“…In contrast, the field of computational plasma physics has traditionally relied on hydrodynamics [5,6] and kinetic [7,8] codes because the temporal and spatial scales of interest are much too large for MD to be tractable; moreover, the detailed description of discrete particles is less important and instead macroscopic field variables are computed. However, MD plays a central role in a diverse set of plasma subfields concerned with understanding microscopic particles such as astrophysical systems [9,10], dusty plasmas [11,12], ultracold neutral plasmas [13,14], dense plasmas [15,16], low temperature plasmas [17,18], plasma beams [19,20], quark-gluon plasmas [21,22], etc.…”