Pressure-Strain Interaction: I. On Compression, Deformation, and Implications For Pi-D
Paul A. Cassak, M. Hasan Barbhuiya

TL;DR
This paper explores the pressure-strain interaction in plasmas, proposing an alternative decomposition to better interpret energy conversion processes, especially in collisionless conditions, and examines the physical mechanisms behind negative Pi-D values.
Contribution
It introduces a new decomposition of pressure-strain interaction separating normal and shear deformation effects, enhancing understanding of energy transfer in collisionless plasmas.
Findings
Proposes grouping pressure dilatation with normal deformation for better physical interpretation.
Develops a kinetic theory framework for compression, normal, and shear deformation.
Identifies mechanisms leading to negative Pi-D in weakly collisional plasmas.
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 , which isolates the power density due to compressible and incompressible effects, respectively. It has been shown that 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 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…
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Taxonomy
TopicsSolar and Space Plasma Dynamics
