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Quantifying Energy Conversion in Higher Order Phase Space Density Moments in Plasmas (2306.01106v1)

Published 1 Jun 2023 in physics.plasm-ph, astro-ph.GA, physics.chem-ph, physics.flu-dyn, and physics.space-ph

Abstract: Weakly collisional and collisionless plasmas are typically far from local thermodynamic equilibrium (LTE), and understanding energy conversion in such systems is a forefront research problem. The standard approach is to investigate changes in internal (thermal) energy and density, but this omits energy conversion that changes any higher order moments of the phase space density. In this study, we calculate from first principles the energy conversion associated with all higher moments of the phase space density for systems not in LTE. Particle-in-cell simulations of collisionless magnetic reconnection reveal that energy conversion associated with higher order moments can be locally significant. The results may be useful in numerous plasma settings, such as reconnection, turbulence, shocks, and wave-particle interactions in heliospheric, planetary, and astrophysical plasmas.

Citations (10)

Summary

  • The paper presents a first-principles approach quantifying energy conversion via higher-order phase space density moments, expanding beyond traditional density and internal energy views in non-equilibrium plasmas.
  • Using particle-in-cell simulations of magnetic reconnection, the study demonstrates that energy conversion related to higher moments significantly influences local plasma dynamics.
  • This research provides a refined framework for understanding energy conversion in non-LTE plasma systems, with implications for space physics, astrophysics, turbulence modeling, and bridging fluid and kinetic scales.

Quantifying Energy Conversion in Higher Order Phase Space Density Moments in Plasmas

This paper presents a first-principles approach to understanding energy conversion in weakly collisional and collisionless plasmas, systems inherently far from local thermodynamic equilibrium (LTE). Traditional models focus on changes in internal energy and density, but this paper aims to expand that view by including energy conversion associated with higher order moments of the phase space density.

Summary of Key Concepts

The concept of phase space density is critical in plasma physics, reflecting a system's particle distribution across position and velocity. For non-LTE systems, characterizing energy conversion solely by changes in density and internal (thermal) energy is insufficient. Internal moments, defined by multiplying phase space density by powers of velocity components and integrating over all velocities, offer a more comprehensive description.

In systems with weak or no collisions, conventional treatment examines the zero and second order moments representing density and internal energy, respectively. Changes in these variables relate to phenomena like compressional work and heating through pressure-strain interactions. The authors, however, calculate energy conversion across higher order moments, making it central to understanding complex plasma dynamics like shocks and turbulence.

Methodology and Numerical Findings

Using particle-in-cell (PIC) simulations focused on collisionless magnetic reconnection, the research highlights that energy conversion related to higher order phase space moments can have significant local influences. The analysis rests on kinetic entropy and its decomposition into position and velocity space entropy, alongside concepts of relative entropy drawn from information theory.

Numerical Simulation Details:

  • The authors employed a PIC simulation with a grid size and resolution tailored to capture the intricate motion and behavior in a reconnection region—domains where magnetic fields realign, often resulting in particle acceleration.
  • They observed that while internal energy changes (linked to heating) are critical, shifts in relative energy are equally vital, as they reflect the evolution towards or away from equilibrium, thus influencing the higher order moments.

Implications and Future Developments

This research underscores the importance of considering energy conversion effects beyond traditional thermodynamic quantities, suggesting a framework more aligned with kinetic theory for non-equilibrium systems. The implications span not just space and astrophysical plasmas, but also turbulence modeling, including kinetic effects in current fluid models.

Future Directions:

  • The relationship between non-LTE behavior and kinetic entropy provides a fertile ground for development, especially through employing machine learning to identify patterns or streamline their modeling in comprehensive fluid dynamics scenarios.
  • Expanding this framework to incorporate varying entropic measures or aligning with quantum statistical approaches could offer new insights, especially in extreme environments like black hole accretion disks or relativistic jets, where plasma processes are pivotal.

Comparison with Current Literature

The paper contends with linear theories within kinetic and gyrokinetic frameworks, establishing that the linearized models align with, but do not extend as comprehensively as the presented kinetic first law, which encompasses all internal moments. Their methodology reflects a significant leap over perturbative models, promising a more precise energetic accounting in far-from-equilibrium settings.

Relation to Previous Works:

  • This work aligns with the ongoing exploration of field-particle correlations, where understanding how electromagnetic fields influence particle dynamics remains crucial.
  • Moreover, the energy conversion pathways envisioned could bridge current fluid dynamic models and kinetic scale physics comprehensively, enabling holistic multi-scale simulations.

In conclusion, this paper widens our lens on energy conversion processes in plasmas, particularly under non-LTE conditions, pushing the boundaries of both theoretical understanding and practical application in plasma physics and related fields.

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