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Dark matter results from 225 live days of XENON100 data

Authors :
W. Hampel
M. Garbini
J.M.F. dos Santos
J. Lamblin
K. Bokeloh
Jean-Pierre Cussonneau
S. Rosendahl
Ethan Brown
M. Selvi
Sebastian Lindemann
Eilam Gross
Boris Bauermeister
P. Beltrame
Jochen Schreiner
Luke Goetzke
Hardy Simgen
A. D. Ferella
G. Sartorelli
A. Teymourian
F. Arneodo
Laura Baudis
H. Landsman
M. Le Calloch
J. A. M. Lopes
S. Fattori
Y. Meng
O. Vitells
A. Rizzo
David B. Cline
S. E. A. Orrigo
A. Kish
João Cardoso
K. Arisaka
R. Persiani
L. Scotto Lavina
C. Grignon
K. L. Giboni
H. Contreras
F. Gao
A. Behrens
E. Pantic
C. Balan
D. Thers
Ehud Duchovni
W. T. Chen
K. E. Lim
M. Weber
Auke-Pieter Colijn
R. F. Lang
Uwe Oberlack
Elena Aprile
Kaixuan Ni
E. Nativ
T. Marrodán Undagoitia
G. Plante
B. Choi
Ch. Weinheimer
A. J. Melgarejo Fernandez
P. R. Scovell
C. Ghag
F. V. Massoli
Qing Lin
M. Alfonsi
K. Lung
A. Molinario
W. Fulgione
Giacomo Bruno
C. Levy
N. Priel
Hui Wang
Florian Kaether
M. P. Decowski
Manfred Lindner
Marc Schumann
P. Shagin
Ran Budnik
Astroparticle Physics (IHEF, IoP, FNWI)
E. Aprile
M. Alfonsi
K. Arisaka
F. Arneodo
C. Balan
L. Baudi
B. Bauermeister
A. Behren
P. Beltrame
K. Bokeloh
E. Brown
G. Bruno
R. Budnik
J. M. R. Cardoso
W.-T. Chen
B. Choi
D. Cline
A. P. Colijn
H. Contrera
J. P. Cussonneau
M. P. Decowski
E. Duchovni
S. Fattori
A. D. Ferella
W. Fulgione
F. Gao
M. Garbini
C. Ghag
K.-L. Giboni
L. W. Goetzke
C. Grignon
E. Gro
W. Hampel
F. Kaether
A. Kish
J. Lamblin
H. Landsman
R. F. Lang
M. Le Calloch
C. Levy
K. E. Lim
Q. Lin
S. Lindemann
M. Lindner
J. A. M. Lope
K. Lung
T. Marrodán Undagoitia
F. V. Massoli
A. J. Melgarejo Fernandez
Y. Meng
A. Molinario
E. Nativ
K. Ni
U. Oberlack
S. E. A. Orrigo
E. Pantic
R. Persiani
G. Plante
N. Priel
A. Rizzo
S. Rosendahl
J. M. F. dos Santo
G. Sartorelli
J. Schreiner
M. Schumann
L. Scotto Lavina
P. R. Scovell
M. Selvi
P. Shagin
H. Simgen
A. Teymourian
D. Ther
O. Vitell
H. Wang
M. Weber
C. Weinheimer
Laboratoire SUBATECH Nantes (SUBATECH)
Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Nantes (UN)-Mines Nantes (Mines Nantes)
XENON100
Source :
Physical Review Letters, 109. American Physical Society, Physical Review Letters, Physical Review Letters, American Physical Society, 2012, 109, pp.181301. ⟨10.1103/PhysRevLett.109.181301⟩
Publication Year :
2012
Publisher :
American Physical Society, 2012.

Abstract

We report on a search for particle dark matter with the XENON100 experiment, operated at the Laboratori Nazionali del Gran Sasso (LNGS) for 13 months during 2011 and 2012. XENON100 features an ultra-low electromagnetic background of (5.3 \pm 0.6) \times 10^-3 events (kg day keVee)^-1 in the energy region of interest. A blind analysis of 224.6 live days \times 34 kg exposure has yielded no evidence for dark matter interactions. The two candidate events observed in the pre-defined nuclear recoil energy range of 6.6-30.5 keVnr are consistent with the background expectation of (1.0 \pm 0.2) events. A Profile Likelihood analysis using a 6.6-43.3 keVnr energy range sets the most stringent limit on the spin-independent elastic WIMP-nucleon scattering cross section for WIMP masses above 8 GeV/c^2, with a minimum of 2 \times 10^-45 cm^2 at 55 GeV/c^2 and 90% confidence level.<br />6 pages, 5 figures. Matches version accepted by PRL. Includes limits up to 10 TeV/c^2, published as supplementary material: http://prl.aps.org/supplemental/PRL/v109/i18/e181301 Please cite high mass limits as "Phys. Rev. Lett. 109, 181301 (2012), online supplementary material."

Details

Language :
English
ISSN :
10797114 and 00319007
Volume :
109
Database :
OpenAIRE
Journal :
Physical Review Letters
Accession number :
edsair.doi.dedup.....aa57720582feda10cc5e9c69a420b7d1
Full Text :
https://doi.org/10.1103/PhysRevLett.109.181301⟩