From Surf Wiki (app.surf) — the open knowledge base
DarkSide (dark matter experiment)
| Field | Value |
|---|---|
| full_name | DarkSide |
| purpose | Detecting dark matter in the form of WIMPs |
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 in order to exclude the radioactive isotope , which makes up one in every 1015 (quadrillion) atoms in atmospheric argon. 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 (20,000 kg) of liquid argon is being planned as of 2019.
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.
Status
Darkside-50 has 46 kg argon target mass. A 3-year run is planned and ton-scale expansion has been proposed.
Initial results using a month of running were reported in 2014. Spin-independent limits were set using 1422 kg×days of exposure to atmospheric argon. A cross section limit of for a 100 Gev WIMP was found.
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 Alberta, Canada
- 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
- GSSI – Gran Sasso Science Institute, 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
References
Publications
- DarkSide Collaboration, "DarkSide-50 Proposal " (2008).
References
- Lofholm, Nancy. (5 October 2012). "Colorado argon will be at the heart of dark matter experiment". Denver Post.
- "Low-background Argon from underground reservoir". DarkSide collaboration.
- (2012-05-31). "The DarkSide of Gran Sasso".
- (2015). "First Results from the DarkSide-50 Dark Matter Experiment at Laboratori Nazionali del Gran Sasso". Physics Letters B.
This article was imported from Wikipedia and is available under the Creative Commons Attribution-ShareAlike 4.0 License. Content has been adapted to SurfDoc format. Original contributors can be found on the article history page.
Ask Mako anything about DarkSide (dark matter experiment) — get instant answers, deeper analysis, and related topics.
Research with MakoFree with your Surf account
Create a free account to save articles, ask Mako questions, and organize your research.
Sign up freeThis content may have been generated or modified by AI. CloudSurf Software LLC is not responsible for the accuracy, completeness, or reliability of AI-generated content. Always verify important information from primary sources.
Report