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darkside experiment Archive
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2016: Results from the first use of low radioactivity argon in a dark matter search
Posted on April 20, 2016 | No CommentsPhys. Rev. D 93, 081101(R) P. Agnes et al. (DarkSide Collaboration) M. Wójcik, G. Zuzel & K. Pelczar Download http://dx.doi.org/10.1103/PhysRevD.93.081101 Abstract Liquid argon is a bright scintillator with potent particle... -
2015: First results from the DarkSide-50 dark matter experiment at Laboratori Nazionali del Gran Sasso
Posted on February 17, 2016 | No CommentsPhysics Letters. B, 2015 vol. 743, p. 456-466 Agnes P., et al. (Dark-Side Collaboration) M. Wójcik, G. Zuzel, K. Pelczar Download http://dx.doi.org/10.1016/j.physletb.2015.03.012 Abstract We report the first results of DarkSide-50,... -
2015: The DarkSide multiton detector for the direct dark matter search
Posted on February 17, 2016 | No CommentsAdvances in High Energy Physics, 2015 vol. 2015 Aalseth C. et al. (Dark-Side Collaboration) M. Wójcik, G. Zuzel, K. Pelczar, A. Odrzywołek Download http://dx.doi.org/10.1155/2015/541362 Abstract Although the existence of dark... -
2013: Light yield in DarkSide-10: A prototype two-phase argon TPC for dark matter searches
Posted on June 3, 2012 | No CommentsAstroparticle Physics Volume 49, September 2013, Pages 44–51 T. Alexander et al., (DarkSide Collaboration) M. Wojcik, G. Zuzel Download http://dx.doi.org/10.1016/j.astropartphys.2013.08.004 http://arxiv.org/abs/1204.6218 Abstract As part of the DarkSide program of direct dark... -
![[nggallery id=5] Wyniki obserwacji astronomicznych z ostatnich stu lat oraz obliczeń modelowych jednoznacznie wskazują, iż ponad 80% masy Wszechświata ma postać ciemnej materii. Tworzyć ją mogą neutralne cząstki, spoza Modelu...](http://zdfk.if.uj.edu.pl/wp-content/uploads/2013/04/Cryo-Plus1-115x115.jpg "Eksperyment DarkSide")
Eksperyment DarkSide
Posted on April 9, 2013 | No Comments[nggallery id=5] Wyniki obserwacji astronomicznych z ostatnich stu lat oraz obliczeń modelowych jednoznacznie wskazują, iż ponad 80% masy Wszechświata ma postać ciemnej materii. Tworzyć ją mogą neutralne cząstki, spoza Modelu...