0000000000124077

AUTHOR

J.-y. Roussé

showing 5 related works from this author

Accumulation of positrons from a LINAC based source

2020

International audience; The GBAR experiment aims to measure the gravitational acceleration of antihydrogen H̅. It will use H̅+ ions formed by the interaction of antiprotons with a dense positronium cloud, which will require about 1010 positrons to produce one H̅+. We present the first results on the positron accumulation, reaching 3.8±0.4×108 e+ collected in 560 s.

010302 applied physicsPhysicsMeasure (physics)General Physics and Astronomy02 engineering and technology021001 nanoscience & nanotechnologyGravitational acceleration01 natural sciencesLinear particle acceleratorPositroniumNuclear physicsPositronPositron plasma; Positron accumulation; Antimatter; Penning-Malmberg trap; Greaves-Surko trap; GBAR[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]AntiprotonAntimatter0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Physics::Accelerator PhysicsPhysics::Atomic Physics0210 nano-technologyAntihydrogenComputingMilieux_MISCELLANEOUSActa Physica Polonica A
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A pulsed high-voltage decelerator system to deliver low-energy antiprotons

2021

International audience; The GBAR (Gravitational Behavior of Antihydrogen at Rest) experiment at CERN requires efficient deceleration of 100 keV antiprotons provided by the new ELENA synchrotron ring to synthesize antihydrogen. This is accomplished using electrostatic deceleration optics and a drift tube that is designed to switch from -99 kV to ground when the antiproton bunch is inside – essentially a charged particle “elevator” – producing a 1 keV pulse. We describe the simulation, design, construction and successful testing of the decelerator device at -92 kV on-line with antiprotons from ELENA.

Nuclear and High Energy PhysicsDrift tubeGeneral RelativityIon-optic simulationsCERN Labdrift tubeAstrophysics::High Energy Astrophysical Phenomena[PHYS.PHYS.PHYS-ACC-PH]Physics [physics]/Physics [physics]/Accelerator Physics [physics.acc-ph]Charged-particle opticsfabrication7. Clean energy01 natural sciencesanti-p: decelerationlaw.inventionNuclear physicslaw0103 physical sciencessynchrotronPhysics::Atomic Physics010306 general physicsAntihydrogennumerical calculationsInstrumentationaccelerator: designPhysicsantihydrogenLarge Hadron Collider010308 nuclear & particles physicsHigh voltageCharged particleSynchrotron[PHYS.PHYS.PHYS-GEN-PH]Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]Pulse (physics)beam opticsAntiprotonPhysics::Accelerator Physics
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Positron production using a 9 MeV electron linac for the GBAR experiment

2020

For the GBAR (Gravitational Behaviour of Antihydrogen at Rest) experiment at CERN's Antiproton Decelerator (AD) facility we have constructed a source of slow positrons, which uses a low-energy electron linear accelerator (linac). The driver linac produces electrons of 9 MeV kinetic energy that create positrons from bremsstrahlung-induced pair production. Staying below 10 MeV ensures no persistent radioactive activation in the target zone and that the radiation level outside the biological shield is safe for public access. An annealed tungsten-mesh assembly placed directly behind the target acts as a positron moderator. The system produces $5\times10^7$ slow positrons per second, a performan…

safetyAntimatterNuclear and High Energy PhysicsCERN LabPhysics - Instrumentation and DetectorstungstenPositronAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesElectron01 natural sciences7. Clean energyLinear particle acceleratorpositron: particle source010305 fluids & plasmaselectron: pair productionNuclear physicselectron: linear acceleratorPositronPositron; Linear accelerator; Antimatter; Antihydrogen; Gravitation0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Detectors and Experimental TechniquesNuclear Experiment010306 general physicsAntihydrogenphysics.ins-detInstrumentationenergy: lowantihydrogenPhysicsLarge Hadron Collidergravitation 2Instrumentation and Detectors (physics.ins-det)linear acceleratorAntiproton DeceleratorPair productionradioactivityAntimattergravitation: accelerationPhysics::Accelerator PhysicsHigh Energy Physics::Experimentperformancepositron: yieldGravitationNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Development of a PbWO 4 detector for single-shot positron annihilation lifetime spectroscopy at the GBAR experiment

2020

International audience; We have developed a PbWO 4 (PWO) detector with a large dynamic range to measure the intensity of a positron beam and the absolute density of the ortho-positronium (o-Ps) cloud it creates. A simulation study shows that a setup based on such detectors may be used to determine the angular distribution of the emission and reflection of o-Ps to reduce part of the uncertainties of the measurement. These will allow to improve the precision in the measurement of the cross section for the (anti) hydrogen formation by (anti) proton-positronium charge exchange and to optimize the yield of antihydrogen ion which is an essential parameter in the GBAR experiment.

PhysicsPhysics::Instrumentation and Detectors[PHYS.PHYS.PHYS-ACC-PH]Physics [physics]/Physics [physics]/Accelerator Physics [physics.acc-ph]DetectorMeasure (physics)General Physics and Astronomy7. Clean energyIonNuclear physicsCross section (physics)[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]PACS: 78.70.Bj 41.75.Fr 36.10.DrYield (chemistry)Reflection (physics)[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]AntihydrogenSpectroscopyComputingMilieux_MISCELLANEOUS
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$^{78}$Ni revealed as a doubly magic stronghold against nuclear deformation

2019

Nuclear magic numbers, which emerge from the strong nuclear force based on quantum chromodynamics, correspond to fully occupied energy shells of protons, or neutrons inside atomic nuclei. Doubly magic nuclei, with magic numbers for both protons and neutrons, are spherical and extremely rare across the nuclear landscape. While the sequence of magic numbers is well established for stable nuclei, evidence reveals modifications for nuclei with a large proton-to-neutron asymmetry. Here, we provide the first spectroscopic study of the doubly magic nucleus $^{78}$Ni, fourteen neutrons beyond the last stable nickel isotope. We provide direct evidence for its doubly magic nature, which is also predi…

1000ProtonNuclear Theorymedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaStrong interactionNuclear TheoryFOS: Physical sciences01 natural sciencesAsymmetryNuclear Theory (nucl-th)Magic number (programming)0103 physical sciencesEffective field theoryPhysics::Atomic and Molecular ClustersNeutronNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentNuclear Experimentmedia_commonPhysics[PHYS]Physics [physics]Multidisciplinary010308 nuclear & particles physicsMagic (programming)Atomic nucleusAtomic physics
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