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Theoretical physicists working at a blackboard collaboration pod in the Beecroft building.
Credit: Jack Hobhouse

Prof Michael Barnes

Professor in Theoretical Physics

Sub department

  • Rudolf Peierls Centre for Theoretical Physics

Research groups

  • Theoretical astrophysics and plasma physics at RPC
michael.barnes@physics.ox.ac.uk
Telephone: 01865 (2)73960
Rudolf Peierls Centre for Theoretical Physics, room 50.10
  • About
  • Publications

Bistable turbulence in strongly magnetised plasmas with a sheared mean flow

(2022)

Authors:

Nicolas Christen, Michael Barnes, Michael R Hardman, Alexander A Schekochihin
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Prevention of core particle depletion in stellarators by turbulence

(2022)

Authors:

H Thienpondt, JM García-Regaña, I Calvo, JA Alonso, JL Velasco, A González-Jerez, M Barnes, K Brunner, O Ford, G Fuchert, J Knauer, E Pasch, L Vanó, the Wendelstein 7-X team
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New linear stability parameter to describe low-$\beta$ electromagnetic microinstabilities driven by passing electrons in axisymmetric toroidal geometry

(2022)

Authors:

MR Hardman, FI Parra, BS Patel, CM Roach, J Ruiz Ruiz, M Barnes, D Dickinson, W Dorland, JF Parisi, D St-Onge, H Wilson
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A phase-shift-periodic parallel boundary condition for low-magnetic-shear scenarios

(2022)

Authors:

DA St-Onge, M Barnes, FI Parra
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Gyrokinetic electrostatic turbulence close to marginality in the Wendelstein 7-X stellarator

Physical Review E American Physical Society 106 (2022) L013202

Authors:

Alessandro Zocco, Linda Podavini, José Manuel Garcìa-Regaña, Michael Barnes, Felix I Parra, A Mishchenko, Per Helander

Abstract:

The transition from strong (fluidlike) to nearly marginal (Floquet-type) regimes of ion-temperature-gradient (ITG) driven turbulence is studied in the stellarator Wendelstein 7-X by means of numerical simulations. Close to marginality, extended (along magnetic field lines) linearly unstable modes are dominant, even in the presence of kinetic electrons, and provide a drive that results in finite turbulent transport. A total suppression of turbulence above the linear stability threshold of the ITG modes, commonly present in tokamaks and known as the “Dimits shift,” is not observed. We show that this is mostly due to the peculiar radial structure of marginal turbulence, which is more localized than in the fluid case and therefore less likely to be stabilized by shearing flows.
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