0000000000392932

AUTHOR

W. Oelert

showing 23 related works from this author

ATRAP antihydrogen experiments

2007

Antihydrogen (Hbar) was first produced at CERN in 1996. Over the past decade our ATRAP collaboration has made massive progress toward our goal of producing large numbers of cold Hbar atoms that will be captured in a magnetic gradient trap for precise comparison between the atomic spectra of matter and antimatter. The AD at CERN provides bunches of 3 × 107 low energy Pbars every 100 seconds. We capture and cool to 4 K, 0.1% of these in a cryogenic Penning trap. By stacking many bunches we are able to do experiments with 3 × 105 Pbars. ∼100 e+/sec from a 22Na radioactive source are captured and cooled in the trap, with 5 × 106 available experiments.We have developed 2 ways to make Hbar from t…

PhysicsAntiparticleCondensed Matter PhysicsPenning trapNuclear physicssymbols.namesakeAntiprotonLaser coolingAntimatterRydberg formulasymbolsPhysics::Atomic PhysicsAtomic physicsNeutral particleAntihydrogenphysica status solidi c
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Drift chamber calibration and particle identification in the P-349 experiment

2019

The goal of the P-349 experiment is to test whether 3.5 GeV/c antiprotons produced in high-energy proton-proton collisions are polarized in view of the preparation of a polarized antiproton beam. In this article, we present the details of the ongoing analysis focused on the drift chambers calibration and particle identification with DIRC.

Physics010308 nuclear & particles physicsPhysicsQC1-99901 natural sciencesParticle identificationNuclear physicsSubatomär fysikAntiproton beamAntiproton0103 physical sciencesSubatomic PhysicsCalibrationPhysics::Accelerator PhysicsHigh Energy Physics::Experimentddc:530Detectors and Experimental Techniques010306 general physicsNuclear Experiment
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A semiconductor laser system for the production of antihydrogen

2012

Laser-controlled charge exchange is a promising method for producing cold antihydrogen. Caesium atoms in Rydberg states collide with positrons and create positronium. These positronium atoms then interact with antiprotons, forming antihydrogen. Las er excitation of the caesium atoms is essential to increase the cross section of the charge-exchange collisions. This method was demonstrated in 2004 by the ATRAP collaboration by using an available copper vapour laser. For a second generation of charge-e xchange experiments we have designed a new semiconductor laser system that features several improvements compared to the copper vapour laser. We describe this new laser system and show the resul…

PhysicsGeneral Physics and Astronomychemistry.chemical_elementLaserlaw.inventionSemiconductor laser theoryPositroniumsymbols.namesakechemistrylawAntimatterExcited stateCaesiumPhysics::Atomic and Molecular ClustersRydberg formulasymbolsddc:530Physics::Atomic PhysicsAtomic physicsAntihydrogenNew Journal of Physics
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Pumped helium system for cooling positron and electron traps to 1.2 K

2011

Abstract Extremely precise tests of fundamental particle symmetries should be possible via laser spectroscopy of trapped antihydrogen ( H ¯ ) atoms. H ¯ atoms that can be trapped must have an energy in temperature units that is below 0.5 K—the energy depth of the deepest magnetic traps that can currently be constructed with high currents and superconducting technology. The number of atoms in a Boltzmann distribution with energies lower than this trap depth depends sharply upon the temperature of the thermal distribution. For example, ten times more atoms with energies low enough to be trapped are in a thermal distribution at a temperature of 1.2 K than for a temperature of 4.2 K. To date, H…

Condensed Matter::Quantum GasesSuperconductivityPhysicsantihydrogenNuclear and High Energy Physicsliquid heliumLiquid heliumPenning trapchemistry.chemical_elementElectronAtmospheric temperature rangePenning traplaw.inventionchemistrylawAntimatterantiprotonrefrigeratorPhysics::Atomic PhysicsAtomic physicsAntihydrogenInstrumentationHelium
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Adiabatic Cooling of Antiprotons

2011

Adiabatic cooling is shown to be a simple and effective method to cool many charged particles in a trap to very low temperatures. Up to 3 x 10(6) (p) over bar are cooled to 3.5 K-10(3) times more cold (p) over bar and a 3 times lower (p) over bar temperature than previously reported. A second cooling method cools (p) over bar plasmas via the synchrotron radiation of embedded (p) over bar (with many fewer (p) over bar than (p) over bar) in preparation for adiabatic cooling. No (p) over bar are lost during either process-a significant advantage for rare particles.

PhysicsHigh Energy Physics::PhenomenologyBremsstrahlungGeneral Physics and AstronomySynchrotron radiationElectronAtmospheric temperature rangeCharged particlelaw.inventionJlawAntiprotonddc:550High Energy Physics::ExperimentPhysics::Atomic PhysicsAtomic physicsAdiabatic processElectron cooling
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Polarization analysis of $\bar{p}$ produced in pA collisions

2019

A quite simple procedure for the generation of a polarized antiproton beam could be worked out if antiprotons are produced with some polarization. In order to investigate this possibility measurements of the polarization of produced antiprotons have been started at a CERN/PS test beam. The polarization will be determined from the asymmetry of the elastic antiproton scattering at a liquid hydrogen target in the CNI region for which the analyzing power is well known. The data are under analysis and an additional measurement is done in 2018. Details on the experiment and the ongoing data analysis will be given.

PhysicsAntiparticle010308 nuclear & particles physicsPhysicsQC1-999Polarization (waves)01 natural sciences7. Clean energyNuclear physicsAntiproton beamAntiproton0103 physical sciencesPhysics::Accelerator Physicsddc:530High Energy Physics::ExperimentPhysics::Atomic Physics010306 general physicsAntihydrogenNuclear Experiment
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Search for polarization effects in the antiproton production process

2015

For the production of a polarized antiproton beam various methods have been suggested including the possibility that antiprotons may be produced polarized which will be checked experimentally. The polarization of antiprotons produced under typical conditions for antiproton beam preparation will be measured at the CERN/PS. If the production process creates some polarization a polarized antiproton beam could be prepared by a rather simple modification of the antiproton beam facility. The detection setup and the expected experimental conditions are described. For the production of a polarized antiproton beam various methods have been suggested including the possibility that antiprotons may be …

PhysicsLarge Hadron ColliderPhysics - Instrumentation and DetectorsFOS: Physical sciencesGeneral Physics and AstronomyParticle acceleratorInstrumentation and Detectors (physics.ins-det)Polarization (waves)law.inventionHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Antiproton beamAntiprotonlawPhysics::Accelerator Physicsddc:530High Energy Physics::ExperimentPhysics::Atomic PhysicsNuclear Experiment (nucl-ex)Detectors and Experimental TechniquesNuclear ExperimentNuclear Experiment
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CERN ELENA project progress report

2015

The Extra Low Energy Antiproton ring (ELENA) is a CERN project aiming at constructing a 30 m circumference synchrotron to further decelerate antiprotons from the Antiproton Decelerator (AD) from 5.3 MeV to 100 keV. The additional deceleration complemented by an electron cooler to reduce emittances will allow the existing AD experiments to increase substantially their antiproton capture efficiencies and render new experiments possible. The ELENA design is now well advanced and the project has entered the construction stage, in particular for what concerns the infrastructure. Installation of the machine components is foreseen during the second half of 2015 and beginning of 2016 followed by ri…

Antiproton DeceleratorLow energyLarge Hadron Colliderbusiness.industryAntiprotonComputer sciencePhysicsQC1-999Physics::Accelerator PhysicsAerospace engineeringbusinessEngineering physicsParticle Physics - ExperimentEPJ Web of Conferences
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Single-component plasma of photoelectrons

2007

Abstract Ten-nanosecond pulses of photoelectrons liberated by intense UV laser pulses from a thin gold layer are captured into a single-component plasma that is ideally suited to cool antiprotons ( p ¯ ) for antihydrogen ( H ¯ ) production. Up to a billion electrons are accumulated using a series of laser pulses, more than are needed for efficient p ¯ cooling in the large traps now being used for loading p ¯ for H ¯ production. The method is demonstrated within an enclosed vacuum space that is entirely at 4 K, and is thus compatible with the exceptional cryogenic vacuum that is desirable for the long-term storage of antihydrogen. The pitfalls of other electron accumulation methods are entir…

PhysicsNuclear and High Energy PhysicsThermionic emissionPlasmaElectronPhotoelectric effectLaserlaw.inventionField electron emissionlawAntimatterPhysics::Atomic PhysicsAtomic physicsAntihydrogenPhysics Letters B
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Antihydrogen production within a Penning-Ioffe trap.

2008

Slow antihydrogen (H) is produced within a Penning trap that is located within a quadrupole Ioffe trap, the latter intended to ultimately confine extremely cold, ground-state H[over ] atoms. Observed H[over ] atoms in this configuration resolve a debate about whether positrons and antiprotons can be brought together to form atoms within the divergent magnetic fields of a quadrupole Ioffe trap. The number of detected H atoms actually increases when a 400 mK Ioffe trap is turned on.

Condensed Matter::Quantum GasesPhysicsAntiparticleGeneral Physics and AstronomyPenning trapTrap (computing)Nuclear physicsAntiprotonAntimatterQuadrupolePhysics::Atomic and Molecular ClustersPhysics::Atomic PhysicsIon trapAtomic physicsAntihydrogenPhysical review letters
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Determination of theη′-Proton Scattering Length in Free Space

2014

Taking advantage of both the high mass resolution of the COSY-11 detector and the high energy resolution of the low-emittance proton beam of the cooler synchrotron COSY, we determine the excitation function for the $pp\ensuremath{\rightarrow}pp{\ensuremath{\eta}}^{\ensuremath{'}}$ reaction close to threshold. Combining these data with previous results, we extract the scattering length for the ${\ensuremath{\eta}}^{\ensuremath{'}}$-proton potential in free space to be $\mathrm{Re}({a}_{p{\ensuremath{\eta}}^{\ensuremath{'}}})=0\ifmmode\pm\else\textpm\fi{}0.43\text{ }\text{ }\mathrm{fm}$ and $\mathrm{Im}({a}_{p{\ensuremath{\eta}}^{\ensuremath{'}}})={0.37}_{\ensuremath{-}0.16}^{+0.40}\text{ }\t…

Excitation functionPhysicsParticle physicsMeson productionProton010308 nuclear & particles physicsGeneral Physics and AstronomyScattering lengthFree space01 natural sciencesProton scattering0103 physical sciencesHigh massHigh Energy Physics::ExperimentAtomic physicsNuclear Experiment010306 general physicsHigh energy resolutionPhysical Review Letters
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Status of the analysis for the search of polarization in the antiproton production process

2016

The P-349 experiment aims to test whether for antiprotons the production process itself can be a source of polarization in view of the preparation of a polarized antiproton beam. In this article we present the details of performed measurements and report on the status of the ongoing analysis.

PhysicsAntiparticle010308 nuclear & particles physicsPhysicsQC1-999Polarization (waves)01 natural sciencesEngineering physicsNuclear physicsSubatomär fysikAntiproton beamAntiprotonAntimatter0103 physical sciencesSubatomic PhysicsPhysics::Accelerator PhysicsNuclear Physics - Experimentddc:530010306 general physicsEPJ Web of Conferences
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Studies on Antihydrogen Atoms with the ATRAP Experiment at CERN

2013

The CPT theorem predicts the same properties of matter and antimatter, however, in the nearby Universe, we observe a huge imbalance of matter and antimatter. Therefore, it is intriguing to measure the properties of particles and antiparticles in order to contribute to an explanation of this phenomena. In this article, we will describe the experimental efforts of the ATRAP Collaboration in order to test the CPT theorem using antihydrogen atoms.

Nuclear physicsPhysics::Popular PhysicsPhysics::General PhysicsEngineeringLarge Hadron Colliderbusiness.industryPhysics::Atomic and Molecular ClustersGeneral Physics and AstronomyHigh Energy Physics::ExperimentAntihydrogenbusinessActa Physica Polonica B Proceedings Supplement
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Cryogenic Particle Accumulation In ATRAP And The First Antihydrogen Production Within A Magnetic Gradient Trap For Neutral Antimatter

2008

ATRAP has made many important improvements since CERN's Antiproton Decelerator (AD) was restarted in 2006. These include substantial increases in the number of positrons (e+) and antiprotons (Pbars) used to make antihydrogen (Hbar) atoms, a new technique for loading electrons (e−) that are used to cool Pbars and e+, implementation of a completely new, larger and more robust apparatus in our second experimental zone and the inclusion of a quadrupole Ioffe trap intended to trap the coldest Hbar atoms produced. Using this new apparatus we have produced large numbers of Hbar atoms within a Penning trap that is located within this quadrupole Ioffe trap using a new technique which shows promise f…

Condensed Matter::Quantum GasesPhysicsAntiparticleElectronPenning trapNuclear physicsAntiproton DeceleratorAntiprotonAntimatterQuadrupolePhysics::Accelerator PhysicsHigh Energy Physics::ExperimentPhysics::Atomic PhysicsAtomic physicsAntihydrogenAIP Conference Proceedings
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Efficient transfer of positrons from a buffer-gas-cooled accumulator into an orthogonally oriented superconducting solenoid for antihydrogen studies

2012

Positrons accumulated in a room-temperature buffer-gas-cooled positron accumulator are efficiently transferred into a superconducting solenoid which houses the ATRAP cryogenic Penning trap used in antihydrogen research. The positrons are guided along a 9 m long magnetic guide that connects the central field lines of the 0.15 T field in the positron accumulator to the central magnetic field lines of the superconducting solenoid. Seventy independently controllable electromagnets are required to overcome the fringing field of the large-bore superconducting solenoid. The guide includes both a 15° upward bend and a 105° downward bend to account for the orthogonal orientation of the positron accu…

Antiparticlesuperconductivity [solenoid]Physics::Instrumentation and DetectorsPenning trapGeneral Physics and Astronomybeam transportSuperconducting magnetlaw.inventionenergy spectrum [positron]Nuclear physicslawddc:530AntihydrogenPhysicsElectromagnetspatial distribution [magnetic field]ATRAPPenning trapMagnetic fieldbeam opticscryogenicsAntimatterMagnetPhysics::Accelerator Physicsaccumulator [positron]Atomic physicsperformanceNew Journal of Physics
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Electron-cooled accumulation of 4 × 109positrons for production and storage of antihydrogen atoms

2016

Four billion positrons (e+) are accumulated in a Penning–Ioffe trap apparatus at 1.2 K and <6 × 10−17 Torr. This is the largest number of positrons ever held in a Penning trap. The e+ are cooled by collisions with trapped electrons (e−) in this first demonstration of using e− for efficient loading of e+ into a Penning trap. The combined low temperature and vacuum pressure provide an environment suitable for antihydrogen () production, and long antimatter storage times, sufficient for high-precision tests of antimatter gravity and of CPT.

Condensed Matter::Quantum GasesPhysicsPhysics::General PhysicsAntiparticleAnnihilationPlasmaElectronCondensed Matter PhysicsPenning trap01 natural sciencesAtomic and Molecular Physics and Optics010305 fluids & plasmasNuclear physicsTorrAntimatter0103 physical sciencesPhysics::Atomic and Molecular ClustersPhysics::Atomic PhysicsAtomic physics010306 general physicsAntihydrogenJournal of Physics B: Atomic, Molecular and Optical Physics
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Antiproton confinement in a Penning-Ioffe trap for antihydrogen.

2007

Antiprotons ((p) over bar) remain confined in a Penning trap, in sufficient numbers to form antihydrogen ((H) over bar) atoms via charge exchange, when the radial field of a quadrupole Ioffe trap is added. This first demonstration with (p) over bar suggests that quadrupole Ioffe traps can be superimposed upon (p) over bar and e(+) traps to attempt the capture of (H) over bar atoms as they form, contrary to conclusions of previous analyses.

Condensed Matter::Quantum GasesPhysicsAntiparticleHigh Energy Physics::PhenomenologyGeneral Physics and AstronomyPenning trapJNuclear physicsAntiprotonAntimatterQuadrupoleddc:550Physics::Atomic and Molecular ClustersHigh Energy Physics::ExperimentPhysics::Atomic PhysicsIon trapAtomic physicsQuadrupole ion trapAntihydrogenPhysical review letters
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Centrifugal Separation of Antiprotons and Electrons

2010

Centrifugal separation of antiprotons and electrons is observed, the first such demonstration with particles that cannot be laser cooled or optically imaged. The spatial separation takes place during the electron cooling of trapped antiprotons, the only method available to produce cryogenic antiprotons for precision tests of fundamental symmetries and for cold antihydrogen studies. The centrifugal separation suggests a new approach for isolating low energy antiprotons and for producing a controlled mixture of antiprotons and electrons.

PhysicsAntiparticleGeneral Physics and AstronomyPlasmaElectronJlaw.inventionNuclear physicsAntiprotonlawAntimatterddc:550Physics::Accelerator PhysicsHigh Energy Physics::ExperimentPhysics::Atomic PhysicsAtomic physicsNuclear ExperimentAntihydrogenLeptonElectron coolingPhysical Review Letters
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Density and geometry of single component plasmas

2007

Abstract The density and geometry of p ¯ and e + plasmas in realistic trapping potentials are required to understand and optimize antihydrogen ( H ¯ ) formation. An aperture method and a quadrupole oscillation frequency method for characterizing such plasmas are compared for the first time, using electrons in a cylindrical Penning trap. Both methods are used in a way that makes it unnecessary to assume that the plasmas are spheroidal, and it is shown that they are not. Good agreement between the two methods illustrates the possibility to accurately determine plasma densities and geometries within non-idealized, realistic trapping potentials.

PhysicsNuclear and High Energy PhysicsOscillationGeometryPlasmaTrappingElectronPenning trapPhysics::Plasma PhysicsUpper hybrid oscillationQuadrupolePhysics::Atomic PhysicsAtomic physicsDetectors and Experimental TechniquesAntihydrogen
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One-Particle Measurement of the Antiproton Magnetic Moment

2013

\DeclareRobustCommand{\pbar}{\HepAntiParticle{p}{}{}\xspace} \DeclareRobustCommand{\p}{\HepParticle{p}{}{}\xspace} \DeclareRobustCommand{\mup}{$\mu_{p}${}{}\xspace} \DeclareRobustCommand{\mupbar}{$\mu_{\pbar}${}{}\xspace} \DeclareRobustCommand{\muN}{$\mu_N${}{}\xspace For the first time a single trapped \pbar is used to measure the \pbar magnetic moment ${\bm\mu}_{\pbar}$. The moment ${\bm\mu}_{\pbar} = \mu_{\pbar} {\bm S}/(\hbar/2)$ is given in terms of its spin ${\bm S}$ and the nuclear magneton (\muN) by $\mu_{\pbar}/\mu_N = -2.792\,845 \pm 0.000\,012$. The 4.4 parts per million (ppm) uncertainty is 680 times smaller than previously realized. Comparing to the proton moment measured using…

PhysicsParticle physicsProtonMagnetic momentAtomic Physics (physics.atom-ph)010308 nuclear & particles physicsOther Fields of PhysicsFOS: Physical sciencesGeneral Physics and Astronomy01 natural sciencesPhysics - Atomic PhysicsCrystallographyAntiproton0103 physical sciencesddc:550010306 general physicsNuclear magneton
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The ELENA facility

2018

The CERN Antiproton Decelerator (AD) provides antiproton beams with a kinetic energy of 5.3 MeV to an active user community. The experiments would profit from a lower beam energy, but this extraction energy is the lowest one possible under good conditions with the given circumference of the AD. The Extra Low Energy Antiproton ring (ELENA) is a small synchrotron with a circumference a factor of 6 smaller than the AD to further decelerate antiprotons from the AD from 5.3 MeV to 100 keV. Controlled deceleration in a synchrotron equipped with an electron cooler to reduce emittances in all three planes will allow the existing AD experiments to increase substantially their antiproton capture effi…

PhysicsLarge Hadron Collider010308 nuclear & particles physicsPhysics::Instrumentation and DetectorsGeneral MathematicsGeneral EngineeringGeneral Physics and AstronomyArticlesKinetic energy01 natural sciencesNuclear physicsAntiproton DeceleratorLow energyAntiproton0103 physical sciencesPhysics::Accelerator PhysicsHigh Energy Physics::Experiment010306 general physicsNuclear ExperimentBeam energy
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Mechanism of the Ne-22 (d, Li-6) O-18 reaction

1984

As part of a systematic study, the (d,Li6) reaction has been measured at a bombarding energy of 80 MeV on Ne22. Angular distributions were obtained in an angular range of 8° to 35° (lab). In the framework of finite-range distorted-wave Born approximation calculations, alpha spectroscopic factors were extracted. The strong collectivity of the low-lying states suggests the necessity of employing a coupled reaction channels formalism in the analysis. Indeed spectroscopic information arising from one-channel distorted-wave Born approximation calculations reveals significant differences between experimental and theoretical results. Furthermore, the shapes of some experimental angular distributio…

Física
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Determination of the eta'-proton scattering length in free space

2014

Taking advantage of both the high mass resolution of the COSY-11 detector and the high energy resolution of the low-emittance proton-beam of the Cooler Synchrotron COSY we determine the excitation function for the pp --&gt; pp eta' reaction close-to-threshold. Combining these data with previous results we extract the scattering length for the eta'-proton potential in free space to be Re(a_{p eta'}) = 0+-0.43 fm and Im(a_{p eta'}) = 0.37(+0.40)(-0.16) fm.

Physics::Accelerator PhysicsFOS: Physical sciencesHigh Energy Physics::ExperimentNuclear Experiment (nucl-ex)Nuclear ExperimentNuclear ExperimentAstrophysics::Galaxy Astrophysics
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