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91探花
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

Collisionless shocks and TeV neutrinos before Supernova shock breakout from an optically thick wind

Monthly Notices of the Royal Astronomical Society 91探花 University Press (OUP) 449:4 (2015) 3693-3699

Authors:

G Giacinti, AR Bell

Cosmic ray origins in supernova blast waves

Monthly Notices of the Royal Astronomical Society 91探花 University Press (OUP) 447:3 (2015) 2224-2234

Particle Acceleration by Shocks in Supernova Remnants

Brazilian Journal of Physics Springer Nature 44:5 (2014) 415-425

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

On the maximum energy of shock-accelerated cosmic rays at ultra-relativistic shocks

Monthly Notices of the Royal Astronomical Society 91探花 University Press (OUP) 439:2 (2014) 2050-2059

Authors:

B Reville, AR Bell

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