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91探花
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

Nonlinear Phase Mixing and Phase-Space Cascade of Entropy in Gyrokinetic Plasma Turbulence

Physical Review Letters American Physical Society (APS) 103:1 (2009) 015003

Authors:

T Tatsuno, W Dorland, AA Schekochihin, GG Plunk, M Barnes, SC Cowley, GG Howes

Linearized model Fokker鈥揚lanck collision operators for gyrokinetic simulations. II. Numerical implementation and tests

Physics of Plasmas AIP Publishing 16:7 (2009) 072107

Authors:

M Barnes, IG Abel, W Dorland, DR Ernst, GW Hammett, P Ricci, BN Rogers, AA Schekochihin, T Tatsuno

Trinity: A Unified Treatment of Turbulence, Transport, and Heating in Magnetized Plasmas

ArXiv 0901.2868 (2009)

Abstract:

To faithfully simulate ITER and other modern fusion devices, one must resolve electron and ion fluctuation scales in a five-dimensional phase space and time. Simultaneously, one must account for the interaction of this turbulence with the slow evolution of the large-scale plasma profiles. Because of the enormous range of scales involved and the high dimensionality of the problem, resolved first-principles global simulations are very challenging using conventional (brute force) techniques. In this thesis, the problem of resolving turbulence is addressed by developing velocity space resolution diagnostics and an adaptive collisionality that allow for the confident simulation of velocity space dynamics using the approximate minimal necessary dissipation. With regard to the wide range of scales, a new approach has been developed in which turbulence calculations from multiple gyrokinetic flux tube simulations are coupled together using transport equations to obtain self-consistent, steady-state background profiles and corresponding turbulent fluxes and heating. This approach is embodied in a new code, Trinity, which is capable of evolving equilibrium profiles for multiple species, including electromagnetic effects and realistic magnetic geometry, at a fraction of the cost of conventional global simulations. Furthermore, an advanced model physical collision operator for gyrokinetics has been derived and implemented, allowing for the study of collisional turbulent heating, which has not been extensively studied. To demonstrate the utility of the coupled flux tube approach, preliminary results from Trinity simulations of the core of an ITER plasma are presented.

Linearized model Fokker鈥揚lanck collision operators for gyrokinetic simulations. I. Theory

Physics of Plasmas AIP Publishing 15:12 (2008) 122509

Authors:

IG Abel, M Barnes, SC Cowley, W Dorland, AA Schekochihin

Nonlinear phase mixing and phase-space cascade of entropy in gyrokinetic plasma turbulence

(2008)

Authors:

T Tatsuno, W Dorland, AA Schekochihin, GG Plunk, M Barnes, SC Cowley, GG Howes

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