Search results for "Accelerator Physics"

showing 10 items of 1294 documents

Observation of a $\gamma$-decaying millisecond isomeric state in $^{128}$Cd$_{80}$

2017

A. Jungclaus et al. -- 6 pags., 5 figs., 2 tabs. -- Open Access funded by Creative Commons Atribution Licence 4.0

Shell model calculationNuclear and High Energy PhysicsFissionSHELL modelNuclear TheoryShell model calculationsTransition strengths[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciences7. Clean energy0103 physical sciencesmedicineddc:530010306 general physicsNuclear ExperimentPhysicsMillisecondRadionuclideIsomeric decay010308 nuclear & particles physicsProjectileParity (physics)lcsh:QC1-999medicine.anatomical_structureIsomeric decaysPhysics::Accelerator PhysicsTransition strengthAtomic physicsNucleuslcsh:Physics
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Modeling particle acceleration and non-thermal emission in supernova remnants

2021

According to the most popular model for the origin of cosmic rays (CRs), supernova remnants (SNRs) are the site where CRs are accelerated. Observations across the electromagnetic spectrum support this picture through the detection of non-thermal emission that is compatible with being synchrotron or inverse Compton radiation from high energy electrons, or pion decay due to proton-proton interactions. These observations of growing quantity and quality promise to unveil many aspects of CRs acceleration and require more and more accurate tools for their interpretation. Here, we show how multi-dimensional MHD models of SNRs, including the effects on shock dynamics due to back-reaction of acceler…

Shock waveMagnetohydrodynamics (MHD)Radiation mechanisms: non-thermalElectromagnetic spectrumAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayAstrophysicsElectronRadiation01 natural sciencesShock wavesAcceleration0103 physical sciencesCosmic rays010303 astronomy & astrophysicsInstrumentationAstrophysics::Galaxy AstrophysicsISM: supernova remnantsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsAstronomy and AstrophysicsParticle accelerationSupernovaSpace and Planetary SciencePhysics::Accelerator PhysicsAstrophysics - High Energy Astrophysical Phenomena
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Laboratory evidence for proton energization by collisionless shock surfing

2021

Charged particles can be accelerated to high energies by collisionless shock waves in astrophysical environments, such as supernova remnants. By interacting with the magnetized ambient medium, these shocks can transfer energy to particles. Despite increasing efforts in the characterization of these shocks from satellite measurements at Earth’s bow shock as well as powerful numerical simulations, the underlying acceleration mechanism or a combination thereof is still widely debated. Here we show that astrophysically relevant super-critical quasi-perpendicular magnetized collisionless shocks can be produced and characterized in the laboratory. We observe the characteristics of super-criticali…

Shock waveProtonAstrophysics::High Energy Astrophysical PhenomenaGeneral Physics and AstronomyFOS: Physical sciences01 natural sciencesAccelerationSettore FIS/05 - Astronomia E Astrofisica0103 physical sciencesBow shock (aerodynamics)010306 general physics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsMechanicsplasmasPhysics - Plasma PhysicsCharged particleComputer Science::Computers and Society[PHYS.PHYS.PHYS-GEN-PH]Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]Magnetic fieldShock (mechanics)Plasma Physics (physics.plasm-ph)Supernova13. Climate actionPhysics::Space PhysicsPhysics::Accelerator Physics
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Search for Isovector Valence-Shell Excitations in 140 Nd and 142 Sm via Coulomb excitation reactions of radioactive ion beams

2018

Projectile Coulomb excitation experiments were performed at HIE-ISOLDE at CERN with the radioactive ion beams of 140Nd and 142Sm. Ions with an energy of 4:62 MeV/A were impinging on a 1.45 mg/cm2 thick 208Pb target. The γ-rays depopulating the Coulomb-excited states were recorded by the HPGe-array MINIBALL and scattered particles were detected by a double-sided silicon strip detector. Experimental intensities were used for the determination of electromagnetic transition matrix elements. A preliminary result of the B(M1; 2+3 → 2+1) of 140Nd and an upper limit for the case of 142Sm are revealing the main fragments of the proton-neutron mixed-symmetry 2+1;ms states.

SiliconPhysics::Instrumentation and DetectorsQC1-999chemistry.chemical_elementCoulomb excitation01 natural sciencesIon0103 physical sciencesNuclear Physics - ExperimentNuclear Experiment010306 general physicsCoulomb excitation experimentsPhysicsLarge Hadron ColliderIsovectorta114010308 nuclear & particles physicsProjectilePhysicsDetectorchemistryPhysics::Accelerator PhysicsAtomic physicsValence electronydinfysiikkaEPJ Web of Conferences
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"Table 2" of "Quasi-free Compton Scattering and the Polarizabilities of the Neutron"

2003

Energy dependence of the quasi-free proton differential cross section.

Single Differential Cross SectionPhotoproduction1.146-1.266ElasticNuclear TheoryPhysics::Accelerator PhysicsGAMMA P --> GAMMA PNuclear ExperimentDSIG/DOMEGA
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"Table 1" of "Quasi-free Compton Scattering and the Polarizabilities of the Neutron"

2003

Energy dependence of the free-proton differential cross section.

Single Differential Cross SectionPhotoproductionElasticNuclear TheoryPhysics::Accelerator PhysicsGAMMA P --> GAMMA P1.13-1.327Nuclear ExperimentDSIG/DOMEGA
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A reservoir trap for antiprotons

2015

We have developed techniques to extract arbitrary fractions of antiprotons from an accumulated reservoir, and to inject them into a Penning-trap system for high-precision measurements. In our trap-system antiproton storage times > 1.08 years are estimated. The device is fail-safe against power-cuts of up to 10 hours. This makes our planned comparisons of the fundamental properties of protons and antiprotons independent from accelerator cycles, and will enable us to perform experiments during long accelerator shutdown periods when background magnetic noise is low. The demonstrated scheme has the potential to be applied in many other precision Penning trap experiments dealing with exotic p…

Speichertechnik - Abteilung BlaumPhysics - Instrumentation and DetectorsMagnetic noiseAtomic Physics (physics.atom-ph)Other Fields of PhysicsFOS: Physical sciences7. Clean energy01 natural sciencesIon trappingphysics.atom-ph010305 fluids & plasmasPhysics - Atomic PhysicsNuclear physicsTrap (computing)0103 physical sciencesPhysics::Atomic PhysicsPhysical and Theoretical ChemistryDetectors and Experimental Techniques010306 general physicsNuclear ExperimentInstrumentationphysics.ins-detSpectroscopyPhysicsInstrumentation and Detectors (physics.ins-det)Condensed Matter PhysicsPenning trapAntiprotonPhysics::Accelerator Physics
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"Table 10" of "A study of strange particle production in nu/mu charged current interactions in the NOMAD experiment."

2002

Ratios of measured yields for K0S/LAMBDA and LAMBDABAR/LAMBDA as a functionof the Bjorken X variable.

Strange productionNUMU NUCLEON --> MU- KS XHigh Energy Physics::PhenomenologyDeep Inelastic ScatteringNNUMU NUCLEON --> MU- LAMBDA XMuon productionInclusiveNUMU NUCLEON --> MU- LAMBDABAR X9.266Physics::Accelerator PhysicsHigh Energy Physics::ExperimentCharged CurrentNuclear Experiment
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Development of Stripline Kickers for Low Emittance Rings: Application to the Beam Extraction Kicker for CLIC Damping Rings

2015

163 páginas. Tesis Doctoral del Departamento de Física Atómica, Molecular y Nuclear de la Universidad de Valencia y del Instituto de Física Corpuscular (IFIC).

StriplinesLow emittance ringsKickerFísica experimental de Altas EnergíasPhysics::Accelerator PhysicsDamping ringsCLICAccelerators and Storage Rings
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Further RF Measurements on the Superconducting 217 MHz CH Demonstrator Cavity for a CW Linac at GSI

2019

Proceedings of the 10th International Particle Accelerator Conference The 10th International Particle Accelerator Conference, Melbourne, Australia, 19 May 2019 - 24 May 2019; Geneva : JACoW Publishing, CERN 2826-2829 (2019). doi:10.18429/JACOW-IPAC2019-WEPRB014

SuperconductivityHistoryMC7: Accelerator TechnologyMaterials sciencebusiness.industryPhase (waves)Injector530Linear particle acceleratorAccelerator PhysicsComputer Science ApplicationsEducationlaw.inventionIonHeavy ion beamlawOptoelectronicsContinuous waveddc:530businessBeam (structure)
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