English

Bridging the gap between collisional and collisionless shock waves

Plasma Physics 2021-07-01 v1 High Energy Astrophysical Phenomena Solar and Stellar Astrophysics Space Physics

Abstract

While the front of a fluid shock is a few mean-free-paths thick, the front of a collisionless shock can be orders of magnitude thinner. By bridging between a collisional and a collisionless formalism, we assess the transition between these two regimes. We consider non-relativistic, un-magnetized, planar shocks in electron/ion plasmas. In addition, our treatment of the collisionless regime is restricted to high Mach number electrostatic shocks. We find that the transition can be parameterized by the upstream plasma parameter Λ\Lambda which measures the coupling of the upstream medium. For Λ1.12\Lambda \lesssim 1.12, the upstream is collisional, i.e. strongly coupled, and the strong shock front is about M1λmfp,1\mathcal{M}_1 \lambda_{\mathrm{mfp},1} thick, where λmfp,1\lambda_{\mathrm{mfp},1} and M1\mathcal{M}_1 are the upstream mean-free-path and Mach number respectively. A transition occurs for Λ1.12\Lambda \sim 1.12 beyond which the front is M1λmfp,1lnΛ/Λ\sim \mathcal{M}_1\lambda_{\mathrm{mfp},1}\ln \Lambda/\Lambda thick for Λ1.12\Lambda\gtrsim 1.12. Considering Λ\Lambda can reach billions in astrophysical settings, this allows to understand how the front of a collisionless shock can be orders of magnitude smaller than the mean-free-path, and how physics transitions continuously between these 2 extremes.

Keywords

Cite

@article{arxiv.2101.09130,
  title  = {Bridging the gap between collisional and collisionless shock waves},
  author = {Antoine Bret and Asaf Pe'er},
  journal= {arXiv preprint arXiv:2101.09130},
  year   = {2021}
}

Comments

13 pages, 4 figures, Under consideration for publication in J. Plasma Phys

R2 v1 2026-06-23T22:25:31.672Z