Search results for "Synchrotron"

showing 10 items of 307 documents

Design and commissioning of the GSI pion beam

2002

We describe the design of the secondary pion beam-line installed at the SIS 18Tm synchrotron at GSI, Darmstadt, and discuss the commissioning results. The experiments were performed with proton and C-12 primary beams at several energies using beryllium production targets. Pion yields in a momentum range between 0.4 and 2.8 GeV/c were identified, At the highest primary beam energies of 3.5 GeV for proton and 2.0 A GeV for carbon ions, the latter beam produces the highest low-momentum pion yield while at momenta of 1.5 GeV/c the yields are comparable and at 2.8 GeV/c the proton beam is superior. A momentum resolution of around 0.5% is achieved and the time resolution (a) ranges from 100 to 15…

PhysicsNuclear and High Energy PhysicsParticle physicsRange (particle radiation)ProtonNuclear Theorychemistry.chemical_elementSynchrotronlaw.inventionNuclear physicsMomentumTime of flightPionchemistrylawPhysics::Accelerator PhysicsHigh Energy Physics::Experiment[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]BerylliumNuclear ExperimentInstrumentationBeam (structure)Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Studies of high density baryon matter with high intensity heavy-ion beams at J-PARC

2016

Abstract In J-PARC heavy-ion project, we aim at studies of QCD phase structures and hadron properties in high baryon density close to the neutron star core. We have developed a heavy-ion acceleration scheme with a new linac and a new booster with existing two synchrotrons with the goal beam rate of about 10 11 Hz. We have also designed a large acceptance spectrometer based on a toroidal magnet. We have evaluated the spectrometer performance, and demonstrated reconstructing dielectron and dimuon spectra with full detector simulations. Finally, we designed a hypernuclear spectrometer which can utilize the full intensity ion beams.

PhysicsNuclear and High Energy PhysicsParticle physicsSpectrometerIon beam010308 nuclear & particles physicsHadron01 natural sciencesSynchrotronLinear particle acceleratorlaw.inventionBaryonNuclear physicslaw0103 physical sciencesPhysics::Accelerator PhysicsJ-PARCNuclear Experiment010306 general physicsBeam (structure)Nuclear Physics A
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Novel optical interferometry of synchrotron radiation for absolute electron beam energy measurements

2018

Abstract A novel interferometric method is presented for the measurement of the absolute energy of electron beams. In the year 2016, a pioneering experiment was performed using a 195 MeV beam of the Mainz Microtron (MAMI). The experimental setup consisted of two collinear magnetic undulators as sources of coherent optical synchrotron light and a high-resolving grating monochromator. Beam energy measurements required the variation of the relative undulator distance in the decimeter range and the analysis of the intensity oscillation length in the interference spectrum. A statistical precision of 1 keV was achieved in 1 h of data taking, while systematic uncertainties of 700 keV were present …

PhysicsNuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsSpectrometer010308 nuclear & particles physicsbusiness.industrySynchrotron radiationFOS: Physical sciencesParticle acceleratorInstrumentation and Detectors (physics.ins-det)Undulator01 natural sciencesSynchrotronlaw.inventionOpticslaw0103 physical sciencesPhysics::Accelerator Physics010306 general physicsbusinessNuclear ExperimentInstrumentationMicrotronBeam (structure)Monochromator
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High brilliance uranium beams for the GSI FAIR

2017

The 40 years old GSI-UNILAC (Universal Linear Accelerator) as well as the heavy ion synchrotron SIS18 will serve as a high current heavy ion injector for the new FAIR (Facility for Antiproton and Ion Research) synchrotron SIS100. In the context of an advanced machine investigation program in combination with the ongoing UNILAC upgrade program, a new uranium beam intensity record (11.5 emA, ${\mathrm{U}}^{29+}$) at very high beam brilliance was achieved recently in a machine experiment campaign. This is an important step paving the way to fulfill the FAIR heavy ion high intensity beam requirements. Results of high current uranium beam measurements applying a newly developed pulsed hydrogen g…

PhysicsNuclear and High Energy PhysicsPhysics and Astronomy (miscellaneous)010308 nuclear & particles physicschemistry.chemical_elementContext (language use)Surfaces and InterfacesUranium01 natural sciencesSynchrotronlaw.inventionNuclear physicsUpgradechemistrylawUniversal linear accelerator0103 physical sciencesPhysics::Accelerator PhysicsFacility for Antiproton and Ion Researchlcsh:QC770-798lcsh:Nuclear and particle physics. Atomic energy. RadioactivityNuclear Experiment010306 general physicsIntensity (heat transfer)Beam (structure)Physical Review Accelerators and Beams
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The polytron as a cw electron accelerator in the 10 GeV range

1991

Abstract This article is concerned with a generalized microtron, characterized essentially by the number of magnet pairs in its bending system. It is shown that the most serious physical energy limit of the microtron, emittance growth due to synchrotron radiation, may be overcome if this number is raised essentially above what has been considered in the past. The main properties of such “polytrons” are investigated and several design examples for 15 GeV output energy are discussed.

PhysicsNuclear and High Energy PhysicsRange (particle radiation)Synchrotron radiationParticle acceleratorBendinglaw.inventionNuclear physicslawMagnetLimit (music)Physics::Accelerator PhysicsThermal emittanceNuclear ExperimentInstrumentationMicrotronNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Search for a neutral Higgs particle in the decay sequence $K^{0}_{L} \to \pi^{0}H^{0}$ and $H^{0} \to e^{+}e^{-}$

1990

Abstract We have searched for the sequence of decays K L 0 → π 0 H 0 and H 0 →e + e − at the CERN Super Proton Synchrotron (SPS), and have allowed for a non-zero H 0 lifetime. Three candidates have been seen, consistent with an expected background of 3.3. Limits on the branching ratio product in the range 10 −8 –10 −7 are presented as a function of the mass and lifetime of the H 0 . These can be used to restrict the neutral Higgs of the minimal standard model.

PhysicsNuclear and High Energy PhysicsSequenceParticle physicsRange (particle radiation)Large Hadron ColliderBranching fractionElementary particleSuper Proton SynchrotronStandard ModelNuclear physicsHiggs bosonHigh Energy Physics::ExperimentParticle Physics - Experiment
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EXTRACTION OF ΛΛ SCATTERING LENGTH

2009

We determine ΛΛ scattering parameters from a ΛΛ invariant mass spectrum that was obtained by 12 C (K-, K+ΛΛ) reaction at the KEK Proton Synchrotron. In the framework of Watson's procedure, the obtained scattering length [Formula: see text] and effective range [Formula: see text] are most consistent with the values predicted by using the Nijmegen soft core models (NSC97's). However, the predicted values by using the Nijmegen hard-core ND ( G -matrix) and the extended soft-core (ESC00) models are out of two standard deviations from the determined scattering parameters.

PhysicsNuclear physicsNuclear and High Energy PhysicsRange (particle radiation)Soft coreExtraction (chemistry)Scattering parametersGeneral Physics and AstronomyProton SynchrotronInvariant massScattering lengthLambdaStandard deviationInternational Journal of Modern Physics E
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Dielectron production in Au + Au collisions atsNN=200GeV

2016

We present measurements of e+e- production at midrapidity in Au+Au collisions at sNN=200 GeV. The invariant yield is studied within the PHENIX detector acceptance over a wide range of mass (mee<5 GeV/c2) and pair transverse momentum (pT<5 GeV/c) for minimum bias and for five centrality classes. The e+e- yield is compared to the expectations from known sources. In the low-mass region (mee=0.30-0.76 GeV/c2) there is an enhancement that increases with centrality and is distributed over the entire pair pT range measured. It is significantly smaller than previously reported by the PHENIX experiment and amounts to 2.3±0.4(stat)±0.4(syst)±0.2(model) or to 1.7±0.3(stat)±0.3(syst)±0.2(model) for min…

PhysicsParticle physicsMeson010308 nuclear & particles physicsDalitz plot01 natural sciencesSuper Proton SynchrotronParticle identificationNuclear physicsPair production0103 physical sciencesHigh Energy Physics::ExperimentRapidityPHENIX detectorNuclear Experiment010306 general physicsGlauberPhysical Review C
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The evolution of the large-scale emission in Fanaroff-Riley type I jets

2011

Recent observations in X-rays and gamma-rays of nearby Fanaroff-Riley type I (FR I) radio galaxies have raised the question of the origin of the emission detected in the termination structures of their jets. The study of these structures can give information on the conditions for particle acceleration and radiation at the front shocks. In addition, an evolutionary scenario can help to disentangle the origin of the detected X-ray emission in young FR I sources, like some gigahertz peaked spectrum active galactic nuclei. This work focuses on the nature and detectability of the radiation seen from the termination regions of evolving FR I jets. We use the results of a relativistic, two-dimensio…

PhysicsPhotonActive galactic nucleusRadio galaxyAstrophysics::High Energy Astrophysical PhenomenaCosmic microwave backgroundCosmic background radiationSynchrotron radiationAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsLight curveParticle accelerationSpace and Planetary ScienceMonthly Notices of the Royal Astronomical Society
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Orbital X‐Ray Variability of the Microquasar LS 5039

2005

The properties of the orbit and the donor star in the high mass X-ray binary microquasar LS 5039 indicate that accretion processes should mainly occur via a radiatively driven wind. In such a scenario, significant X-ray variability would be expected due to the eccentricity of the orbit. The source has been observed at X-rays by several missions, although with a poor coverage that prevents to reach any conclusion about orbital variability. Therefore, we conducted RossiXTE observations of the microquasar system LS 5039 covering a full orbital period of 4 days. Individual observations are well fitted with an absorbed power-law plus a Gaussian at 6.7 keV, to account for iron line emission that …

PhysicsPhotonAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)FOS: Physical sciencesBinary numberAstronomy and AstrophysicsAstrophysicsCompact starRadiationAstrophysicsEphemerisOrbital periodSynchrotronAccretion (astrophysics)law.inventionX-ray binariesSpace and Planetary SciencelawX-raysRaigs XAstrophysics::Earth and Planetary AstrophysicsQuasarsQuàsarsEstels binaris de raigs XThe Astrophysical Journal
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