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Phys. Rev. Lett. 95, 068001 (2005) [4 pages]

Velocity Distributions of Granular Gases with Drag and with Long-Range Interactions

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K. Kohlstedt1,2, A. Snezhko1, M. V. Sapozhnikov1,3, I. S. Aranson1, J. S. Olafsen2, and E. Ben-Naim4
1Argonne National Laboratory, 9700 South Cass Avenue, Argonne, Illinois 60439, USA
2Department of Physics and Astronomy, University of Kansas, Lawrence, Kansas 66045, USA
3Institute for Physics of Microstructures, Russian Academy of Sciences, GSP-105, Nizhny Novgorod 603600, Russia
4Theoretical Division and Center for Nonlinear Studies, Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA

Received 23 November 2004; revised 17 March 2005; published 1 August 2005

We study velocity statistics of electrostatically driven granular gases. For two different experiments, (i) nonmagnetic particles in a viscous fluid and (ii) magnetic particles in air, the velocity distribution is non-Maxwellian, and its high-energy tail is exponential, P(v)∼exp⁡(-|v|). This behavior is consistent with the kinetic theory of driven dissipative particles. For particles immersed in a fluid, viscous damping is responsible for the exponential tail, while for magnetic particles, long-range interactions cause the exponential tail. We conclude that velocity statistics of dissipative gases are sensitive to the fluid environment and to the form of the particle interaction.

© 2005 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevLett.95.068001
DOI:
10.1103/PhysRevLett.95.068001
PACS:
45.70.−n, 47.70.Nd, 81.05.Rm