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Numerical simulations of a continuously injected relativistic electron beam relaxation into a plasma with large-scale density gradients

Published 14 Aug 2022 in physics.plasm-ph and astro-ph.SR | (2208.06786v2)

Abstract: In this paper the influence of large-scale decreasing and increasing gradients of the density of magnetized plasma on the relaxation process of a continuously injected relativistic electron beam with an energy of 611 keV ($v_b=0.9c$) and a pitch-angle distribution is studied using particle-in-cell numerical simulations. It is found that for the selected parameters in the case of a smoothly decreasing gradient and in a homogeneous plasma the formation of spatially limited plasma oscillations of large amplitude occurs. In such cases, modulation instability develops and a long-wave longitudinal modulation of the ion density is formed. In addition, the large amplitude of plasma waves accelerates plasma electrons to energies on the order of the beam energy. In the case of increasing and sharply decreasing gradients, a significant decrease in the amplitude of plasma oscillations and the formation of a turbulent ion density spectrum are observed. The possibility of acceleration of beam electrons to energies more than 2 times higher than the initial energy of the beam particles is also demonstrated. This process takes place not only during beam propagation in growing plasma density, but also in homogeneous plasma due to interaction of beam particles with plasma oscillations of large amplitude.

Citations (2)

Summary

  • The paper reveals that large-scale density gradients critically influence electron beam relaxation, driving plasma oscillations and ion density modulations.
  • It employs advanced PIC simulations to capture both linear and nonlinear beam-plasma interactions in magnetized environments.
  • Findings indicate that density gradients can either enhance electron acceleration through plasma waves or suppress beam-plasma instabilities, with implications for astrophysical and laboratory studies.

Numerical Simulations of Relativistic Electron Beam Relaxation in Plasmas with Density Gradients

The paper presents a comprehensive study using particle-in-cell (PIC) simulations to examine the relaxation processes of a continuously injected relativistic electron beam into a magnetized plasma with large-scale density gradients. The focus is on how these density gradients—both increasing and decreasing—influence the beam relaxation and related phenomena such as plasma oscillations, particle acceleration, and ion density modulation.

The exploration is critical in numerous domains like space physics and controlled laboratory plasma experiments. The PIC simulations are implemented with a detailed numerical model capable of handling the multi-scale and multi-physics nature of the problem, effectively considering the linear and nonlinear interactions between the beam and plasma.

Key Findings

  • Beam Relaxation Dynamics: In both homogeneous plasmas and those with decreasing density gradients, a localized packet of large-amplitude plasma oscillations is formed. These oscillations further develop modulation instability, leading to long-wave ion density variations. Such density modulations can trap plasma waves, which might eventually excite electromagnetic radiation at harmonics of the plasma frequency.
  • Acceleration Mechanisms: Remarkably, the large-amplitude plasma waves can accelerate plasma electrons to energies comparable to or exceeding the initial beam energy. This outcome is consistent across both uniform plasma cases and those with decreasing gradient profiles.
  • Suppression and Stimulation of Instability: With increasing density gradients, an observed suppression of beam-plasma instability occurs, suggesting a complex dependence where the gradient strength can dampen or amplify instabilities based on its direction relative to beam propagation.
  • Numerical Discrepancies: The study discusses how conditions, such as density gradients and geometry, influence beam relaxation patterns compared to predictions from linear instability theory, showcasing the limitations of existing analytical models when applied to real-world conditions.

Implications

The research provides valuable insights into the interaction of high-energy particle streams with plasmas, as seen in various astrophysical and laboratory settings. For instance, in space physics, understanding such interactions enhances the modeling of solar flares or cosmic jets. In laboratory plasmas, this knowledge aids the development of advanced radiative sources and improves confinement regimes in magnetic traps.

Future Directions

The study opens pathways for further research on the complexity of plasma wave dynamics in more realistic multi-dimensional setups. Investigating different parameters like the beam's energy distribution and pitch-angle would deepen the understanding of these complex interactions. Furthermore, extending the simulations to include additional physical processes, like collisional effects or more intricate magnetic field configurations, could prove pivotal in bridging theoretical predictions with observational data.

In conclusion, the findings from this study present a vital step towards unraveling the complex dynamics of beam-plasma interaction in inhomogeneous environments and underscore the potential for further inquiry into nonlinear plasma phenomena. The comprehensive use of PIC simulations provides a robust framework not only for understanding current phenomena but also for exploring new physics regimes in plasma research.

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