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Runko: Modern multiphysics toolbox for plasma simulations

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arxiv 1906.06306 v3 pith:KMMWEN3S submitted 2019-06-14 physics.comp-ph astro-ph.IMphysics.plasm-ph

classification physics.comp-phastro-ph.IMphysics.plasm-ph
keywords simulationsframeworkplasmarelativisticcodedesigndifferentmodern
verification ladder T0 review T1 audit T2 compute T3 formal
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Runko is a new open-source plasma simulation framework implemented in C++ and Python. It is designed to function as an easy-to-extend general toolbox for simulating astrophysical plasmas with different theoretical and numerical models. Computationally intensive low-level kernels are written in modern C++ taking advantage of polymorphic classes, multiple inheritance, and template metaprogramming. High-level functionality is operated with Python scripts. The hybrid program design ensures good code performance together with ease of use. The framework has a modular object-oriented design that allows the user to easily add new numerical algorithms to the system. The code can be run on various computing platforms ranging from laptops (shared-memory systems) to massively parallel supercomputer architectures (distributed-memory systems). The framework supports heterogeneous multiphysics simulations in which different physical solvers can be combined and run simultaneously. Here we showcase the framework's relativistic particle-in-cell (PIC) module by presenting (i) 1D simulations of relativistic Weibel instability, (ii) 2D simulations of relativistic kinetic turbulence in a suddenly stirred magnetically-dominated pair plasma, and (iii) 3D simulations of collisionless shocks in an unmagnetized medium.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Kinetic turbulence in shining pair plasma: intermittent beaming and thermalization by radiative cooling

    astro-ph.HE 2019-08 conditional novelty 7.0 of 10

    Adding inverse-Compton cooling to driven relativistic pair-plasma turbulence makes the steady-state particle energy distribution nearly Maxwellian and produces intermittent, reconnection-associated particle beams at h...

  2. The interplay of magnetically-dominated turbulence and magnetic reconnection in producing nonthermal particles

    astro-ph.HE 2019-09 conditional novelty 6.0 of 10

    In relativistic pair-plasma turbulence, particles are first injected by parallel electric fields at plasmoid-mediated reconnecting current sheets, then accelerated stochastically by perpendicular electric fields, yiel...

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