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AHKASH: a new Hybrid particle-in-cell code for simulations of astrophysical collisionless plasma.

Authors :
Achikanath Chirakkara, Radhika
Federrath, Christoph
Seta, Amit
Source :
Monthly Notices of the Royal Astronomical Society; Nov2024, Vol. 534 Issue 4, p3761-3782, 22p
Publication Year :
2024

Abstract

We introduce A strophysical H ybrid- K inetic simulations with the flash code (⁠|$\tt {AHKASH}$|⁠) – a new Hybrid particle-in-cell (PIC) code developed within the framework of the multiphysics code flash. The new code uses a second-order accurate Boris integrator and a predictor–predictor–corrector algorithm for advancing the Hybrid-kinetic equations, using the constraint transport method to ensure that magnetic fields are divergence-free. The code supports various interpolation schemes between the particles and grid cells, with post-interpolation smoothing to reduce finite particle noise. We further implement a |$\delta f$| method to study instabilities in weakly collisional plasmas. The new code is tested on standard physical problems such as the motion of charged particles in uniform and spatially varying magnetic fields, the propagation of Alfvén and whistler waves, and Landau damping of ion acoustic waves. We test different interpolation kernels and demonstrate the necessity of performing post-interpolation smoothing. We couple the turbgen turbulence driving module to the new Hybrid PIC code, allowing us to test the code on the highly complex physical problem of the turbulent dynamo. To investigate steady-state turbulence with a fixed sonic Mach number, it is important to maintain isothermal plasma conditions. Therefore, we introduce a novel cooling method for Hybrid PIC codes and provide tests and calibrations of this method to keep the plasma isothermal. We describe and test the 'hybrid precision' method, which significantly reduces (by a factor |$\sim 1.5$|⁠) the computational cost, without compromising the accuracy of the numerical solutions. Finally, we test the parallel scalability of the new code, showing excellent scaling up to 10,000 cores. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
00358711
Volume :
534
Issue :
4
Database :
Complementary Index
Journal :
Monthly Notices of the Royal Astronomical Society
Publication Type :
Academic Journal
Accession number :
180738337
Full Text :
https://doi.org/10.1093/mnras/stae2188