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Improved EDELWEISS-III sensitivity for low-mass WIMPs using a profile likelihood approach | | EDELWEISS Collaboration
; L. Hehn
; E. Armengaud
; Q. Arnaud
; C. Augier
; A. Benoît
; L. Bergé
; J. Billard
; J. Blümer
; T. de Boissière
; A. Broniatowski
; P. Camus
; A. Cazes
; M. Chapellier
; F. Charlieux
; M. De Jésus
; L. Dumoulin
; K. Eitel
; N. Foerster
; J. Gascon
; A. Giuliani
; M. Gros
; G. Heuermann
; Y. Jin
; A. Juillard
; C. Kéfélian
; M. Kleifges
; V. Kozlov
; H. Kraus
; V. A. Kudryavtsev
; H. Le-Sueur
; S. Marnieros
; X.-F. Navick
; C. Nones
; E. Olivieri
; P. Pari
; B. Paul
; M.-C. Piro
; D. Poda
; E. Queguiner
; S. Rozov
; V. Sanglard
; B. Schmidt
; S. Scorza
; B. Siebenborn
; D. Tcherniakhovski
; L. Vagneron
; M. Weber
; E. Yakushev
; | | Date: |
12 Jul 2016 | | Abstract: | We report on a dark matter search for a Weakly Interacting Massive Particle
(WIMP) in the mass range $m_chi in [4, 30],mathrm{GeV}/c^2$ with the
EDELWEISS-III experiment. A 2D profile likelihood analysis is performed on data
from eight selected detectors with the lowest energy thresholds leading to a
combined fiducial exposure of 496 kg-days. External backgrounds from $gamma$-
and $eta$-radiation, recoils from $^{206}$Pb and neutrons as well as detector
intrinsic backgrounds were modelled from data outside the region of interest
and constrained in the analysis. The basic data selection and most of the
background models are the same as those used in a previously published analysis
based on Boosted Decision Trees (BDT). For the likelihood approach applied in
the analysis presented here, a larger signal efficiency and a subtraction of
the expected background lead to a higher sensitivity, especially for the lowest
WIMP masses probed. No statistically significant signal was found and upper
limits on the spin-independent WIMP-nucleon scattering cross section can be set
with a hypothesis test based on the profile likelihood test statistics. The 90%
C.L. exclusion limit set for WIMPs with $m_chi = 4,mathrm{GeV/}c^2$ is $1.6
imes 10^{-39},mathrm{cm^2}$, which is an improvement of a factor of seven
with respect to the BDT-based analysis. For WIMP masses above
$15,mathrm{GeV/}c^2$ the exclusion limits found with both analyses are in
good agreement. | | Source: | arXiv, 1607.3367 | | Services: | Forum | Review | PDF | Favorites | |
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