0000000001020926

AUTHOR

L. Mosca

showing 5 related works from this author

High intensity neutrino oscillation facilities in Europe

2013

The EUROnu project has studied three possible options for future, high intensity neutrino oscillation facilities in Europe. The first is a Super Beam, in which the neutrinos come from the decay of pions created by bombarding targets with a 4 MW proton beam from the CERN High Power Superconducting Proton Linac. The far detector for this facility is the 500 kt MEMPHYS water Cherenkov, located in the Frejus tunnel. The second facility is the Neutrino Factory, in which the neutrinos come from the decay of mu(+) and mu(-) beams in a storage ring. The far detector in this case is a 100 kt magnetized iron neutrino detector at a baseline of 2000 km. The third option is a Beta Beam, in which the neu…

Nuclear and High Energy PhysicsPhysics and Astronomy (miscellaneous)Physics::Instrumentation and Detectors[PHYS.PHYS.PHYS-ACC-PH]Physics [physics]/Physics [physics]/Accelerator Physics [physics.acc-ph]7. Clean energy01 natural sciencesNuclear physicsneutrino0103 physical sciencesEmmaFysiklcsh:Nuclear and particle physics. Atomic energy. Radioactivityddc:530010306 general physicsNeutrino oscillationQCAstroparticle physicsPhysicsLarge Hadron ColliderBeta-Beam010308 nuclear & particles physicsFísicaSurfaces and InterfacesAccelerators and Storage RingsNeutrino detectorPhysical Scienceslcsh:QC770-798Physics::Accelerator PhysicsNeutrino FactoryHigh Energy Physics::ExperimentNeutrino[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Storage ringLepton
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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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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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Large underground, liquid based detectors for astro-particle physics in Europe: scientific case and prospects

2007

This document reports on a series of experimental and theoretical studies conducted to assess the astro-particle physics potential of three future large-scale particle detectors proposed in Europe as next generation underground observatories. The proposed apparatus employ three different and, to some extent, complementary detection techniques: GLACIER (liquid Argon TPC), LENA (liquid scintillator) and MEMPHYS (\WC), based on the use of large mass of liquids as active detection media. The results of these studies are presented along with a critical discussion of the performance attainable by the three proposed approaches coupled to existing or planned underground laboratories, in relation to…

PhysicsParticle physicsPhysics::Instrumentation and Detectors010308 nuclear & particles physicsDetectorActive detectionFOS: Physical sciencesAstronomy and AstrophysicsScintillator01 natural sciencesCritical discussionHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]0103 physical sciencesLiquid argonLiquid basedHigh Energy Physics::Experiment[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Neutrino010306 general physicsParticle Physics - PhenomenologyJournal of Cosmology and Astroparticle Physics
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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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