Search results for "antiproton"

showing 10 items of 183 documents

Antihydrogen production in a combined trap

1993

In this paper we study the properties of a Paul trap with a superimposed magnetic field (combined trap) and discuss the possibility of using this trap to simultaneously store positrons and antiprotons to form antihydrogen.

Condensed Matter::Quantum GasesPhysicsNuclear and High Energy PhysicsCondensed Matter PhysicsAtomic and Molecular Physics and OpticsMagnetic fieldTrap (computing)Nuclear physicsAntiprotonPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentPhysics::Atomic PhysicsIon trapPhysical and Theoretical ChemistryAtomic physicsAntihydrogenHyperfine Interactions
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Extremely cold antiprotons for antihydrogen production

1993

The possibility to produce, trap and study antihydrogen atoms rests upon the recent availability of extremely cold antiprotons in a Penning trap. Over the last five years, our TRAP Collaboration has slowed, cooled and stored antiprotons at energies 1010 lower than was previously possible. The storage time exceeds 3.4 months despite the extremely low energy, which corresponds to 4.2 K in temperature units. The first example of measurements which become possible with extremely cold antiprotons is a comparison of the antiproton inertial masses which shows they are the same to a fractional accuracy of 4×10−8. (This is 1000 times more accurate than previous comparisons and large additional incre…

Condensed Matter::Quantum GasesPhysicsNuclear and High Energy PhysicsCondensed Matter PhysicsPenning trapAtomic and Molecular Physics and OpticsNuclear physicsTrap (computing)Low energyAntiprotonHigh Energy Physics::ExperimentPhysics::Atomic PhysicsPhysical and Theoretical ChemistryAtomic physicsNuclear ExperimentAntihydrogenHyperfine Interactions
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A single trapped antiproton and antiprotons for antihydrogen production

1993

During the last several years, our TRAP collaboration has pioneered techniques for slowing, trapping, cooling and indefinitely storing antiprotons to energies more than 1010 times lower than previously possible. The radio signal from a single trapped antiproton is now being used for precision measurements. Many cold antiprotons are “stacked” as another important step toward the eventual production of antihydrogen, and positrons have been trapped in vacuum.

Condensed Matter::Quantum GasesPhysicsNuclear and High Energy PhysicsParticle physicsTrappingCondensed Matter PhysicsAtomic and Molecular Physics and OpticsTrap (computing)Nuclear physicsAntiprotonRadio signalPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentPhysics::Atomic PhysicsPhysical and Theoretical ChemistryAntihydrogenHyperfine Interactions
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Using electric fields to prevent mirror-trapped antiprotons in antihydrogen studies

2013

The signature of trapped antihydrogen ($\overline{\mathrm{H}}$) atoms is the annihilation signal detected when the magnetic trap that confines the atoms is suddenly switched off. This signal would be difficult to distinguish from the annihilation signal of any trapped $\overline{p}$ that is released when the magnetic trap is switched off. This work deduces the large cyclotron energy ($g$137 eV) required for magnetic trapping of $\overline{p}$, considers the possibility that such $\overline{p}$ are produced, and explores the effectiveness of an electric field applied to clear charged particles from the trapping volume before $\overline{\mathrm{H}}$ detection. No mechanisms are found that can…

Condensed Matter::Quantum GasesPhysicsParticle physicsAnnihilationHigh Energy Physics::PhenomenologyCyclotronAtomic and Molecular Physics and OpticsCharged particlelaw.inventionlawAntiprotonElectric fieldMagnetic trapPhysics::Atomic PhysicsAtomic physicsAntihydrogenEnergy (signal processing)Physical Review A
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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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Radio data and synchrotron emission in consistent cosmic ray models

2011

It is well established that phenomenological two-zone diffusion models of the galactic halo can very well reproduce cosmic-ray nuclear data and the observed antiproton flux. Here, we consider lepton propagation in such models and compute the expected galactic population of electrons, as well as the diffuse synchrotron emission that results from their interaction with galactic magnetic fields. We find models in agreement not only with cosmic ray data but also with radio surveys at essentially all frequencies. Requiring such a globally consistent description strongly disfavors very large ($L\gtrsim 15$ kpc) and, even stronger, small ($L\lesssim 1$ kpc) effective diffusive halo sizes. This has…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical PhenomenaPopulationDark matterFOS: Physical sciencesSynchrotron radiationCosmic rayAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesGalactic haloHigh Energy Physics - Phenomenology (hep-ph)0103 physical scienceseducation010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicseducation.field_of_studydark matter theorycosmic ray theory; dark matter theory010308 nuclear & particles physicsAstronomy and Astrophysicscosmic ray theoryAstrophysics - Astrophysics of GalaxiesHigh Energy Physics - PhenomenologyAntiprotonAstrophysics of Galaxies (astro-ph.GA)HaloAstrophysics - Cosmology and Nongalactic AstrophysicsRadio waveJournal of Cosmology and Astroparticle Physics
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Polarization in p-p and $$\bar p - p$$ elastic scatteringelastic scattering

1970

Elastic scatteringPhysicsCondensed matter physicsAntiprotonScatteringGeneral Physics and AstronomyElementary particlePolarization (waves)Lettere al Nuovo Cimento
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"Table 3" of "Measurements of the anti-proton - proton elastic cross-section in the beam momentum range between 180-MeV/c and 600-MeV/c"

1992

No description provided.

ElasticIntegrated Cross SectionCross SectionProton-AntiProton Elastic Cross SectionSIGPBAR P --> PBAR P
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"Table 1" of "Measurements of the anti-proton - proton elastic cross-section in the beam momentum range between 180-MeV/c and 600-MeV/c"

1992

No description provided.

ElasticIntegrated Cross SectionCross SectionProton-AntiProton Elastic Cross SectionSIGPBAR P --> PBAR P
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"Table 2" of "Measurements of the anti-proton - proton elastic cross-section in the beam momentum range between 180-MeV/c and 600-MeV/c"

1992

No description provided.

ElasticIntegrated Cross SectionCross SectionProton-AntiProton Elastic Cross SectionSIGPBAR P --> PBAR P
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