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Results from the Super Cryogenic Dark Matter Search (SuperCDMS) experiment at Soudan

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arxiv 1708.08869 v1 pith:KHANK6CW submitted 2017-08-29 hep-ex hep-ph

SuperCDMS Collaboration: R. Agnese , T. Aramaki , I.J. Arnquist , W. Baker , D. Balakishiyeva , S. Banik , D. Barker , R. Basu Thakur
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D.A. Bauer T. Binder M.A. Bowles P.L. Brink R. Bunker B. Cabrera D.O. Caldwell R. Calkins C. Cartaro D.G. Cerdeño Y. Chang Y. Chen J. Cooley B. Cornell P. Cushman M. Daal P.C.F. Di Stefano T. Doughty E. Fascione E. Figueroa-Feliciano M. Fritts G. Gerbier R. Germond M. Ghaith G.L. Godfrey S.R. Golwala J. Hall H.R. Harris Z. Hong E.W. Hoppe L. Hsu M.E. Huber V. Iyer D. Jardin A. Jastram C. Jena M.H. Kelsey A. Kennedy A. Kubik N.A. Kurinsky B. Loer E. Lopez Asamar P. Lukens D. MacDonell R. Mahapatra V. Mandic N. Mast E.H. Miller N. Mirabolfathi B. Mohanty J.D. Morales Mendoza J. Nelson J.L. Orrell S.M. Oser K. Page W.A. Page R. Partridge M. Penalver Martinez M. Pepin A. Phipps S. Poudel M. Pyle H. Qiu W. Rau P. Redl A. Reisetter T. Reynolds A. Roberts A.E. Robinson H.E. Rogers T. Saab B. Sadoulet J. Sander K. Schneck R.W. Schnee S. Scorza K. Senapati B. Serfass D. Speller M. Stein J. Street H.A. Tanaka D. Toback R. Underwood A.N. Villano B. von Krosigk B. Welliver J.S. Wilson M.J. Wilson D.H. Wright S. Yellin J.J. Yen B.A. Young X. Zhang X. Zhao
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classification hep-exhep-ph
keywords resultssearchsoudansupercdmstimesanalysisbackgroundsblinded
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

We report the result of a blinded search for Weakly Interacting Massive Particles (WIMPs) using the majority of the SuperCDMS Soudan dataset. With an exposure of 1690 kg days, a single candidate event is observed, consistent with expected backgrounds. This analysis (combined with previous Ge results) sets an upper limit on the spin-independent WIMP--nucleon cross section of $1.4 \times 10^{-44}$ ($1.0 \times 10^{-44}$) cm$^2$ at 46 GeV/$c^2$. These results set the strongest limits for WIMP--germanium-nucleus interactions for masses $>$12 GeV/$c^2$.

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