0000000001020918

AUTHOR

M. Gros

showing 7 related works from this author

Precise measurement of 2νββ decay of 100Mo with the CUPID-Mo detection technology

2020

We report the measurement of the two-neutrino double-beta (2 νββ) decay of 100Mo to the ground state of 100Ru using lithium molybdate (Li2100MoO4) scintillating bolometers. The detectors were developed for the CUPID-Mo program and operated at the EDELWEISS-III low background facility in the Modane underground laboratory (France). From a total exposure of 42.235 kg× day, the half-life of 100Mo is determined to be T1/22ν=[7.12-0.14+0.18(stat.)±0.10(syst.)]×1018 years. This is the most accurate determination of the 2 νββ half-life of 100Mo to date.

Quantum PhysicsParticle and Plasma PhysicsMolecularNuclearnucl-exphysics.ins-detAtomicNuclear & Particles Physics
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Precise measurement of $$2\nu \beta \beta $$ 2νββ decay of $$^{100}$$ 100 Mo with the CUPID-Mo detection technology

2020

We report the measurement of the two-neutrino double-beta ($$2\nu \beta \beta $$ 2νββ ) decay of $$^{100}$$ 100 Mo to the ground state of $$^{100}$$ 100 Ru using lithium molybdate ($$\hbox {Li}_2^{\;\;100}\hbox {MoO}_4$$ Li2100MoO4 ) scintillating bolometers. The detectors were developed for the CUPID-Mo program and operated at the EDELWEISS-III low background facility in the Modane underground laboratory (France). From a total exposure of 42.235 kg$$\times $$ × day, the half-life of $$^{100}$$ 100 Mo is determined to be $$T_{1/2}^{2\nu }=[7.12^{+0.18}_{-0.14}\,\mathrm {(stat.)}\pm 0.10\,\mathrm {(syst.)}]\times 10^{18}$$ T1/22ν=[7.12-0.14+0.18(stat.)±0.10(syst.)]×1018 years. This is the mo…

European Physical Journal
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Interpretation of the Anomalous NaI Events

2001

Anomalous events, with scintillation decay times shorter than nuclear recoils, have been observed by the UKDMC and Saclay NaI experiments. By using the event categories observed in the EDELWEISS experiment, we propose to interpret the anomalous NaI events as surface nuclear recoils accompanied with a small energy loss of an escaping alpha particle. The discrimination performances of the NaI experiments which have not taken into account these events in their analysis, notably for axial WIMP interactions, must then be reevaluated.

Nuclear physicsPhysicsScintillationEnergy lossWIMPPhysics::Instrumentation and DetectorsAstrophysics::Instrumentation and Methods for AstrophysicsAlpha particleEDELWEISSEvent (particle physics)Interpretation (model theory)
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INTEGRAL/SPI ground calibration

2003

Three calibration campaigns of the spectrometer SPI have been performed before launch in order to determine the instrument characteristics, such as the effective detection area, the spectral resolution and the angular resolution. Absolute determination of the effective area has been obtained from simulations and measurements. At 1 MeV, the effective area is 65 cm^2 for a point source on the optical axis, the spectral resolution ~2.3 keV. The angular resolution is better than 2.5 deg and the source separation capability about 1 deg. Some temperature dependant parameters will require permanent in-flight calibration.

Point source[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]FOS: Physical sciencesInstrumentation ; Detectors ; Spectrographs ; Space vehicles ; Gamma rays ; ObservationsAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAAstrophysics01 natural sciences[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]OpticsSpectrographs0103 physical sciencesCalibrationSource separationAngular resolutionSpectral resolutionspace vehicles: instrumentsInstrumentation010303 astronomy & astrophysicsObservations:ASTRONOMÍA Y ASTROFÍSICA::Astronomía óptica [UNESCO]instrumentation: spectrographsPhysicsSpectrometer[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsbusiness.industryinstrumentation: detectorsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Astronomía ópticaGamma raysAntenna apertureAstrophysics (astro-ph)DetectorsSpace vehiclesAstronomy and AstrophysicsOptical axisSpace and Planetary Sciencebusiness:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]gamma rays: observations
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Precise measurement of $2\nu\beta\beta$ decay of $^{100}$Mo with the CUPID-Mo detection technology

2020

We report the measurement of the two-neutrino double-beta ($2\nu\beta\beta$) decay of $^{100}$Mo to the ground state of $^{100}$Ru using lithium molybdate (\crystal) scintillating bolometers. The detectors were developed for the CUPID-Mo program and operated at the EDELWEISS-III low background facility in the Modane underground laboratory. From a total exposure of $42.235$ kg$\times$d, the half-life of $^{100}$Mo is determined to be $T_{1/2}^{2\nu}=[7.12^{+0.18}_{-0.14}\,\mathrm{(stat.)}\pm0.10\,\mathrm{(syst.)}]\times10^{18}$ years. This is the most accurate determination of the $2\nu\beta\beta$ half-life of $^{100}$Mo to date. We also confirm, with the statistical significance of $>3\sigm…

Lithium molybdatePhysics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)Analytical chemistry[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]nucl-ex01 natural sciencesAtomicchemistry.chemical_compoundParticle and Plasma Physicstwo-neutrino double-beta decay scintillating bolometers0103 physical sciencesddc:530Beta (velocity)Nuclear[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsNuclear ExperimentEngineering (miscellaneous)physics.ins-detS076H2NPhysicsQuantum Physics010308 nuclear & particles physicsPhysicsMolecularBeta decayNuclear & Particles Physics3. Good healthchemistrydouble beta decays bolometersUnderground laboratoryGround state
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Status of the EDELWEISS experiment

1999

The Edelweiss Dark Matter Experiment is installed in the Modane Underground Laboratory since 1994. In 1997 the first detector of a 70 g heat and ionization Ge low-temperature detector built by the collaboration showed its discrimination capabilities. During the last two years the installation was upgraded, and a new generation of 70 g Ge detectors is operational. The detector environment is drastically controlled to avoid radioactive contamination. A test run with two new 70 g detectors shows a reduction by a factor of ten in the background level before 7-ray rejection which is now around 2 events/kg/keV/day. Three 320 g Ge cryogenic detectors have been constructed and are now being tested …

CryostatPhysicsNuclear and High Energy Physics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]Dark matterBolometerDetectorCosmic rayEDELWEISSAtomic and Molecular Physics and OpticsParticle detectorlaw.invention[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Nuclear physicsWIMPlaw[SDU]Sciences of the Universe [physics]Measuring instrumentInstrumentationEvent (probability theory)
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Background discrimination capabilities of a heat and ionization germanium cryogenic detector

2001

The discrimination capabilities of a 70 g heat and ionization Ge bolometer are studied. This first prototype has been used by the EDELWEISS Dark Matter experiment, installed in the Laboratoire Souterrain de Modane, for direct detection of WIMPs. Gamma and neutron calibrations demonstrate that this type of detector is able to reject more than 99.6% of the background while retaining 95% of the signal, provided that the background events distribution is not biased towards the surface of the Ge crystal. However, the 1.17 kg.day of data taken in a relatively important radioactive environment show an extra population slightly overlapping the signal. This background is likely due to interactions o…

Dark matterPopulationFOS: Physical sciencesAstrophysicsEDELWEISSAstrophysics01 natural scienceslaw.inventionNuclear physics[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]RecoillawIonization0103 physical sciencesNeutron010306 general physicseducationPhysicseducation.field_of_study[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsBolometerDetectorAstrophysics (astro-ph)Astronomy and AstrophysicsDark matter ; WIMP ; cryogenic detector
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