M. De Jésus
University of Lyon
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Featured researches published by M. De Jésus.
Physics Letters B | 2011
E. Armengaud; C. Augier; A. Benoit; L. Bergé; J. Blümer; A. Broniatowski; V. Brudanin; B. Censier; G. Chardin; M. Chapellier; F. Charlieux; P. Coulter; G.A. Cox; X. Defay; M. De Jésus; Y. Dolgorouki; J. Domange; L. Dumoulin; K. Eitel; D. Filosofov; N. Fourches; J. Gascon; G. Gerbier; J. Gironnet; M. Gros; S. Henry; S. Hervé; A. Juillard; H. Kluck; V. Kozlov
Abstract The EDELWEISS-II Collaboration has completed a direct search for WIMP dark matter with an array of ten 400-g cryogenic germanium detectors in operation at the Laboratoire Souterrain de Modane. The combined use of thermal phonon sensors and charge collection electrodes with an interleaved geometry enables the efficient rejection of γ-induced radioactivity as well as near-surface interactions. A total effective exposure of 384 kg d has been achieved, mostly coming from fourteen months of continuous operation. Five nuclear recoil candidates are observed above 20 keV, while the estimated background is 3.0 events. The result is interpreted in terms of limits on the cross-section of spin-independent interactions of WIMPs and nucleons. A cross-section of 4.4 × 10 − 8 pb is excluded at 90%CL for a WIMP mass of 85 GeV. New constraints are also set on models where the WIMP-nucleon scattering is inelastic.
Astroparticle Physics | 1999
G. Gerbier; J. Mallet; L. Mosca; C. Tao; B. Chambon; V. Chazal; M. De Jésus; D. Drain; Y. Messous; C. Pastor
Abstract An extensive study of NaI(Tl) as a Dark Matter particle detector is presented. Emphasis is put on the response of the detector, both in energy and pulse shape, to all particles interacting in the detector, namely high energy (MeV) photons, low energy photons (X-rays), betas from external radioactivity, and neutrons, which induce nuclear recoils. The initial hope that the shorter decay times of nuclear recoils induced by WIMPs could be statistically separated from Compton interactions is weakened by the fact that low energy X-rays and betas exhibit pulse shapes similar to recoils. As a consequence, any indication of shorter decay time pulses leads to an ambiguous interpretation. Underground data for the WIMP search were obtained in a low activity environment at the Laboratoire Souterrain de Modane (LSM), with a 10 kg crystal having high photoelectron yield and 2 keV energy threshold. The data contain pulse shapes with decay times shorter than for Compton interactions and are not compatible with calibration reference shapes or a mixture of these. The effect is shown to come from a population with decay times even shorter than nuclear recoils but its origin was not identified. The Compton rejection efficiency is limited to factors ranging from 3 at 5 keV to 8 at 20 keV (electron equivalent energy). It is shown that the sensitivity of NaI(Tl) detectors to the cross section of Spin Independent coupling WIMPs is only slightly improved by the pulse shape analysis, while it is mostly determined by the differential energy rate at threshold. The sensitivity to the cross section of Spin Dependent coupling WIMPs is improved by about an order of magnitude by the pulse shape analysis.
Physics Letters B | 2001
A. Benoit; L. Bergé; A. Broniatowksi; B. Chambon; M. Chapellier; G. Chardin; P. Charvin; M. De Jésus; P. Di Stefano; D. Drain; L. Dumoulin; J. Gascon; G. Gerbier; C. Goldbach; M. Goyot; M. Gros; J.P. Hadjout; A. Juillard; A. de Lesquen; M. Loidl; J. Mallet; S. Marnieros; O. Martineau; N. Mirabolfathi; L. Mosca; L. Miramonti; X.-F. Navick; G. Nollez; P. Pari; M. Stern
The EDELWEISS collaboration has performed a direct search for WIMP dark matter using a 320 g heat-and-ionization cryogenic Ge detector operated in a low-background environment in the Laboratoire Souterrain de Modane. No nuclear recoils are observed in the fiducial volume in the 30-200 keV energy range during an effective exposure of 4.53 kg.days. Limits for the cross-section for the spin-independent interaction of WIMPs and nucleons are set in the framework of the Minimal Supersymmetric Standard Model (MSSM). The central value of the signal reported by the experiment DAMA is excluded at 90% CL.
Physics Letters B | 2009
A. Broniatowski; X. Defay; E. Armengaud; L. Bergé; A. Benoit; O. Besida; J. Blümer; A. Chantelauze; M. Chapellier; G. Chardin; F. Charlieux; S. Collin; O. Crauste; M. De Jésus; P. Di Stefano; Y. Dolgorouki; J. Domange; L. Dumoulin; K. Eitel; J. Gascon; G. Gerbier; M. Gros; M. Hannawald; S. Hervé; A. Juillard; H. Kluck; V. Kozlov; R. Lemrani; A. Lubashevskiy; C. Marrache
A new design of a cryogenic germanium detector for dark matter search is presented, taking advantage of the coplanar grid technique of event localisation for improved background discrimination. Experiments performed with prototype devices in the EDELWEISS II setup at the Modane underground facility demonstrate the remarkably high efficiency of these devices for the rejection of low-energy
Astroparticle Physics | 1998
V. Chazal; R. Brissot; J.F. Cavaignac; B. Chambon; M. De Jésus; D. Drain; Y. Giraud-Heraud; C. Pastor; A. Stutz; L. Vagneron
\beta
Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 2006
R. Lemrani; M. Robinson; V.A. Kudryavtsev; M. De Jésus; G. Gerbier; N.J.C. Spooner
, approaching 10
Physics Letters B | 2010
E. Armengaud; C. Augier; A. Benoit; L. Bergé; O. Besida; J. Blümer; A. Broniatowski; A. Chantelauze; M. Chapellier; G. Chardin; F. Charlieux; S. Collin; X. Defay; M. De Jésus; P. Di Stefano; Y. Dolgorouki; J. Domange; L. Dumoulin; K. Eitel; J. Gascon; G. Gerbier; M. Gros; M. Hannawald; S. Hervé; A. Juillard; H. Kluck; V. Kozlov; R. Lemrani; P. Loaiza; A. Lubashevskiy
^5
Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 2003
E. Simon; L. Bergé; A. Broniatowski; R. Bouvier; B. Chambon; M. De Jésus; D. Drain; L. Dumoulin; J. Gascon; J.P. Hadjout; A. Juillard; O. Martineau; C. Pastor; M. Stern; L. Vagneron
. This opens the road to investigate the range beyond 10
Journal of Cosmology and Astroparticle Physics | 2013
E. Armengaud; Q. Arnaud; C. Augier; A. Benoit; L. Bergé; T. Bergmann; J. Blümer; A. Broniatowski; V. Brudanin; P. Camus; A. Cazes; B. Censier; M. Chapellier; F. Charlieux; F. Couëdo; P. Coulter; G.A. Cox; T. de Boissière; M. De Jésus; Y. Dolgorouky; A.A. Drillien; L. Dumoulin; K. Eitel; D. Filosofov; N. Fourches; J. Gascon; G. Gerbier; M. Gros; L. Hehn; S. Henry
^{-8}
Astroparticle Physics | 1999
S. Pécourt; B. Chambon; M. De Jésus; D. Drain; G. Gerbier; J. Mallet; M. Massaq; L. Mosca; C. Pastor; C. Tao; L. Vagneron
pb in the WIMP-nucleon collision cross-sections, as proposed in the EURECA project of a one-ton cryogenic detector mass.