Revision as of 00:51, 9 February 2015 editTrurle (talk | contribs)Autopatrolled, Extended confirmed users, Pending changes reviewers16,588 editsNo edit summary← 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}} | ||
(23 intermediate revisions by 15 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 250 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> | |||
] 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></ref> (Astroparticle Physics European Coordination) to allow testing with an independent experimental set-up and in a model-independent way. At the beginning of 2015, the calibration and testing of 25-kg setup was successfully completed, and plans were put forward to increase detector mass to either 100kg or directly to 250kg.<ref></ref> | |||
==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).