Skip to main content
Home
Department Of Physics text logo
  • Research
    • Our research
    • Our research groups
    • Our research in action
    • Research funding support
    • Summer internships for undergraduates
  • Study
    • Undergraduates
    • Postgraduates
  • Engage
    • For alumni
    • For business
    • For schools
    • For the public
Menu
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

Extended electron tails in electrostatic microinstabilities and the nonadiabatic response of passing electrons

Plasma Physics and Controlled Fusion IOP Publishing 64:5 (2022) 055004

Authors:

Mr Hardman, Fi Parra, C Chong, T Adkins, Ms Anastopoulos-Tzanis, M Barnes, D Dickinson, Jf Parisi, H Wilson

Abstract:

Ion-gyroradius-scale microinstabilities typically have a frequency comparable to the ion transit frequency. Due to the small electron-to-ion mass ratio and the large electron transit frequency, it is conventionally assumed that passing electrons respond adiabatically in ion-gyroradius-scale modes. However, in gyrokinetic simulations of ion-gyroradius-scale modes in axisymmetric toroidal magnetic fields, the nonadiabatic response of passing electrons can drive the mode, and generate fluctuations in narrow radial layers, which may have consequences for turbulent transport in a variety of circumstances. In flux tube simulations, in the ballooning representation, these instabilities reveal themselves as modes with extended tails. The small electron-to-ion mass ratio limit of linear gyrokinetics for electrostatic instabilities is presented, in axisymmetric toroidal magnetic geometry, including the nonadiabatic response of passing electrons and associated narrow radial layers. This theory reveals the existence of ion-gyroradius-scale modes driven solely by the nonadiabatic passing electron response, and recovers the usual ion-gyroradius-scale modes driven by the response of ions and trapped electrons, where the nonadiabatic response of passing electrons is small. The collisionless and collisional limits of the theory are considered, demonstrating parallels in structure and physical processes to neoclassical transport theory. By examining initial-value simulations of the fastest-growing eigenmodes, the predictions for mass-ratio scaling are tested and verified numerically for a range of collision frequencies. Insight from the small electron-to-ion mass ratio theory may lead to a computationally efficient treatment of extended modes.
More details from the publisher
Details from ORA
More details
Details from ArXiV

Three-Dimensional Inhomogeneity of Electron-Temperature-Gradient Turbulence in the Edge of Tokamak Plasmas

(2022)

Authors:

JF Parisi, FI Parra, CM Roach, MR Hardman, AA Schekochihin, IG Abel, N Aiba, J Ball, M Barnes, B Chapman-Oplopoiou, D Dickinson, W Dorland, C Giroud, DR Hatch, JC Hillesheim, J Ruiz Ruiz, S Saarelma, D St-Onge
More details from the publisher

Interpreting Radial Correlation Doppler Reflectometry using Gyrokinetic Simulations

(2022)

Authors:

J Ruiz Ruiz, FI Parra, VH Hall-Chen, N Christen, M Barnes, J Candy, J Garcia, C Giroud, W Guttenfelder, JC Hillesheim, C Holland, NT Howard, Y Ren, AE White, JET contributors.
More details from the publisher
Details from ArXiV

A novel approach to radially global gyrokinetic simulation using the flux-tube code $\texttt{stella}$

(2022)

Authors:

DA St-Onge, M Barnes, FI Parra
More details from the publisher
Details from ArXiV

Input files for "A novel approach to radially global gyrokinetic simulation using the flux-tube code stella": arXiv 2201.01506

University of Oxford (2022)

Authors:

Denis A St-Onge, Michael Barnes, Felix I Parra

Abstract:

A collection of input files, and instructions on how to use them, for the manuscript entitled 'A novel approach to radially global gyrokinetic simulation using the flux-tube code stella'. These input files, which are designed for the gyrokinetic flux-tube code stella, are specifically for the simulations resulting in figures 2-10.
More details from the publisher
Details from ORA

Pagination

  • First page First
  • Previous page Prev
  • …
  • Page 6
  • Page 7
  • Page 8
  • Page 9
  • Current page 10
  • Page 11
  • Page 12
  • Page 13
  • Page 14
  • …
  • Next page Next
  • Last page Last

Footer Menu

  • Contact us
  • Giving to the Dept of Physics
  • Work with us
  • Media

User account menu

  • Log in

Follow us

FIND US

Clarendon Laboratory,

Parks Road,

Oxford,

OX1 3PU

CONTACT US

Tel: +44(0)1865272200

University of Oxfrod logo Department Of Physics text logo
IOP Juno Champion logo Athena Swan Silver Award logo

© University of Oxford - Department of Physics

Cookies | Privacy policy | Accessibility statement

Built by: Versantus

  • Home
  • Research
  • Study
  • Engage
  • Our people
  • News & Comment
  • Events
  • Our facilities & services
  • About us
  • Current students
  • Staff intranet