Kinetic simulation of magnetic field generation and collisionless shock formation in expanding laboratory plasmas

Fox, W.; Matteucci, J.; Moissard, C.; Schaeffer, D. B.; Bhattacharjee, A.; Germaschewski, K.; Hu, S. X.

doi:10.1063/1.5050813

Title: Kinetic simulation of magnetic field generation and collisionless shock formation in expanding laboratory plasmas

Journal Article · Mon Oct 08 00:00:00 EDT 2018 · Physics of Plasmas

DOI:https://doi.org/10.1063/1.5050813· OSTI ID:1476877

^[1]; Matteucci, J. ^[2];

^[3]; Schaeffer, D. B. ^[2]; Bhattacharjee, A. ^[1];

^[4];

^[5]

Princeton Plasma Physics Lab. (PPPL), Princeton, NJ (United States); Princeton Univ., Princeton, NJ (United States)
Princeton Univ., Princeton, NJ (United States)
Ecole Polytechnique, Palaiseau (France)
Univ. of New Hampshire, Durham, NH (United States)
Univ. of Rochester, Rochester, NY (United States)

Recent laboratory experiments with laser-produced plasmas have observed and studied a number of fundamental physical processes relevant to magnetized astrophysical plasmas, including magnetic reconnection, collisionless shocks, and magnetic field generation by Weibel instability, opening up new experimental platforms for laboratory astrophysics. We develop a fully kinetic simulation model for first-principles simulation of these systems including the dynamics of magnetic fields—magnetic field generation by the Biermann battery effect or Weibel instability; advection by the ion flow, Hall effect, and Nernst effect; and destruction of the field by dissipative mechanisms. Key dimensionless parameters describing the system are derived for scaling between kinetic simulation, recent experiments, and astrophysical plasmas. First, simulations are presented which model Biermann battery magnetic field generation in plasmas expanding from a thin target. Ablation of two neighboring plumes leads to the formation of a current sheet as the opposing Biermann-generated fields collide, modeling recent laser-driven magnetic reconnection experiments. Second, we simulate recent experiments on collisionless magnetized shock generation, by expanding a piston plasma into a pre-magnetized ambient plasma. For parameters considered, the Biermann effect generates additional magnetic fields in the curved shock front and thereby increases shock particle reflection. In conclusion, both cases show the importance of kinetic processes in the interaction of plasmas with magnetic fields and open opportunities to benchmark these important processes through comparison of theory and experiments.

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Research Organization:: Oak Ridge National Laboratory (ORNL), Oak Ridge, TN (United States). Oak Ridge Leadership Computing Facility (OLCF); Princeton Plasma Physics Laboratory (PPPL), Princeton, NJ (United States)

Sponsoring Organization:: USDOE Office of Science (SC)

Grant/Contract Number:: AC05-00OR22725; SC0008655; SC0016249

OSTI ID:: 1476877

Alternate ID(s):: OSTI ID: 1476680

Journal Information:: Physics of Plasmas, Vol. 25, Issue 10; ISSN 1070-664X

Publisher:: American Institute of Physics (AIP)Copyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 24 works

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