World Library  
Flag as Inappropriate
Email this Article


Article Id: WHEBN0022693937
Reproduction Date:

Title: Edelweiss  
Author: World Heritage Encyclopedia
Language: English
Subject: Alps, Gebirgsjäger, Dark matter, 7th Mountain Division (Wehrmacht), Index of physics articles (E)
Publisher: World Heritage Encyclopedia



EDELWEISS (Expérience pour DEtecter Les Wimps En Site Souterrain) is a dark matter search experiment located in the Modane Underground Laboratory. The experiment uses cryogenic detectors, measuring both the phonon and ionization signals produced by particle interactions in germanium crystals. This technique allows nuclear recoils events to be distinguished from electron recoil events.

The EURECA project is a proposed future dark matter experiment, which will involve researchers from EDELWEISS and the CRESST dark matter search.

Dark matter

Dark matter is material which does not emit or absorb light. Measurements of the rotation curves of spiral galaxies suggest it makes up the majority of the mass of galaxies; and precision measurements of the cosmic microwave background radiation suggest it accounts for a significant fraction of the density of the Universe.

A possible explanation of dark matter comes from particle physics. WIMP (Weakly Interacting Massive Particle) is a general term for hypothetical particles which interact only through the weak nuclear and gravitational force. This theory suggests our galaxy is surrounded by a dark halo of such particles. EDELWEISS is one of a number of dark matter search experiments aiming to directly detect WIMP dark matter, by detecting the elastic scattering of a WIMP off an atom within a particle detector. As the interaction rate is so low, this requires sensitive detectors, good background discrimination, and a deep underground site (to reduce the background from cosmic rays).


EDELWEISS is located in the Modane underground laboratory, in the Fréjus road tunnel between France and Italy, below 1800m of rock. A 20 cm lead shield reduces the gamma background, and a polyethylene shield reduces the neutron flux. All materials close to the detectors are screened for radiopurity. A dilution refrigerator is used to cool the detectors, built in the opposite orientation to most instruments with the detectors at the top and the refrigeration mechanism below.

EDELWEISS uses high purity germanium cryogenic bolometers cooled to 20 milliKelvin above absolute zero. The phonon and ionization signals produced by a particle interaction are measured. This allows background events to be rejected as nuclear recoils events (produced by WIMP or neutron interactions) produce much less ionization than electron recoil events (produced by alpha, beta and gamma radiation). The detectors are similar to those used by the CDMS experiment. Simultaneous detection of ionization and heat with semiconductors at low temperature was an original idea by Lawrence M. Krauss, Mark Srednicki and Frank Wilczek.[1]

A major limitation of early detectors was the problem of surface events. Due to incomplete charge collection, a particle interaction near the surface of the crystal gave no ionization signal, so electron recoils near the surface could be mistaken for nuclear recoils. To avoid this, the collaboration developed new detectors with interdigitised electrodes. Different voltages are applied to a series of electrodes so the direction of electric field is different near the surface of the crystal, allowing over 99.5% of surface events to be rejected.[2]

The results from the first phase of the experiment (EDELWEISS I) were published in 2005, excluding WIMP dark matter with an interaction cross-section above ~10−6pb.[3] EDELWEISS-II ran 2009-2010, limiting high mass[4] and low mass WIMPs[5] and axions.[6] A cross-section of 4.4*10−8 pb is excluded at 90% C.L. for WIMP mass of 85 GeV. EDELWEISS-III, under construction, will have 40 detectors. EURECA design work will continue as EDELWEISS-III runs into 2015, operating after 2017.


EDELWEISS is a collaboration of the following member institutions:

CEA – Commissariat à l'Énergie Atomique

  • IRFU - Institut de Recherche sur les Lois Fondamentales de l'Univers
  • IRAMIS - Institut Rayonnement Matière de Saclay

CNRS – Centre National de la Recherche Scientifique

  • CSNSM - Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse, Orsay
  • IPNL - Institut de Physique Nucléaire de Lyon
  • Institut NÉEL, Grenoble
  • IAS - Institut d'Astrophysique Spatiale, Paris

Institutions outside France

See also


  1. ^ Krauss, L.; Srednicki, M.; Wilczek, F. (1986). "Solar System Constraints and Signatures for Dark Matter Candidates".  
  2. ^ Juillard, A. (2008). "Status of the EDELWEISS-II Experiment".  
  3. ^ Sanglard, V.; et al. (2005). "Final results of the EDELWEISS-I dark matter search with cryogenic heat-and-ionization Ge detectors".  
  4. ^ "Final results of the EDELWEISS-II WIMP search using a 4-kg array of cryogenic germanium detectors with interleaved electrodes". Physics Letters B 702 (2011) 329-335. 2012.  
  5. ^ "A search for low-mass WIMPs with EDELWEISS-II heat-and-ionization detectors". Phys. Rev. D86, 051701. 2012. 
  6. ^ "Axion searches with EDELWEISS-II". JCAP 1311 (2013) 067. 2013.  

External links

  • EDELWEISS Collaboration home page
  • EURECA Collaboration home page
This article was sourced from Creative Commons Attribution-ShareAlike License; additional terms may apply. World Heritage Encyclopedia content is assembled from numerous content providers, Open Access Publishing, and in compliance with The Fair Access to Science and Technology Research Act (FASTR), Wikimedia Foundation, Inc., Public Library of Science, The Encyclopedia of Life, Open Book Publishers (OBP), PubMed, U.S. National Library of Medicine, National Center for Biotechnology Information, U.S. National Library of Medicine, National Institutes of Health (NIH), U.S. Department of Health & Human Services, and, which sources content from all federal, state, local, tribal, and territorial government publication portals (.gov, .mil, .edu). Funding for and content contributors is made possible from the U.S. Congress, E-Government Act of 2002.
Crowd sourced content that is contributed to World Heritage Encyclopedia is peer reviewed and edited by our editorial staff to ensure quality scholarly research articles.
By using this site, you agree to the Terms of Use and Privacy Policy. World Heritage Encyclopedia™ is a registered trademark of the World Public Library Association, a non-profit organization.

Copyright © World Library Foundation. All rights reserved. eBooks from Hawaii eBook Library are sponsored by the World Library Foundation,
a 501c(4) Member's Support Non-Profit Organization, and is NOT affiliated with any governmental agency or department.