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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
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Research interests

Astrophysical plasmas

Cosmic rays are high energy particles, mostly protons, arriving at the Earth and detected in many places in the Universe. Blast waves launched by supernova explosions (Cassiopeia A is a good example) are probably the main source of cosmic rays in our Milky Way Galaxy, reaching energies up to a few PeV. The highest energy cosmic rays with energies exceeding 100EeV are almost certainly accelerated in even more energetic events outside our own galaxy. Our aim is to understand the plasma processes responsible for cosmic ray acceleration and to explain cosmic ray origins.

Laser-produced plasmas

Solids and gases can be heated and converted to a plasma with a very high energy density with high power lasers. An important potential application is inertial fusion energy (IFE) for electricity generation. At very high laser intensities the plasma is relativistic. Lasers are now entering a regime in which QED is important.

Research interests

Astrophysical plasmas
Laser-produced plasmas

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