon veto shielding. Published analysis of this measurement campaign was optimized for WIMP masses above 50 GeV. Recently, the analysis was extended to the low-mass WIMP region using a quality subset of the 2009-2010 data setting new limits on the spin-independent WIMP-nucleon scattering cross-section. We present the low-mass WIMP analysis, background investigations and the latest measurements with a subset of the forty 800-g detectors that will be installed for the Edelweiss-III. Ongoing installation works of the Edelweiss-III setup and further plans for a next generation experiment, EURECA, are discussed.