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ArDM

January 01, 1970

The ArDM (Argon Dark Matter) Experiment was a particle physics experiment based on a liquid argon detector, aiming at measuring signals from WIMPs (Weakly Interacting Massive Particles), which may constitute the Dark Matter in the universe. Elastic scattering of WIMPs from argon nuclei is measurable by observing free electrons from ionization and photons from scintillation, which are produced by the recoiling nucleus interacting with neighbouring atoms. The ionization and scintillation signals can be measured with dedicated readout techniques, which constituted a fundamental part of the detector.

In order to get a high enough target mass the noble gas argon was used in the liquid phase as target material. Since the boiling point of argon is at 87 K at normal pressure, the operation of the detector required a cryogenic system.

The ArDM experiment ended in 2019 when data taking was stopped and the experiment's apparatus decommissioned. The ArDM experiment's apparatus was then reused for another physics experiment, DArT (part of the DarkSide program), at Canfranc Underground Laboratory.[1]

ArDM did not find signals of dark matter particles.

Detecting WIMPs with argon edit

The ArDM detector aimed at directly detecting signals from WIMPs via elastic scattering from argon nuclei. During the scattering, a certain recoil energy - typically lying between 1 keV and 100 keV - is supposedly transferred from the WIMP to the argon nucleus.

It is not known how frequently a signal from WIMP-argon interaction can be expected (if at all). This rate depends on the properties of the WIMP. One of the most popular candidates for a WIMP is the Lightest Supersymmetric Particle (LSP) or neutralino from supersymmetric theories. Its cross section with nucleons presumably lies between 10−12 pb and 10−6 pb, making WIMP-nucleon interactions a rare event. The total event rate can be increased by optimizing the target properties, such as increasing the target mass. The ArDM detector was planned to contain approximately one ton of liquid argon. This target mass corresponded to an event rate of approximately 100 events per day at a cross section of 10−6 pb or 0.01 events per day at 10−10 pb.

Small event rates require a powerful background rejection. An important background for argon based detectors comes from the presence of the unstable 39Ar isotope in natural argon liquefied from the atmosphere. 39Ar undergoes beta decay with a halflife of 269 years and an endpoint of the beta spectrum at 565 keV. The ratio of ionization over scintillation from electron and gamma interactions is different than WIMP scattering should produce. The 39Ar background is therefore well distinguishable, with a precise determination of the ionization/scintillation ratio. As an alternative, the use of depleted argon from underground wells has been considered.

Neutrons emitted by detector components and by materials surrounding the detector interact with argon in the same way as the putative WIMPs. The neutron background is therefore nearly indistinguishable and has to be reduced as well as possible, as for example by carefully choosing the detector materials. Furthermore, an estimation or measurement of the remaining neutron flux is necessary.

The detector was run underground in order to avoid backgrounds induced by cosmic rays.

History edit

The ArDM detector was assembled and tested at CERN in 2006. Above ground studies of the equipment and detector performance were performed before it was moved underground in 2012 in the Canfranc Underground Laboratory in Spain. It was commissioned and tested at room temperature.[2] During the April 2013 run underground, the light yield was improved compared to surface conditions. Cold argon gas runs were planned as well as continued detector development. Liquid argon results were planned for 2014.

Beyond the one-ton version, the detector size can be increased without fundamentally changing its technology. A ten-ton liquid argon detector was considerex as an expansion possibility for ArDM. Experiments for Dark Matter detection at a mass scale of 1 kg to 100 kg with negative results demonstrated the necessity of ton-scale experiments.

Future Directions edit

 
Design of DarkSide-50 liquid argon dewar containing the two-phase TPC.

Despite studying inherently 'dark' matter, the future seems bright for dark matter detector development. The "Dark Side Program", of which ArDM was a member, is a consortium that has conducted and continues to develop new experiments based on condensed atmospheric argon (LAr), instead of xenon, liquid.[3] One recent Dark Side apparatus, the Dark Side-50 (DS-50), employs a method known as "two-phase liquid argon time projection chambers (LAr TPCs)," which allows for three-dimensional determination of collision event positions created by the electroluminescence created by argon collisions with dark matter particles.[4] The Dark Side program released its first results on its findings in 2015, so far being the most sensitive results for argon-based dark matter detection.[5] LAr-based methods used for future apparatuses present an alternative to xenon-based detectors and could potentially lead to new, more sensitive multi-ton detectors in the near future.[6]

References edit

  1. ^ https://lsc-canfranc.es/wp-content/uploads/2020/02/1906_ArDM_May2019_LSC_statusreport.pdf
  2. ^ Badertscher, A.; Bay, F.; Bourgeois, N.; Cantini, C.; Curioni, A.; Daniel, M.; Degunda, U.; Luise, S Di; Epprecht, L.; Gendotti, A.; Horikawa, S.; Knecht, L.; Lussi, D.; Maire, G.; Montes, B.; Murphy, S.; Natterer, G.; Nikolics, K.; Nguyen, K.; Periale, L.; Ravat, S.; Resnati, F.; Romero, L.; Rubbia, A.; Santorelli, R.; Sergiampietri, F.; Sgalaberna, D.; Viant, T.; Wu, S. (2013). "ArDM: first results from underground commissioning". JINST. 8 (9): C09005. arXiv:1309.3992. Bibcode:2013JInst...8C9005B. doi:10.1088/1748-0221/8/09/C09005. S2CID 118684007.
  3. ^ Rossi, B.; Agnes, P.; Alexander, T.; Alton, A.; Arisaka, K.; Back, H. O.; Baldin, B.; Biery, K.; Bonfini, G. (2016-07-01). "The DarkSide Program". EPJ Web of Conferences. 121: 06010. Bibcode:2016EPJWC.12106010R. doi:10.1051/epjconf/201612106010.
  4. ^ "DarkSide-50 detector". darkside.lngs.infn.it. Retrieved 2017-06-02.
  5. ^ The DarkSide Collaboration; Agnes, P.; Agostino, L.; Albuquerque, I. F. M.; Alexander, T.; Alton, A. K.; Arisaka, K.; Back, H. O.; Baldin, B. (2016-04-08). "Results from the first use of low radioactivity argon in a dark matter search". Physical Review D. 93 (8): 081101. arXiv:1510.00702. Bibcode:2016PhRvD..93h1101A. doi:10.1103/PhysRevD.93.081101. ISSN 2470-0010. S2CID 118655583.
  6. ^ Grandi, Luca. "grandilab.uchicago: dark matter search with noble liquid technology". grandilab.uchicago.edu. Retrieved 2017-06-02.

External links edit

  • ArDM web site

January 01, 1970
ardm, argon, dark, matter, experiment, particle, physics, experiment, based, liquid, argon, detector, aiming, measuring, signals, from, wimps, weakly, interacting, massive, particles, which, constitute, dark, matter, universe, elastic, scattering, wimps, from,. The ArDM Argon Dark Matter Experiment was a particle physics experiment based on a liquid argon detector aiming at measuring signals from WIMPs Weakly Interacting Massive Particles which may constitute the Dark Matter in the universe Elastic scattering of WIMPs from argon nuclei is measurable by observing free electrons from ionization and photons from scintillation which are produced by the recoiling nucleus interacting with neighbouring atoms The ionization and scintillation signals can be measured with dedicated readout techniques which constituted a fundamental part of the detector In order to get a high enough target mass the noble gas argon was used in the liquid phase as target material Since the boiling point of argon is at 87 K at normal pressure the operation of the detector required a cryogenic system The ArDM experiment ended in 2019 when data taking was stopped and the experiment s apparatus decommissioned The ArDM experiment s apparatus was then reused for another physics experiment DArT part of the DarkSide program at Canfranc Underground Laboratory 1 ArDM did not find signals of dark matter particles Contents 1 Detecting WIMPs with argon 2 History 3 Future Directions 4 References 5 External linksDetecting WIMPs with argon editThe ArDM detector aimed at directly detecting signals from WIMPs via elastic scattering from argon nuclei During the scattering a certain recoil energy typically lying between 1 keV and 100 keV is supposedly transferred from the WIMP to the argon nucleus It is not known how frequently a signal from WIMP argon interaction can be expected if at all This rate depends on the properties of the WIMP One of the most popular candidates for a WIMP is the Lightest Supersymmetric Particle LSP or neutralino from supersymmetric theories Its cross section with nucleons presumably lies between 10 12 pb and 10 6 pb making WIMP nucleon interactions a rare event The total event rate can be increased by optimizing the target properties such as increasing the target mass The ArDM detector was planned to contain approximately one ton of liquid argon This target mass corresponded to an event rate of approximately 100 events per day at a cross section of 10 6 pb or 0 01 events per day at 10 10 pb Small event rates require a powerful background rejection An important background for argon based detectors comes from the presence of the unstable 39Ar isotope in natural argon liquefied from the atmosphere 39Ar undergoes beta decay with a halflife of 269 years and an endpoint of the beta spectrum at 565 keV The ratio of ionization over scintillation from electron and gamma interactions is different than WIMP scattering should produce The 39Ar background is therefore well distinguishable with a precise determination of the ionization scintillation ratio As an alternative the use of depleted argon from underground wells has been considered Neutrons emitted by detector components and by materials surrounding the detector interact with argon in the same way as the putative WIMPs The neutron background is therefore nearly indistinguishable and has to be reduced as well as possible as for example by carefully choosing the detector materials Furthermore an estimation or measurement of the remaining neutron flux is necessary The detector was run underground in order to avoid backgrounds induced by cosmic rays History editThe ArDM detector was assembled and tested at CERN in 2006 Above ground studies of the equipment and detector performance were performed before it was moved underground in 2012 in the Canfranc Underground Laboratory in Spain It was commissioned and tested at room temperature 2 During the April 2013 run underground the light yield was improved compared to surface conditions Cold argon gas runs were planned as well as continued detector development Liquid argon results were planned for 2014 Beyond the one ton version the detector size can be increased without fundamentally changing its technology A ten ton liquid argon detector was considerex as an expansion possibility for ArDM Experiments for Dark Matter detection at a mass scale of 1 kg to 100 kg with negative results demonstrated the necessity of ton scale experiments Future Directions edit nbsp Design of DarkSide 50 liquid argon dewar containing the two phase TPC Despite studying inherently dark matter the future seems bright for dark matter detector development The Dark Side Program of which ArDM was a member is a consortium that has conducted and continues to develop new experiments based on condensed atmospheric argon LAr instead of xenon liquid 3 One recent Dark Side apparatus the Dark Side 50 DS 50 employs a method known as two phase liquid argon time projection chambers LAr TPCs which allows for three dimensional determination of collision event positions created by the electroluminescence created by argon collisions with dark matter particles 4 The Dark Side program released its first results on its findings in 2015 so far being the most sensitive results for argon based dark matter detection 5 LAr based methods used for future apparatuses present an alternative to xenon based detectors and could potentially lead to new more sensitive multi ton detectors in the near future 6 References edit https lsc canfranc es wp content uploads 2020 02 1906 ArDM May2019 LSC statusreport pdf Badertscher A Bay F Bourgeois N Cantini C Curioni A Daniel M Degunda U Luise S Di Epprecht L Gendotti A Horikawa S Knecht L Lussi D Maire G Montes B Murphy S Natterer G Nikolics K Nguyen K Periale L Ravat S Resnati F Romero L Rubbia A Santorelli R Sergiampietri F Sgalaberna D Viant T Wu S 2013 ArDM first results from underground commissioning JINST 8 9 C09005 arXiv 1309 3992 Bibcode 2013JInst 8C9005B doi 10 1088 1748 0221 8 09 C09005 S2CID 118684007 Rossi B Agnes P Alexander T Alton A Arisaka K Back H O Baldin B Biery K Bonfini G 2016 07 01 The DarkSide Program EPJ Web of Conferences 121 06010 Bibcode 2016EPJWC 12106010R doi 10 1051 epjconf 201612106010 DarkSide 50 detector darkside lngs infn it Retrieved 2017 06 02 The DarkSide Collaboration Agnes P Agostino L Albuquerque I F M Alexander T Alton A K Arisaka K Back H O Baldin B 2016 04 08 Results from the first use of low radioactivity argon in a dark matter search Physical Review D 93 8 081101 arXiv 1510 00702 Bibcode 2016PhRvD 93h1101A doi 10 1103 PhysRevD 93 081101 ISSN 2470 0010 S2CID 118655583 Grandi Luca grandilab uchicago dark matter search with noble liquid technology grandilab uchicago edu Retrieved 2017 06 02 External links editArDM web site Retrieved from https en wikipedia org w index php title ArDM amp oldid 1193640056, wikipedia, wiki, book, books, library,

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