G. Nollez
Institut d'Astrophysique de Paris
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Featured researches published by G. Nollez.
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.
Astroparticle Physics | 1996
A. de Bellefon; I. Berkes; C. Bobin; D. Broszkiewicz; B. Chambon; M. Chapellier; G. Chardin; P. Charvin; V. Chazal; N. Coron; M. De Jésus; D. Drain; L. Dumoulin; Y. Giraud-Heraud; C. Goldbach; G. Guerier; J.P. Hadjout; J. Leblanc; D. Marchand; M. Massaq; Y. Messous; X.-F. Navick; G. Nollez; P. Pari; C. Pastor; M.C. Perillo-Isaac; I. Prostakov; D. Yvon
Abstract A dark matter detection experiment using a low temperature 24 g sapphire bolometer is presented. The low radioactive background cryogenic facility, installed in a deep underground site, is described, as well as the low-noise read-out electronics and the data analysis. From the energy spectrum, measured down to 4 keV, exclusion plots are derived for WIMPs having coherent vector coupling or axial coupling to ordinary matter.
Astroparticle Physics | 2007
S. Fiorucci; A. Benoit; L. Bergé; J. Blümer; A. Broniatowski; B. Censier; A. Chantelauze; M. Chapellier; G. Chardin; S. Collin; X. Defay; M. De Jésus; H. Deschamps; P. Di Stefano; Y. Dolgorouky; L. Dumoulin; K. Eitel; M. Fesquet; J. Gascon; G. Gerbier; C. Goldbach; M. Gros; M. Horn; A. Juillard; R. Lemrani; A. de Lesquen; A. Lubashevskiy; Marchese Luca; S. Marnieros; L. Mosca
Abstract This paper presents our interpretation and understanding of the different backgrounds in the EDELWEISS-I data sets. We analyze in detail the several populations observed, which include gammas, alphas, neutrons, thermal sensor events and surface events, and try to combine all data sets to provide a coherent picture of the nature and localization of the background sources. In light of this interpretation, we draw conclusions regarding the background suppression scheme for the EDELWEISS-II phase.
Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 2004
O. Martineau; A. Benoı̂t; L. Bergé; A. Broniatowski; L. Chabert; B. Chambon; M. Chapellier; G. Chardin; P. Charvin; M. De Jésus; P. Di Stefano; D. Drain; L. Dumoulin; J. Gascon; G. Gerbier; E. Gerlic; C. Goldbach; M. Goyot; M. Gros; J.P. Hadjout; S. Hervé; A. Juillard; A. de Lesquen; M. Loidl; J. Mallet; S. Marnieros; N. Mirabolfathi; L. Mosca; X.-F. Navick; G. Nollez
Several aspects of the analysis of the data obtained with the cryogenic heat-and-ionization Ge detectors used by the EDELWEISS dark matter search experiment are presented. Their calibration, the determination of their energy threshold, fiducial volume and nuclear recoil acceptance are detailed.
Physics Letters B | 2005
A. Benoit; L. Bergé; J. Blümer; A. Broniatowski; B. Censier; L. Chabert; M. Chapellier; G. Chardin; S. Collin; M. De Jésus; H. Deschamps; P. Di Stefano; Y. Dolgorouky; D. Drain; L. Dumoulin; K. Eitel; M. Fesquet; S. Fiorucci; J. Gascon; G. Gerbier; C. Goldbach; M. Gros; R. Gumbsheimer; M. Horn; A. Juillard; A. de Lesquen; M. Luca; J. Mallet; S. Marnieros; L. Mosca
The EDELWEISS collaboration is searching for WIMP dark matter using natural Ge cryogenic detectors. The whole data set of the first phase of the experiment contains a fiducial exposure of 4.8 kg.day on Ge-73, the naturally present (7.8%), high-spin Ge isotope. The sensitivity of the experiment to the spin-dependent WIMP-nucleon interactions is evaluated using the model-independent framework proposed by Tovey et al.
Physics Letters B | 2000
A. Benoit; L. Bergé; A. Broniatowski; B. Chambon; M. Chapellier; G. Chardin; P. Charvin; M. De Jésus; P. Di Stefano; D. Drain; L. Dumoulin; P. Garoche; J. Gascon; C. Goldbach; M. Gros; A. Juillard; A. de Lesquen; D. L'Hôte; J. Mallet; J. Mangin; S. Marnieros; N. Mirabolfathi; L. Miramonti; L. Mosca; X.-F. Navick; G. Nollez; P. Pari; S. Pécourt; E. Simon; M. Stern
Four categories of events have been identified in the EDELWEISS-I dark matter experiment using germanium cryogenic detectors measuring simultaneously charge and heat signals. These categories of events are interpreted as electron and nuclear interactions occurring in the volume of the detector, and electron and nuclear interactions occurring close to the surface of the detectors (within ≈10–20 μm of the surface). We discuss the hypothesis that low energy surface nuclear recoils, which seem to have been unnoticed by previous WIMP searches, may provide an interpretation of the anomalous events recorded by the UKDMC and Saclay NaI experiments. The present analysis points to the necessity of taking into account surface nuclear and electron recoil interactions for a reliable estimate of background rejection factors.
Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 1994
J.W. Zhou; P. de Marcillac; G. E. Artzner; N. Coron; C. Goldbach; J. Leblanc; G. Nollez; H.H. Stroke
Abstract Bolometers at low temperature are being developed as particle spectrometers and potential detectors of dark matter particles through the measurement of recoil energies. A successful observation of the recoil spectrum from a 210 Po electrodeposited source was made for the first time with the use of a 2 mm 3 composite-composite diamond bolometer operated in a 300 mK cryostat. The measured recoil ratio is 0.98±0.06 recoil/alpha above 50 keV, with the well defined peak in the spectrum at 101±2.5 keV.
Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 1992
N. Coursol; N. Coron; D. Massé; H.H. Stroke; J.W. Zhou; P. de Marcillac; J. Leblanc; G. E. Artzner; G. Dambier; J. Bouchard; G. Jegoudez; J.P. Lepeltier; G. Nollez; C. Golbach; J.-L. Picolo
Two major limitations met in the field of ionizing radiation metrology, i.e. energy resolution and detection energy threshold, may be improved by one or two orders of magnitude by using composite bolometers cooled below 300 mK and operating in the pulse mode. The major advantages are: possibility of choosing the absorber (from diamond to BGO: Al2O3, Ge, Si, BaF2, LiF, etc), the absence of statistical noise (phonon quanta are in the 10−4 eV range) and ultimate resolution in the 10−1 eV range for small bolometers. The theoretical and experimental limits are analyzed and solutions for extraneous noise limitations in a complete system are described. The most recent results in alpha-particle and gamma-ray spectrometry using a new design, the composite-composite bolometer, are given. In these, a resolution of 10.5 keV was obtained for 6 MeV alpha particles and < 2.5 keV for241Am 18 keV X rays using a 24 sapphire bolometer. The ideal bolometer concept is also discussed. In this, the simultaneous detection of quanta (due to ionization, fluorescence, ballistic phonons) and thermal energies will make it possible to have lower thresholds by amplification in the target. It should thus be possible to determine the characteristics of the particles (their precise arrival time and the positions of the impacts) and provide improvements in the field of integral counting for the absolute measurement of radioactivity.
Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 1996
A. de Bellefon; L. Bergé; I. Berkés; D. Broszkiewicz; B. Chambon; M. Chapellier; G. Chardin; P. Charvin; V. Chazal; N. Coron; M. De Jesus; D. Drain; L. Dumoulin; Y. Giraud-Heraud; G. Guerrier; C. Goldbach; J.P Hadjout; James Walter Leblanc; Y. Messous; X.-F. Navick; G. Nollez; C. Pastor; P. Pari; I. Prostakov; M.C. Perillo-Isaac; D. Yvon
Abstract The status of the EDELWEISS experiment (Experience pour DEtecter Les Wimps En SIte Souterrain) in the Frejus Underground Laboratory is reported. The cryostat is described with the main lines of low radioactivity design and readout system. The first results using bolometer detectors together with the measurement of the internal radioactive background using a 100 cm 3 classical Ge crystal are reported. The future program of the experiment will be outlined.
Nuclear Physics B - Proceedings Supplements | 1999
C. Bobin; N. Coron; G. Dambier; E. García; C. Goldbach; D. González; J. Leblanc; P. de Marcillac; A. Morales; J. Morales; G. Nollez; A. Ortiz de Solórzano; J. Puimedón; A. Salinas; M.L. Sarsa; S. Scopel; J.A. Villar
Abstract An experiment to look for light WIMPs with sapphire bolometers is to be installed in the Canfranc Underground Laboratory (at 2450 m.w.e) in the Spanish Pyrenees. In the first stage two small 25g bolometers with NTD-Ge sensors, operating at 25mK, with an energy threshold of 300eV and FWHM energy resolution of 120eV at 1.5keV will perform a background test experiment. The features of the bolometers, the radioactivity measurements of the components and the set-up and status of the experiment are reported.