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A CHANDRA image of the supernova remnant Cas A superimposed on the Gemini laser at the UK Central Laser Facility

The plasma physics of supernova remnants in astrophysics is similar to plasma physics of solids irradiated with powerful lasers in the laboratory.

Credit: 1) The Royal Society (personal photo) 2) NASA/CXC/MIT/UMass Amherst/M.D.Stage et al. (Cas A) 3) STFC (laser)

Tony Bell FRS

Academic Visitor

Research theme

  • Particle astrophysics & cosmology
  • Plasma physics

Sub department

  • Atomic and Laser Physics
Tony.Bell@physics.ox.ac.uk
Telephone: 01865 (2)72210
Clarendon Laboratory, room 316.4
  • About
  • Publications

The interaction of cosmic rays and magnetized plasma

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 358:1 (2005) 181-187
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Turbulent amplification of magnetic field and diffusive shock acceleration of cosmic rays

Monthly Notices of the Royal Astronomical Society 353 (2004) 550-558
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An implicit Vlasov-Fokker-Planck code to model non-local electron transport in 2-D with magnetic fields

JOURNAL OF COMPUTATIONAL PHYSICS 194:1 (2004) 1-34

Authors:

RJ Kingham, AR Bell
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Resistive Collimation of Electron Beams in Laser-Produced Plasmas

Physical Review Letters 91 (2003) 035003 4pp

Authors:

AR Bell, R.J. Kingham
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Nonlocal magnetic-field generation in plasmas without density gradients.

Phys Rev Lett 88:4 (2002) 045004

Authors:

RJ Kingham, AR Bell

Abstract:

Conventional theories of magnetic-field generation by laser pulses in collisional plasmas require the presence of density gradients or anisotropic pressure. Using the first two-dimensional Fokker-Planck code to self-consistently include magnetic fields, we find that magnetic fields can be spontaneously generated when a collisional plasma is nonuniformly heated even though inverted delta n = 0 and the pressure is purely isotropic. These magnetic fields, which can become strong enough to significantly affect transport, are attributed to nonlocal effects that are missing in the standard, local theories.
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