English

Pressure-Strain Interaction: I. On Compression, Deformation, and Implications For Pi-D

Plasma Physics 2023-01-04 v1 Fluid Dynamics Space Physics

Abstract

The pressure-strain interaction describes the rate per unit volume that energy is converted between bulk flow and thermal energy in neutral fluids or plasmas. The term has been written as a sum of the pressure dilatation and the collisionless analogue of viscous heating referred to as PiD{\rm Pi-D}, which isolates the power density due to compressible and incompressible effects, respectively. It has been shown that PiD{\rm Pi-D} can be negative, which makes its identification as collisionless viscous heating troubling. We argue that an alternate decomposition of pressure-strain interaction can be useful for interpreting the underlying physics. Since PiD{\rm Pi-D} contains both normal deformation and shear deformation, we propose grouping the normal deformation with the pressure dilatation to describe the power density due to converging/diverging flows, with the balance describing the power density purely due to shear deformation. We then develop a kinetic theory interpretation of compression, normal deformation, and shear deformation. We use the results to determine the physical mechanisms that can make PiD{\rm Pi-D} negative. We argue that both decompositions can be useful for the study of energy conversion in weakly collisional or collisionless fluids and plasmas, and implications are discussed.

Keywords

Cite

@article{arxiv.2211.13160,
  title  = {Pressure-Strain Interaction: I. On Compression, Deformation, and Implications For Pi-D},
  author = {Paul A. Cassak and M. Hasan Barbhuiya},
  journal= {arXiv preprint arXiv:2211.13160},
  year   = {2023}
}

Comments

16 pages, 4 figures, accepted to Physics of Plasmas

R2 v1 2026-06-28T06:42:04.586Z