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Author
E. Aprile
J. Aalbers
F. Agostini
M. Alfonsi
L. Althueser
F.D. Amaro
M. Anthony
F. Arneodo
L. Baudis
B. Bauermeister
M.L. Benabderrahmane
T. Berger
P.A. Breur
A. Brown
A. Brown
E. Brown
S. Bruenner
G. Bruno
R. Budnik
C. Capelli
J.M.R. Cardoso
D. Cichon
D. Coderre
A.P. Colijn
J. Conrad
J.P. Cussonneau
M.P. Decowski
P. de Perio
P. Di Gangi
A. Di Giovanni
S. Diglio
A. Elykov
G. Eurin
J. Fei
A.D. Ferella
A. Fieguth
W. Fulgione
A. Gallo Rosso
M. Galloway
F. Gao
M. Garbini
C. Geis
L. Grandi
Z. Greene
H. Qiu
C. Hasterok
E. Hogenbirk
J. Howlett
R. Itay
F. Joerg
XENON Collaboration
Date
14-9-2018
Title
Dark Matter Search Results from a One Ton-Year Exposure of XENON1T
Journal
Physical Review Letters
Volume | Issue number
121 | 11
Article number
111302
Number of pages
8
Document type
Article
Faculty
Faculty of Science (FNWI)
Institute
Institute for High Energy Physics (IHEF)
Informatics Institute (IVI)
Abstract

We report on a search for weakly interacting massive particles (WIMPs) using 278.8 days of data collected with the XENON1T experiment at LNGS. XENON1T utilizes a liquid xenon time projection chamber with a fiducial mass of (1.30±0.01) ton, resulting in a 1.0 ton yr exposure. The energy region of interest, [1.4,10.6] keVee ([4.9,40.9] keVnr), exhibits an ultralow electron recoil background rate of [82-3+5(syst)±3(stat)] events/(ton yr keVee). No significant excess over background is found, and a profile likelihood analysis parametrized in spatial and energy dimensions excludes new parameter space for the WIMP-nucleon spin-independent elastic scatter cross section for WIMP masses above 6 GeV/c2, with a minimum of 4.1×10-47 cm2 at 30 GeV/c2 and a 90% confidence level.

URL
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Other links
Link to publication in Scopus
Language
English
Note
© 2018 American Physical Society
Persistent Identifier
https://hdl.handle.net/11245.1/4e39d67c-7ddb-4254-aa30-ab2430abc279
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    Dark Matter Search Results from a One Ton-Year Exposure of XENON1T(Final published version)

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