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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

Particle Acceleration by Shocks in Supernova Remnants

Brazilian Journal of Physics Springer Nature 44:5 (2014) 415-425
More details from the publisher

Turbulent amplification of magnetic fields in laboratory laser-produced shock waves

Nature Physics Springer Nature 10:7 (2014) 520-524

Authors:

J Meinecke, HW Doyle, F Miniati, AR Bell, R Bingham, R Crowston, RP Drake, M Fatenejad, M Koenig, Y Kuramitsu, C C. Kuranz, DQ Lamb, D Lee, MJ MacDonald, CD Murphy, H-S Park, A Pelka, A Ravasio, Y Sakawa, AA Schekochihin, A Scopatz, P Tzeferacos, WC Wan, NC Woolsey, R Yurchak, B Reville, G Gregori
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On the maximum energy of shock-accelerated cosmic rays at ultra-relativistic shocks

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 439:2 (2014) 2050-2059

Authors:

B Reville, AR Bell
More details from the publisher

Modelling gamma-ray photon emission and pair production in high-intensity laser-matter interactions

Journal of Computational Physics 260 (2014) 273-285

Authors:

CP Ridgers, JG Kirk, R Duclous, TG Blackburn, CS Brady, K Bennett, TD Arber, AR Bell

Abstract:

In high-intensity (>1021 Wcm -2) laser-matter interactions gamma-ray photon emission by the electrons can strongly affect the electron's dynamics and copious numbers of electron-positron pairs can be produced by the emitted photons. We show how these processes can be included in simulations by coupling a Monte Carlo algorithm describing the emission to a particle-in-cell code. The Monte Carlo algorithm includes quantum corrections to the photon emission, which we show must be included if the pair production rate is to be correctly determined. The accuracy, convergence and energy conservation properties of the Monte Carlo algorithm are analysed in simple test problems. © 2013 Elsevier Inc.
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Synchrotron radiation, pair production, and longitudinal electron motion during 10-100 PW laser solid interactions

Physics of Plasmas AIP Publishing 21:3 (2014) 033108

Authors:

CS Brady, CP Ridgers, TD Arber, AR Bell
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