Interacting dust grains in complex plasmas: Ion wake formation and the electric potential

Author:

Vermillion K.1ORCID,Banka R.1ORCID,Mendoza A.1,Wyatt B.12ORCID,Matthews L.1ORCID,Hyde T.1ORCID

Affiliation:

1. Center for Astrophysics, Space Physics, and Engineering Research (CASPER), Baylor University 1 , Waco, Texas 76704, USA

2. Tarleton State University 2 , Stephenville, Texas 76401, USA

Abstract

Dust grains have been used as minimally invasive probes to determine plasma parameters including the plasma density, temperature, and electric field in a plasma discharge. However, the dust grains in a plasma generate local potential disturbances due to the collection of charge and the subsequent electrostatic interactions between the dust and charged plasma particles. Dust grains in close proximity to one another exhibit interesting non-reciprocal interactions and self-organize into structures such as one-dimensional filamentary chains, two-dimensional “zigzags,” and three-dimensional helices, among others. The formation of these structures suggests that although the dust grains may be less invasive than traditional plasma probes, the disturbance to the local plasma environment introduced by dust grains is non-trivial. Commonly used analytic forms of the electric potential describing complex plasmas have failed to resolve the near-dust region, and as a result are insufficient to provide insight about the formation of complex dust structures. Here, we use an N-body simulation to compute the electric potential from ion densities near various dust grain configurations. We provide an alternative description to the standard analytic model for the electric potential of dust and ion wakes based on a Gaussian shaped cloud of ions. The electric potential obtained from simulations is used to identify minimum energy configurations for two and three dust grains. It is further demonstrated that the minimum potential region identified for N dust grains and their associated ion wakes does not predict the minimum-energy configuration of N + 1 dust grains.

Funder

Division of Physics

Office of Science

Nvidia

Publisher

AIP Publishing

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