DarkSide (dark matter experiment)

The DarkSide collaboration is an international affiliation of universities and labs seeking to directly detect

The Darkside-10 prototype detector had 10 kg of liquid argon. It was built at Princeton University and operated there for seven months, after which it was transported to Gran Sasso National Laboratory in 2011. The detector operated in Gran Sasso 2011-2012.^{[3][additional citation(s) needed]}

Status

Darkside-50 has 46 kg argon target mass. A 3-year run is planned and ton-scale expansion has been proposed.^{[citation needed]}

Initial results using a month of running were reported in 2014.^[4] Spin-independent limits were set using 1422 kg×days of exposure to atmospheric argon. A cross section limit of 6.1×10⁻⁴⁴ cm² for a 100 Gev WIMP was found.^[4]

Members

The following institutions' physics departments include members of DarkSide:

• Augustana College
  , USA
• Black Hills State University, USA
• Drexel University, USA
• Fermi National Accelerator Laboratory
  , USA
• The University of Chicago
  , USA
• Princeton University, USA
• Temple University, USA
• University of Arkansas, USA
• University of California at Los Angeles
  , USA
• University of California at Davis
  , USA
• University of Houston, USA
• University of Massachusetts at Amherst
  , USA
• University of Hawaii
  , USA
• Virginia Tech, USA
• Williams College, USA
• Fort Lewis College, USA
• University College of London
  , GB
• University of Oxford, GB
• Royal Holloway, University of London, GB
• INFN – Laboratori Nazionali del Gran Sasso
  , Italy
• Università degli Studi di Genova
  , Italy
• Università degli Studi di Milano
  , Italy
• Università degli Studi di Napoli
  , Italy
• Università degli Studi di Perugia
  , Italy
• Università degli Studi di Cagliari
  , Italy
• CERN – The European Organization for Nuclear Research, Switzerland/France
• Jagiellonian University, Cracow, Poland
• Joint Institute for Nuclear Research, Dubna, Russia
• Lomonosov Moscow State University
  , Russia
• Novosibirsk State University, Russia
• Institute for Nuclear Research of NASU
  , Kiev, Ukraine
• RRC Kurchatov Institute, Russia
• National Research Nuclear University
  , Moscow, Russia
• Institute for Theoretical and Experimental Physics, Moscow, Russia
• St. Petersburg Nuclear Physics Institute, Gatchina, Russia

See also

References

• Akimov, D.; et al. (2012). "Light Yield in DarkSide-10: A Prototype Two-phase Liquid Argon TPC for Dark Matter Searches".
  arXiv:1204.6218v1 [astro-ph.IM
  ].
• Back, H. O.; et al. (2012). "First Large Scale Production of Low Radioactivity Argon from Underground Sources".
  arXiv:1204.6024 [astro-ph.IM
  ].
• Back, H. O.; et al. (2012). "First Commissioning of a Cryogenic Distillation Column for Low Radioactivity Underground Argon".
  arXiv:1204.6061v2 [astro-ph.IM
  ].
• Xu, J.; et al. (2015). "A study of the trace ³⁹Ar content in argon from deep underground sources". Astroparticle Physics. 66: 53–60.
  S2CID 117711599
  .
• Wright, Alex; Mosteiro, Pablo; Loer, Ben; Calaprice, Frank (2011). "A highly efficient neutron veto for dark matter experiments". Nuclear Instruments and Methods in Physics Research Section A. 644 (1): 18–26.
  S2CID 118467340
  .
• DarkSide Collaboration, “DarkSide-50 Proposal Archived 2013-02-24 at the Wayback Machine” (2008).
• Galbiati, C.; et al. (2008). "Discovery of underground argon with a low level of radioactive ³⁹Ar and possible applications to WIMP dark matter detectors". Journal of Physics: Conference Series. 120 (4): 042015.
  S2CID 118355785
  .

• Official website