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RESEARCH PRODUCT
Status of the EDELWEISS experiment
B. ChambonJ. ManginN. MirabolfathiA. JuillardM. SternP. Di StefanoLino MiramontiD. DrainP. GarocheS. PécourtM. GrosL. MoscaX-f. NavickA. De LesquenP. PariG. NollezJ.-p. TorreC. GoldbachS. MarnierosLaurent BergéP. CharvinP. CharvinE. SimonJ. GasconG. ChardinL. DumoulinD. YvonM. De JesusM. ChapellierAlain BenoitJ. MalletA. BroniatowskiD. L'hotesubject
CryostatPhysicsNuclear and High Energy Physics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]Dark matterBolometerDetectorCosmic rayEDELWEISSAtomic and Molecular Physics and OpticsParticle detectorlaw.invention[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Nuclear physicsWIMPlaw[SDU]Sciences of the Universe [physics]Measuring instrumentInstrumentationEvent (probability theory)description
The Edelweiss Dark Matter Experiment is installed in the Modane Underground Laboratory since 1994. In 1997 the first detector of a 70 g heat and ionization Ge low-temperature detector built by the collaboration showed its discrimination capabilities. During the last two years the installation was upgraded, and a new generation of 70 g Ge detectors is operational. The detector environment is drastically controlled to avoid radioactive contamination. A test run with two new 70 g detectors shows a reduction by a factor of ten in the background level before 7-ray rejection which is now around 2 events/kg/keV/day. Three 320 g Ge cryogenic detectors have been constructed and are now being tested and should soon be operational in the present cryostat. A new cryostat is being built and will allow a detection volume of 100 1. It is expected to be installed in Modane next year. In a first step of 21×320 g Ge detectors, the Edelweiss-II experiment should test an important fraction of the MSSM Susy parameter space.
year | journal | country | edition | language |
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1999-08-15 |