DarkSide (dark matter experiment)

The DarkSide collaboration is an international affiliation of universities and labs seeking to directly detect dark matter in the form of weakly interacting massive particles (WIMPs). The collaboration is planning, building and operating a series of liquid argon time projection chambers (TPCs) that are employed at the Gran Sasso National Laboratory in Assergi, Italy. The detectors are filled with liquid argon from underground sources^[1] in order to exclude the radioactive isotope ³⁹
Ar, which makes up one in every 10¹⁵ (quadrillion) atoms in atmospheric argon.^[2] The Darkside-10 (DS-10) prototype was tested in 2012, and the Darkside-50 (DS-50) experiment has been operating since 2013. Darkside-20k (DS-20k) with 20 tonnes of liquid argon is being planned as of 2019.^{[citation needed]}

DarkSide

DarkSide
Purpose	Detecting dark matter in the form of WIMPs

Darkside-10

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
• INFN – Università degli Studi di Genova, Italy
• INFN – Università degli Studi di Milano, Italy
• INFN – Università degli Studi di Napoli, Italy
• INFN – Università degli Studi di Perugia, Italy
• INFN – Università degli Studi di Cagliari, Italy
• CERN – The European Organization for Nuclear Research, Switzerland/France
• Jagiellonian University, Cracow, Poland
• Belgorod State University, Russia
• Joint Institute for Nuclear Research, Dubna, Russia
• Lomonosov Moscow State University, Russia
• Novosibirsk State University, Russia
• 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
• Institute for Nuclear Research of NASU, Kyiv, Ukraine

See also

• ANAIS
• ArDM
• CDEX
• CDMS
• CRESST
• DAMA/NaI
• DAMA/LIBRA
• DEAP
• DRIFT
• EDELWEISS
• LZ experiment
• LUX
• PICASSO
• SIMPLE
• WARP
• XENON
• ZEPLIN

References

1. Lofholm, Nancy (5 October 2012). "Colorado argon will be at the heart of dark matter experiment". Denver Post.
2. "Low-background Argon from underground reservoir". DarkSide collaboration. Archived from the original on 2016-07-23.
3. "The DarkSide of Gran Sasso". CERN Courier. 2012-05-31. Retrieved 2021-06-19.
4. Agnes, P.; et al. (2015). "First Results from the DarkSide-50 Dark Matter Experiment at Laboratori Nazionali del Gran Sasso". Physics Letters B. 743 (456): 456–466. arXiv:1410.0653. Bibcode:2015PhLB..743..456A. doi:10.1016/j.physletb.2015.03.012. S2CID 119112092.

Publications

• 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. arXiv:1204.6011. Bibcode:2015APh....66...53X. doi:10.1016/j.astropartphys.2015.01.002. 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. arXiv:1010.3609. Bibcode:2011NIMPA.644...18W. doi:10.1016/j.nima.2011.04.009. 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. arXiv:0712.0381. Bibcode:2008JPhCS.120d2015G. doi:10.1088/1742-6596/120/4/042015. S2CID 118355785.

External links

• Official website