Apar-T: code, validation, and physical interpretation of particle-in-cell results
arXiv:1308.5892 · doi:10.1051/0004-6361/201321557
Abstract
We present the parallel particle-in-cell (PIC) code Apar-T and, more importantly, address the fundamental question of the relations between the PIC model, the Vlasov-Maxwell theory, and real plasmas. First, we present four validation tests: spectra from simulations of thermal plasmas, linear growth rates of the relativistic tearing instability and of the filamentation instability, and non-linear filamentation merging phase. For the filamentation instability we show that the effective growth rates measured on the total energy can differ by more than 50% from the linear cold predictions and from the fastest modes of the simulation. Second, we detail a new method for initial loading of Maxwell-Jüttner particle distributions with relativistic bulk velocity and relativistic temperature, and explain why the traditional method with individual particle boosting fails. Third, we scrutinize the question of what description of physical plasmas is obtained by PIC models. These models rely on two building blocks: coarse-graining, i.e., grouping of the order of p~10^10 real particles into a single computer superparticle, and field storage on a grid with its subsequent finite superparticle size. We introduce the notion of coarse-graining dependent quantities, i.e., quantities depending on p. They derive from the PIC plasma parameter Lambda^{PIC}, which we show to scale as 1/p. We explore two implications. One is that PIC collision- and fluctuation-induced thermalization times are expected to scale with the number of superparticles per grid cell, and thus to be a factor p~10^10 smaller than in real plasmas. The other is that the level of electric field fluctuations scales as 1/Lambda^{PIC} ~ p. We provide a corresponding exact expression. Fourth, we compare the Vlasov-Maxwell theory, which describes a phase-space fluid with infinite Lambda, to the PIC model and its relatively small Lambda.
24 pages, 14 figures, accepted in Astronomy & Astrophysics
References in corpus (12)
- Simulations of particle acceleration beyond the classical synchrotron burnoff limit in magnetic reconnection: An explanation of the Crab flares
- Relativistic Brownian Motion
- One-to-one direct modeling of experiments and astrophysical scenarios: pushing the envelope on kinetic plasma simulations
- The Role of the Guide Field in Relativistic Pair Plasma Reconnection
- Thermal equilibrium and statistical thermometers in special relativity
- Collisionless shock formation, spontaneous electromagnetic fluctuations and streaming instabilities
- Apar-T: code, validation, and physical interpretation of particle-in-cell results
- Photon-Plasma: a modern high-order particle-in-cell code
- Growth rates of the Weibel and tearing mode instabilities in a relativistic pair plasma
- Particle-In-Cell Simulation of Electron Acceleration in Solar Coronal Jets
- The Generation of Random Variates From a Relativistic Maxwellian Distribution
- Particle Acceleration, Magnetic Field Generation, and Associated Emission in Collisionless Relativistic Jets
Cited by in corpus (33)
- Relativistic magnetic reconnection in pair plasmas and its astrophysical applications
- Electron and proton heating in trans-relativistic magnetic reconnection
- Electron Heating by the Ion Cyclotron Instability in Collisionless Accretion Flows. I. Compression-Driven Instabilities and the Electron Heating Mechanism
- Relativistic magnetic reconnection in collisionless ion-electron plasmas explored with particle-in-cell simulations
- Electron Weibel Instability in Relativistic Counter-Streaming Plasmas with Flow-Aligned External Magnetic Fields
- Apar-T: code, validation, and physical interpretation of particle-in-cell results
- The energetics of relativistic magnetic reconnection: ion-electron repartition and particle distribution hardness
- PIC methods in astrophysics: Simulations of relativistic jets and kinetic physics in astrophysical systems
- On the Growth and Saturation of the Gyroresonant Streaming Instabilities
- Loading Relativistic Maxwell Distributions in Particle Simulations
- Hard particle spectra of galactic X-ray sources by relativistic magnetic reconnection in laser lab
- Bright gamma-ray flares powered by magnetic reconnection in QED-strength magnetic fields
- Electron Heating by the Ion Cyclotron Instability in Collisionless Accretion Flows. II. Electron Heating Efficiency as a Function of Flow Conditions
- Non-Maxwellian electron distribution functions due to self-generated turbulence in collisionless guide-field reconnection
- Comptonization by Reconnection Plasmoids in Black Hole Coronae II: Electron-Ion Plasma
- A new hybrid code (CHIEF) implementing the inertial electron fluid equation without approximation
- High-energy synchrotron flares powered by strongly radiative relativistic magnetic reconnection: 2D and 3D PIC simulations
- Fully kinetic large scale simulations of the collisionless Magnetorotational instability
- An fully implicit scheme for numerical integration of the relativistic particle equation of motion
- Electron Preacceleration at Weak Quasi-perpendicular Intracluster Shocks: Effects of Preexisting Nonthermal Electrons
- An asymptotic preserving scheme for the relativistic Vlasov--Maxwell equations in the classical limit
- Supersonic turbulence in 3D isothermal flow collision
- Instabilities of collisionless current sheets revisited: the role of anisotropic heating
- Turbulent transport in 2D collisionless guide field reconnection
- A well-balanced scheme for the simulation tool-kit A-MaZe: implementation, tests, and first applications to stellar structure
- Wave emission of non-thermal electron beams generated by magnetic reconnection
- Transport of relativistic jet in the magnetized intergalactic medium
- Simulations of multicomponent relativistic thermalization
- Particle-in-Cell Simulations of Relativistic Magnetic Reconnection with Advanced Maxwell Solver Algorithms
- Differences between real and particle-in-cell plasmas: effects of coarse-graining
- The baryon loading effect on relativistic astrophysical jet transport in the interstellar medium
- Analytical treatment of particle motion in circularly polarized slab-mode wave fields
- Effects of radiative losses on the relativistic jets of high-mass microquasars