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. 2017 Nov 3;119(18):181301.
doi: 10.1103/PhysRevLett.119.181301. Epub 2017 Oct 30.

First Dark Matter Search Results from the XENON1T Experiment

E Aprile  1 J Aalbers  2 F Agostini  3   4 M Alfonsi  5 F D Amaro  6 M Anthony  1 F Arneodo  7 P Barrow  8 L Baudis  8 B Bauermeister  9 M L Benabderrahmane  7 T Berger  10 P A Breur  2 A Brown  2 A Brown  8 E Brown  10 S Bruenner  11 G Bruno  3 R Budnik  12 L Bütikofer  13 J Calvén  9 J M R Cardoso  6 M Cervantes  14 D Cichon  11 D Coderre  13 A P Colijn  2 J Conrad  9 J P Cussonneau  15 M P Decowski  2 P de Perio  1 P Di Gangi  4 A Di Giovanni  7 S Diglio  15 G Eurin  11 J Fei  16 A D Ferella  9 A Fieguth  17 W Fulgione  3   18 A Gallo Rosso  3 M Galloway  8 F Gao  1 M Garbini  4 R Gardner  19 C Geis  5 L W Goetzke  1 L Grandi  19 Z Greene  1 C Grignon  5 C Hasterok  11 E Hogenbirk  2 J Howlett  1 R Itay  12 B Kaminsky  13 S Kazama  8 G Kessler  8 A Kish  8 H Landsman  12 R F Lang  14 D Lellouch  12 L Levinson  12 Q Lin  1 S Lindemann  11   13 M Lindner  11 F Lombardi  16 J A M Lopes  6 A Manfredini  12 I Mariş  7 T Marrodán Undagoitia  11 J Masbou  15 F V Massoli  4 D Masson  14 D Mayani  8 M Messina  1 K Micheneau  15 A Molinario  3 K Morå  9 M Murra  17 J Naganoma  20 K Ni  16 U Oberlack  5 P Pakarha  8 B Pelssers  9 R Persiani  15 F Piastra  8 J Pienaar  14 V Pizzella  11 M-C Piro  10 G Plante  1 N Priel  12 L Rauch  11 S Reichard  8   14 C Reuter  14 B Riedel  19 A Rizzo  1 S Rosendahl  17 N Rupp  11 R Saldanha  19 J M F Dos Santos  6 G Sartorelli  4 M Scheibelhut  5 S Schindler  5 J Schreiner  11 M Schumann  13 L Scotto Lavina  21 M Selvi  4 P Shagin  20 E Shockley  19 M Silva  6 H Simgen  11 M V Sivers  13 A Stein  22 S Thapa  19 D Thers  15 A Tiseni  2 G Trinchero  18 C Tunnell  19 M Vargas  17 N Upole  19 H Wang  22 Z Wang  3 Y Wei  8 C Weinheimer  17 J Wulf  8 J Ye  16 Y Zhang  1 T Zhu  1 XENON Collaboration
Affiliations

First Dark Matter Search Results from the XENON1T Experiment

E Aprile et al. Phys Rev Lett. .

Abstract

We report the first dark matter search results from XENON1T, a ∼2000-kg-target-mass dual-phase (liquid-gas) xenon time projection chamber in operation at the Laboratori Nazionali del Gran Sasso in Italy and the first ton-scale detector of this kind. The blinded search used 34.2 live days of data acquired between November 2016 and January 2017. Inside the (1042±12)-kg fiducial mass and in the [5,40] keV_{nr} energy range of interest for weakly interacting massive particle (WIMP) dark matter searches, the electronic recoil background was (1.93±0.25)×10^{-4} events/(kg×day×keV_{ee}), the lowest ever achieved in such a dark matter detector. A profile likelihood analysis shows that the data are consistent with the background-only hypothesis. We derive the most stringent exclusion limits on the spin-independent WIMP-nucleon interaction cross section for WIMP masses above 10 GeV/c^{2}, with a minimum of 7.7×10^{-47} cm^{2} for 35-GeV/c^{2} WIMPs at 90% C.L.

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