• Featured in Physics
  • Editors' Suggestion
  • Open Access

Characterization of Quasi-Keplerian, Differentially Rotating, Free-Boundary Laboratory Plasmas

V. Valenzuela-Villaseca, L. G. Suttle, F. Suzuki-Vidal, J. W. D. Halliday, S. Merlini, D. R. Russell, E. R. Tubman, J. D. Hare, J. P. Chittenden, M. E. Koepke, E. G. Blackman, and S. V. Lebedev
Phys. Rev. Lett. 130, 195101 – Published 12 May 2023
Physics logo See Focus story: A Lab Plasma Rotates and Produces Jets

Abstract

We present results from pulsed-power driven differentially rotating plasma experiments designed to simulate physics relevant to astrophysical disks and jets. In these experiments, angular momentum is injected by the ram pressure of the ablation flows from a wire array Z pinch. In contrast to previous liquid metal and plasma experiments, rotation is not driven by boundary forces. Axial pressure gradients launch a rotating plasma jet upward, which is confined by a combination of ram, thermal, and magnetic pressure of a surrounding plasma halo. The jet has subsonic rotation, with a maximum rotation velocity 23±3km/s. The rotational velocity profile is quasi-Keplerian with a positive Rayleigh discriminant κ2r2.8±0.8rad2/s2. The plasma completes 0.5–2 full rotations in the experimental time frame (150ns).

  • Figure
  • Figure
  • Figure
  • Figure
  • Received 22 December 2021
  • Accepted 29 March 2023

DOI:https://doi.org/10.1103/PhysRevLett.130.195101

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Plasma Physics

Focus

Key Image

A Lab Plasma Rotates and Produces Jets

Published 12 May 2023

A spinning plasma ring mimics the rotating structure surrounding a black hole.

See more in Physics

Authors & Affiliations

V. Valenzuela-Villaseca1,*,†, L. G. Suttle1, F. Suzuki-Vidal1,‡, J. W. D. Halliday1, S. Merlini1, D. R. Russell1, E. R. Tubman1,∥, J. D. Hare1,§, J. P. Chittenden1, M. E. Koepke2, E. G. Blackman3, and S. V. Lebedev1

  • 1Blackett Laboratory, Imperial College London, London SW7 2BW, United Kingdom
  • 2Department of Physics, West Virginia University, Morgantown, West Virginia 26506, USA
  • 3Department of Physics and Astronomy, University of Rochester, Rochester, New York 14627, USA

  • *vv5425@princeton.edu
  • Current address: Department of Astrophysical Sciences, Princeton University, Princeton, New Jersey 08544, USA.
  • Current address: First Light Fusion Ltd., Yarnton, Kidlington OX5 1QU, United Kingdom.
  • Current address: Lawrence Livermore National Laboratory, Livermore, California 94550, USA.
  • §Current address: Plasma Science and Fusion Center, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA.

Article Text

Click to Expand

References

Click to Expand
Issue

Vol. 130, Iss. 19 — 12 May 2023

Reuse & Permissions
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review Letters

Reuse & Permissions

It is not necessary to obtain permission to reuse this article or its components as it is available under the terms of the Creative Commons Attribution 4.0 International license. This license permits unrestricted use, distribution, and reproduction in any medium, provided attribution to the author(s) and the published article's title, journal citation, and DOI are maintained. Please note that some figures may have been included with permission from other third parties. It is your responsibility to obtain the proper permission from the rights holder directly for these figures.

×

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×