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相关论文: On Particle Transport and Radiation Production in …

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Plasmas with electromagnetic fields turbulent at sub-Larmor-scales are a feature of a wide variety of high-energy-density environments, and are essential to the description of many astrophysical/laboratory plasma phenomena. Radiation from…

等离子体物理 · 物理学 2015-09-16 Brett D. Keenan , Alexander L. Ford , Mikhail V. Medvedev

Radiative diagnostics of high-energy density plasmas is addressed in this paper. We propose that the radiation produced by energetic particles in small-scale magnetic field turbulence, which can occur in laser-plasma experiments,…

等离子体物理 · 物理学 2015-05-28 Sarah J. Reynolds , Mikhail V. Medvedev

Magnetized high-energy-density plasmas can often have strong electromagnetic fluctuations whose correlation scale is smaller than the electron Larmor radius. Radiation from the electrons in such plasmas, which markedly differs from both…

等离子体物理 · 物理学 2016-04-07 Brett D. Keenan , Mikhail V. Medvedev

Plasmas created by high-intensity lasers are often subject to the formation of kinetic-streaming instabilities, such as the Weibel instability, which lead to the spontaneous generation of high-amplitude, tangled magnetic fields. These…

等离子体物理 · 物理学 2015-11-24 Brett D. Keenan , Mikhail V. Medvedev

We calculate spectra of radiation produced by a relativistic particle in the presence of one-dimensional Langmuir turbulence which might be generated by a streaming instability in the plasma, in particular, in the shock front or at the…

天体物理学 · 物理学 2009-06-23 Gregory D. Fleishman , Igor N. Toptygin

The character of radiation of relativistic charged particles in strong magnetic fields largely depends on the disposition of particle trajectories relative to the field lines. The motion of particles with trajectories close to the curved…

高能天体物理现象 · 物理学 2015-01-23 Stanislav Kelner , Felix Aharonian

Spectrum of radiation of a relativistic particle moving in a nonhomogeneous magnetic field is considered. The spectrum depends on the pitch-angle $\alpha$ between the velocity direction and a line tangent to the field line. In case of very…

高能天体物理现象 · 物理学 2016-09-30 V. Epp , T. G. Mitrofanova

Test particle transport determined by the Lorentz force in turbulent magnetized plasmas is studied. The time dependent diffusion coefficient, valid for the whole range of parameters, is obtained by developing the decorrelation trajectory…

等离子体物理 · 物理学 2015-06-26 M. Vlad , F. Spineanu

The transport of high-energy particles in the presence of small-scale, turbulent magnetic fields is a long-standing issue in astrophysics. Analytical theories on transport perpendicular to the large-scale magnetic field disagree with…

高能天体物理现象 · 物理学 2025-10-03 Marco Kuhlen , Vo Hong Minh Phan , Philipp Mertsch

Synchrotron radiation detected from relativistic astrophysical objects such as pulsar-wind nebulae and {jets from active galactic nuclei} depends on the magnetic fields and the distribution functions of energetic electrons in these systems.…

星系天体物理 · 物理学 2026-03-04 Daniel Humphrey , Cristian Vega , Stanislav Boldyrev , Vadim Roytershteyn

Recently a new transport theory of cosmic rays in magnetized space plasmas extending the quasilinear approximation to the particle orbit has been developed for the case of an axisymmetric incompressible magnetic turbulence. Here we…

高能天体物理现象 · 物理学 2015-06-03 Sabrina Casanova , Reinhard Schlickeiser

High-amplitude, chaotic/turbulent electromagnetic fluctuations are ubiquitous in high-energy-density laboratory and astrophysical plasmas, where they can be excited by various kinetic-streaming and/or anisotropy-driven instabilities, such…

等离子体物理 · 物理学 2015-11-11 Brett D. Keenan , Alexander L. Ford , Mikhail V. Medvedev

The transport of charged particles in various astrophysical environments permeated by magnetic fields is described in terms of a diffusion process, which relies on diffusion-tensor parameters generally inferred from Monte-Carlo simulations.…

高能天体物理现象 · 物理学 2022-12-09 Olivier Deligny

The transport of charged particles in various astrophysical environments permeated by magnetic fields is described in terms of a diffusion process, which relies on diffusion-tensor parameters generally inferred from Monte-Carlo simulations.…

高能天体物理现象 · 物理学 2021-10-20 Olivier Deligny

The effects of resonant magnetic perturbations on the turbulent transport of fast ions in tokamak devices are investigated using a theoretical transport model of test-particle type. The direct numerical simulation method is used to compute,…

等离子体物理 · 物理学 2024-06-19 D. I. Palade

We present results from particle-in-cell simulations of driven turbulence in magnetized, collisionless, and relativistic pair plasma. We find that fluctuations are consistent with the classical $k_\perp^{-5/3}$ magnetic energy spectrum at…

等离子体物理 · 物理学 2017-02-14 Vladimir Zhdankin , Gregory R. Werner , Dmitri A. Uzdensky , Mitchell C. Begelman

The investigation of the diffusive transport of charged particles in a turbulent magnetic field remains a subject of considerable interest. Research has most frequently concentrated on determining the diffusion coefficient in the presence…

Various astrophysical studies have motivated the investigation of the transport of high energy particles in magnetic turbulence, either in the source or en route to the observation sites. For strong turbulence and large rigidity, the…

高能天体物理现象 · 物理学 2011-07-08 I. Plotnikov , G. Pelletier , M. Lemoine

The diffusions and anomalous diffusions of charged particles in the plateau regime of toroidal plasma with a Maxwellian velocity distribution are studied. The transport theory of plasma is discussed under the toroidal coordinate system and…

等离子体物理 · 物理学 2021-12-28 Wang Hong , Du Jiulin

Energetic particle transport in a finite amplitude magnetosonic and Alfvenic turbulence is considered using Monte Carlo particle simulations, which involve an integration of particle equation of motion. We show that in a low-Betha plasma…

天体物理学 · 物理学 2008-02-03 G. Michalek , M. Ostrowski , R. Schlickeiser
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