Search results for "Synchro"

showing 10 items of 886 documents

Spin polarisation and dichroism in ARUPS from thin rare earth films

2001

Abstract In the present study, spin polarisation and dichroism were investigated in angular resolved VUV photoemission ARUPS from magnetised as well as paramagnetic rare earth surfaces. Thin Gd(0001) films were prepared epitaxially on W(110). The photoelectrons were excited by polarised synchrotron radiation from the BESSY I synchrotron radiation source. A SPLEED detector attached to an electron spectrometer mounted on a single axis goniometer was used for angular resolved spin analysis. The main part of this work focused on the characteristic surface state of Gd(0001) which shows a splitting, as previously observed by linear magnetic dichroism and spin polarised photoemission. The spin ana…

PhysicsCircular dichroismRadiationElectron spectrometerMagnetismSynchrotron Radiation SourceSynchrotron radiationAngle-resolved photoemission spectroscopyDichroismCondensed Matter PhysicsAtomic and Molecular Physics and OpticsElectronic Optical and Magnetic MaterialsCondensed Matter::Materials ScienceCrystallographyCondensed Matter::Strongly Correlated ElectronsPhysical and Theoretical ChemistryAtomic physicsSpin (physics)SpectroscopyJournal of Electron Spectroscopy and Related Phenomena
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Stability and Chaos

2010

In this chapter we study a larger class of dynamical systems that include but go beyond Hamiltonian systems. We are interested, on the one hand, in dissipative systems, i.e. systems that lose energy through frictional forces or into which energy is fed from exterior sources, and, on the other hand, in discrete, or discretized, systems such as those generated by studying flows by means of the Poincare mapping. The occurence of dissipation implies that the system is coupled to other, external systems, in a controllable manner. The strength of such couplings appears in the set of solutions, usually in the form of parameters. If these parameters are varied it may happen that the flow undergoes …

PhysicsClassical mechanicsFlow (mathematics)Dynamical systems theoryIntegrable systemSynchronization of chaosDissipative systemDegrees of freedom (physics and chemistry)DissipationHamiltonian system
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Laser cooling of relativistic heavy-ion beams for FAIR

2015

Laser cooling is a powerful technique to reduce the longitudinal momentum spread of stored relativistic ion beams. Based on successful experiments at the experimental storage ring at GSI in Darmstadt, of which we show some important results in this paper, we present our plans for laser cooling of relativistic ion beams in the future heavy-ion synchrotron SIS100 at the Facility for Antiproton and Ion Research in Darmstadt.

PhysicsCondensed Matter PhysicsAtomic and Molecular Physics and OpticsSynchrotronCharged particlelaw.inventionIonNuclear physicsPhysics::Plasma PhysicslawAntiprotonLaser coolingAntimatterPhysics::Accelerator PhysicsFacility for Antiproton and Ion ResearchPhysics::Atomic PhysicsNuclear ExperimentMathematical PhysicsStorage ringPhysica Scripta
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Circular dichroism in x-ray photoemission from core levels of nonmagnetic species

1992

Circular dichroism in the angular distribution of photoelectrons (CDAD) has been observed in core-level photoemission from spherically symmetric initial states of nonmagnetic species utilizing circularly polarized soft-x-ray radiation from BESSY. Up to now, CDAD was predicted and observed only for aligned initial states. The data for oriented CO molecules prove that circular x-ray dichroism in photoemission from core levels is a general phenomenon that is not restricted to ferromagnets. High asymmetries of 50% suggest future applications as an effective circular x-ray analyzer.

PhysicsCondensed Matter::Materials ScienceCircular dichroismFerromagnetismX-ray magnetic circular dichroismVibrational circular dichroismX-raySynchrotron radiationCondensed Matter::Strongly Correlated ElectronsAtomic physicsDichroismPhotoelectric effectPhysical Review B
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Frontiers of Heavy - Ion Physics and Superheavy Elements

2003

This contribution will focus on three topics of GSI nuclear structure research: super heavy elements, direct mass measurements in the storage ring, and the measurement of spallation cross section in reversed kinematics. The GSI project for an extended synchrotron facility will be outlined.

PhysicsFocus (computing)Nuclear and High Energy PhysicsFissionNuclear structureTransactinide elementSuperheavy ElementsSynchrotronlaw.inventionNuclear physicsCross section (physics)Nuclear Energy and EngineeringlawHeavy ionSpallationStorage ringJournal of Nuclear Science and Technology
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Synchrotron Radiation from the Crab Nebula Discriminates between Models of Space-Time Foam

2003

It has been argued by Jacobson, Liberati and Mattingly that synchrotron radiation from the Crab Nebula imposes a stringent constraint on any modification of the dispersion relations of the electron that might be induced by quantum gravity. We supplement their analysis by deriving the spectrum of synchrotron radiation from the coupling of an electrically-charged particle to an external magnetic fields in the presence of quantum-gravity effects of the general form $(E/M_{QG})^\alpha$. We find that the synchrotron constraint from the Crab Nebula practically excludes $\alpha \lsim 1.74$ for $M_{QG} \sim m_P = 1.2 \times 10^{19}$ GeV. On the other hand, this analysis does not constrain any modif…

PhysicsHigh Energy Physics - TheoryAstrophysics and AstronomyPhotonAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)Synchrotron radiationFOS: Physical sciencesAstronomy and AstrophysicsElectronGeneral Relativity and Quantum Cosmology (gr-qc)AstrophysicsSynchrotronGeneral Relativity and Quantum CosmologyComputational physicslaw.inventionNuclear physicsHigh Energy Physics - PhenomenologyCrab NebulaHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)lawDispersion relationQuantum gravityEquivalence principle
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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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Dark matter synchrotron emission and radio observations

2012

We compute the synchrotron emission induced by electrons produced by DM annihilations inside our galaxy. The signal is compared with observations in a large range of frequencies, from 22 MHz up to 1420 MHz. We set constraints on the DM mass and annihilation cross-section and highlight the impact of astrophysical uncertainties.

PhysicsHistoryAnnihilationHot dark matterDark matterAstronomyAstrophysicsLarge rangeElectronSignalGalaxyComputer Science ApplicationsEducationSynchrotron emissionPhysics::Accelerator PhysicsJournal of Physics: Conference Series
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Fast timing and trigger Cherenkov detector for collider experiments

2016

Analysis of fast timing and trigger Cherenkov detector's design for its use in collider experiments is presented. Several specific requirements are taken into account - necessity of the radiator's placement as close to the beam pipe as possible along with the requirement of gapless (solid) radiator's design. Characteristics of the Cherenkov detector's laboratory prototype obtained using a pion beam at the CERN Proton Synchrotron are also presented, showing the possibility of obtaining sufficiently high geometrical efficiency along with good enough time resolution (50 ps sigma).

PhysicsHistoryLarge Hadron ColliderPhysics::Instrumentation and DetectorsCherenkov detectorProton SynchrotronTime resolutionComputer Science ApplicationsEducationlaw.inventionNuclear physicsGapless playbacklawRadiator (engine cooling)Physics::Accelerator PhysicsHigh Energy Physics::ExperimentColliderBeam (structure)Journal of Physics: Conference Series
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Galactic synchrotron emission from astrophysical electrons

2012

The interaction between the galactic magnetic field and the non-thermal population of electrons is responsible for a large part of the radio sky from 10 MHz up to several GHz. This population is mostly composed of electrons with primary and secondary origin. Cosmic ray propagation models describe their evolution in space and energy, and allow to study the impact on the radio sky in intensity and morphology at different frequencies. We consider different propagation models and test their compatibility with available radio maps. We find models highly consistent both with B/C data, the local electron flux and synchrotron emission observations. The resulting constraints on propagation models co…

PhysicsHistoryeducation.field_of_studyAstrophysics::High Energy Astrophysical Phenomenamedia_common.quotation_subjectDark matterPopulationAstronomyCosmic rayAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsElectronComputer Science ApplicationsEducationMagnetic fieldSynchrotron emissionSkyAntiprotoneducationmedia_common
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