| Revision as of 19:41, 2 September 2018 editHeadbomb (talk | contribs)Edit filter managers, Autopatrolled, Extended confirmed users, Page movers, File movers, New page reviewers, Pending changes reviewers, Rollbackers, Template editors453,535 editsm →top: prep for bot, replaced: >[https://arxiv.org/abs/1508.07213 J. Amaré et al., Status of the ANAIS Dark Matter Project at the Canfranc Underground Laboratory, Contributed to the 11th Patras Workshop on Axions, WIMPs and WISPs, Zaragoza, JuneTag: AWB← Previous edit | Latest revision as of 06:46, 12 May 2022 edit undoChristian75 (talk | contribs)Extended confirmed users, New page reviewers, Pending changes reviewers, Rollbackers114,301 edits {{R with history}} | ||
| (11 intermediate revisions by 8 users not shown) | |||
| Line 1: | Line 1: | ||
| #REDIRECT ] | |||
| {{technical|date=October 2012}} | |||
| {{R with history}} | |||
| '''ANAIS''' is a ] experiment designed to detect ]. ANAIS stands for ''Annual modulation with NAI ]s''. Its main goal is the direct detection of the dark matter through its ] off the target nuclei in a radiopure ] crystal. This dark matter signal should be annually modulated by the change in the relative velocity of ]-], a result of the rotation of the Earth around the Sun. | |||
| ANAIS is the scaled conclusion of feasibility studies carried out with different prototypes by the ] group at the ], Spain. The complete experiment will use more than one hundred of kg of ultrapure ]-] NaI(Tl) crystals. Data recording began at the end of October 2012 using 25 kg in two prototype detectors as the last step before launching the larger experiment.<ref>, J. Amaré et al., Journal of Physics (Conference Series) 375 (2012) 01202</ref><ref>. S. Cebrián et al., Astropart. Phys. 37 (2012) 6</ref> A third detector was installed in 2014<ref></ref> showing a better radiopurity allowing the commissioning of the full experiment expected by mid-2016.<ref>https://www.arxiv.org/abs/1508.07213</ref> | |||
| ] and ],<ref> R.Bernabei et al. European Physical Journal C 56: 333, 2010</ref> experimental efforts performed at the ], accumulated more than thirteen annual cycles of data (also with NaI scintillators), obtaining a positive signal.<ref>.R.Bernabei et al. European Physical Journal C 67: 39, 2010</ref> Comparison of that result with negative results from other targets and experimental techniques is strongly model dependent. ANAIS (adopting the same target and technique that DAMA/LIBRA) appeared in the last roadmap of ApPEC<ref> {{webarchive |url=https://web.archive.org/web/20121213141219/http://www.aspera-eu.org/images/stories/roadmap/SAC-Roadmap-Nov-1-2011-final.pdf |date=December 13, 2012 }}</ref> (Astroparticle Physics European Coordination) to allow testing with an independent experimental set-up and in a model-independent way. | |||
| ==References== | |||
| {{Reflist}} | |||
| ==External links== | |||
| * | |||
| * | |||
| {{Dark matter}} | |||
| ] | |||
| ] | |||
Latest revision as of 06:46, 12 May 2022
Redirect to:
- With history: This is a redirect from a page containing substantive page history. This page is kept as a redirect to preserve its former content and attributions. Please do not remove the tag that generates this text (unless the need to recreate content on this page has been demonstrated), nor delete this page.
- This template should not be used for redirects having some edit history but no meaningful content in their previous versions, nor for redirects created as a result of a page merge (use {{R from merge}} instead), nor for redirects from a title that forms a historic part of Misplaced Pages (use {{R with old history}} instead).