Search results for "Plasma oscillation"

showing 7 items of 7 documents

Broadband microwave emission spectrum associated with kinetic instabilities in minimum-B ECR plasmas

2017

Plasmas of electron cyclotron resonance ion sources (ECRISs) are prone to kinetic instabilities due to the resonant heating mechanism resulting in anisotropic electron velocity distribution. Frequently observed periodic oscillations of extracted ion beam current in the case of high plasma heating power and/or strong magnetic field have been proven to be caused by cyclotrontype instabilities leading to a notable reduction and temporal variation of highly charged ion production. Thus, investigations of such instabilities and techniques for their suppression have become important topics in ECRIS research. The microwave emission caused by the instabilities contains information on the electron e…

010302 applied physicsPhysicsRange (particle radiation)microwave sourcesIon sourcesIon beamta114Highly charged ionPlasmaAstrophysics::Cosmology and Extragalactic Astrophysicsplasma instabilitiesmagnetic fieldsCondensed Matter PhysicsPlasma oscillationmagneettikentät01 natural sciences7. Clean energyElectron cyclotron resonanceIonPhysics::Plasma Physicsmicrowave spectra0103 physical sciencesAtomic physics010306 general physicsMicrowave
researchProduct

Flux flow effects in very long Josephson junctions

2000

We report on measurements on very long, L ≃ 30λj, NbAlOxNb underdamped in-line junctions, on which we observed displaced linear slope (DLS) generated by the application of an external magnetic field. We study the behaviour of the branches as a function of the applied magnetic field in terms of both current amplitude and voltage position. The DLS is seen to shift rigidly towards higher voltages when increasing the field, spanning a region roughly centred around the Josephson plasma frequency. We discuss the behaviour of linear branches in terms of one dimensional flux-flow along the extended side of the junction, comparing our data with the results of numerical modeling; from these calculat…

Josephson effectPi Josephson junctionPhysicsSettore FIS/03Condensed matter physicsField (physics)Position (vector)Statistical and Nonlinear PhysicsFunction (mathematics)Condensed Matter PhysicsPlasma oscillationMagnetic fieldVoltage
researchProduct

Dark photon dark matter in the presence of inhomogeneous structure

2020

Dark photon dark matter will resonantly convert into visible photons when the dark photon mass is equal to the plasma frequency of the ambient medium. In cosmological contexts, this transition leads to an extremely efficient, albeit short-lived, heating of the surrounding gas. Existing work in this field has been predominantly focused on understanding the implications of these resonant transitions in the limit that the plasma frequency of the Universe can be treated as being perfectly homogeneous, i.e. neglecting inhomogeneities in the electron number density. In this work we focus on the implications of heating from dark photon dark matter in the presence of inhomogeneous structure (which …

Nuclear and High Energy PhysicsPhotonCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsPlasma oscillation01 natural sciencesDark photon[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]High Energy Physics - Phenomenology (hep-ph)0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. RadioactivityThermal Field Theory010306 general physicsReionizationPhysicsRange (particle radiation)010308 nuclear & particles physicsStar formationFísicaCosmology of Theories beyond the SMHigh Energy Physics - PhenomenologyOrders of magnitude (time)[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]lcsh:QC770-798Astrophysics - Cosmology and Nongalactic AstrophysicsJournal of High Energy Physics
researchProduct

Modeling dark photon oscillations in our inhomogeneous Universe

2020

A dark photon may kinetically mix with the Standard Model photon, leading to observable cosmological signatures. The mixing is resonantly enhanced when the dark photon mass matches the primordial plasma frequency, which depends sensitively on the underlying spatial distribution of electrons. Crucially, inhomogeneities in this distribution can have a significant impact on the nature of resonant conversions. We develop and describe, for the first time, a general analytic formalism to treat resonant oscillations in the presence of inhomogeneities. Our formalism follows from the theory of level crossings of random fields and only requires knowledge of the one-point probability distribution func…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)PhotonRandom fieldPhoton conversion010308 nuclear & particles physicsFOS: Physical sciencesObservableProbability density functionElectronAstrophysics::Cosmology and Extragalactic AstrophysicsPlasma oscillation01 natural sciencesDark photonHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Quantum electrodynamics0103 physical sciences010306 general physicsAstrophysics - Cosmology and Nongalactic Astrophysics
researchProduct

Stability of gyrotron operation in very high-order modes

2012

This study was motivated by the desire to increase the power, which can be delivered by gyrotrons in long pulse and continuous regimes. Since the admissible power level is determined by the density of ohmic losses in resonator walls, to increase the radiated power a gyrotron should operate in higher order modes. Using an existing gyrotron developed for plasma experiments in the International Thermonuclear Experimental Reactor as a base model, the stability of operation of such a gyrotron in modes with larger number of radial variations was studied. It is shown that the power level achievable in such gyrotrons in stable single mode regimes is close to 1.5 MW. The power level 1.7–1.8 MW can b…

PhysicsThermonuclear fusionTerahertz radiationAmplifierSingle-mode optical fiberMechanicsPlasmaEffective radiated powerCondensed Matter PhysicsPlasma oscillationStability (probability)Power (physics)Computational physicslaw.inventionAmplitude modulationResonatorNuclear magnetic resonanceControl theoryPhysics::Plasma PhysicslawGyrotronHigh orderOhmic contactNumerical stabilityPhysics of Plasmas
researchProduct

Transverse distribution of beam current oscillations of a 14 GHz electron cyclotron resonance ion source

2014

The temporal stability of oxygen ion beams has been studied with the 14 GHz A-ECR at JYFL (University of Jyvaskyla, Department of Physics). A sector Faraday cup was employed to measure the distribution of the beam current oscillations across the beam profile. The spatial and temporal characteristics of two different oscillation “modes” often observed with the JYFL 14 GHz ECRIS are discussed. It was observed that the low frequency oscillations below 200 Hz are distributed almost uniformly. In the high frequency oscillation “mode,” with frequencies >300 Hz at the core of the beam, carrying most of the current, oscillates with smaller amplitude than the peripheral parts of the beam. The result…

Physicsta114Oscillationbeam current oscillationsCyclotronElectric Conductivitytransverse distributionFaraday cupElectronsCyclotronsLower hybrid oscillationPlasma oscillationElectron cyclotron resonancelaw.inventionsymbols.namesakelawUpper hybrid oscillationsymbolsAtomic physicsInstrumentationBeam (structure)Review of Scientific Instruments
researchProduct

Nonlinear electrostatic oscillations in a cold magnetized electron-positron plasma

2017

We study the spatio-temporal evolution of the nonlinear electrostatic oscillations in a cold magnetized electron-positron (e-p) plasma using both analytics and simulations. Using a perturbative method we demonstrate that the nonlinear solutions change significantly when a pure electrostatic mode is excited at the linear level instead of a mixed upper-hybrid and zero-frequency mode that is considered in a recent study. The pure electrostatic oscillations undergo phase mixing nonlinearly. However, the presence of the magnetic field significantly delays the phase-mixing compared to that observed in the corresponding unmagnetized plasma. Using 1D PIC simulations we then analyze the damping of t…

[PHYS]Physics [physics]PhysicsFOS: Physical sciencesElectronPlasmaCondensed Matter PhysicsPlasma oscillationLower hybrid oscillation01 natural sciencesPhysics - Plasma Physics010305 fluids & plasmasMagnetic fieldPlasma Physics (physics.plasm-ph)Two-stream instabilityPhysics::Plasma Physics[PHYS.PHYS.PHYS-PLASM-PH]Physics [physics]/Physics [physics]/Plasma Physics [physics.plasm-ph]Upper hybrid oscillation0103 physical sciencesAstrophysical plasmaAtomic physics010306 general physicsComputingMilieux_MISCELLANEOUSPhysics of Plasmas
researchProduct