Discovery of double Hall pattern associated with collisionless magnetic reconnection in dusty plasmas

Author:

Yang Shu-Di1,Wang Liang2,Dong Chuanfei23ORCID

Affiliation:

1. School of Physics, Peking University , Beijing 100871, China

2. Princeton Plasma Physics Laboratory and Department of Astrophysical Sciences, Princeton University , Princeton, NJ 08540, USA

3. Department of Astronomy, Boston University , Boston, MA 02215, USA

Abstract

ABSTRACT Magnetic reconnection is prevalent in magnetized plasmas in space and laboratories. Despite significant investigations on reconnection in electron–ion plasmas, studies of reconnection in magnetized plasmas with negatively charged dust grains are quite sparse. Here, we report the first fully kinetic simulations of collisionless reconnection in a three-species (i.e. electron, proton, and negatively charged dust grain) dusty plasma, through which the discovery of double Hall pattern is made. The double Hall pattern consists of a traditional Hall quadruple current in between the ion and electron diffusion region and a reversed Hall current in between the boundary of the ion and dust diffusion region. The analysis of the reconnection rate is also given. This study may be applicable to explain observations of planetary magnetospheres and the astrophysical objects, and may be realized in the laboratory studies of dusty plasmas.

Funder

U.S. Department of Energy

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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