Magnetically driven granular gas in low gravity

ORAL

Abstract

Experimental investigation of granular gas systems in three dimensions desire the removal of the weight of constituent particles. In a sounding rocket experiment module, such condition is realized and maintained for 6 minutes, allowing 4 rounds of particle excitation and cooling. Varying magnetic force from 8 magnets surrounding the sample cell is adopted as the bulk-driving mechanism to enable a homogeneous spatial distribution of around 3000 particles. Soft ferromagnetic particles are chosen to minimize the long-range interactions between particles once the excitation finishes. The ensuing cooling behavior is thus mainly governed by energy-dissipative particle collisions and the kinetic theory of granular gases becomes comparable with the experimental results. From such comparisons, the prediction of non-Maxwellian velocity distribution is confirmed, while the Haff's cooling law, although qualitatively verified, quantitatively overestimates the cooling time scale significantly.

*We acknowledge partial funding from BMWi/DLR through Projects No. 50WM1651 and 50WM1945 for the experimental work. We acknowledge JSPS Overseas Research Fellowships and Alexander von Humboldt Research Fellowship for the simulation work.

Publication: https://doi.org/10.1063/1.5085319
https://doi.org/10.1103/PhysRevLett.124.208007
https://doi.org/10.1038/s41526-019-0079-y

Presenters

  • Peidong Yu

    • German Aerospace Center (DLR)

Authors

  • Peidong Yu

    • German Aerospace Center (DLR)
  • Matthias Sperl

    • German Aerospace Center
  • Matthias Schroeter

    • Max Planck Institute for Dynamics and Se
  • Masato Adachi

    • German Aerospace Center