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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

Experimental studies of the advanced fast ignitor scheme

PHYSICS OF PLASMAS 7:9 (2000) PII [S1070-664X(00)02809-3]

Authors:

PA Norreys, R Allott, RJ Clarke, J Collier, D Neely, SJ Rose, M Zepf, M Santala, AR Bell, K Krushelnick, AE Dangor, NC Woolsey, RG Evans, H Habara, T Norimatsu, R Kodama

Non-linear amplification of a magnetic field driven by cosmic ray streaming

ASTROPHYSICS AND SPACE SCIENCE 272:1-3 (2000) 255-262

Authors:

SG Lucek, AR Bell

Non-linear amplification of a magnetic field driven by cosmic ray streaming

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 314:1 (2000) 65-74

Authors:

SG Lucek, AR Bell

Plasma formation in metallic wire Z pinches

PHYSICAL REVIEW E 61:4 (2000) 4370-4380

Authors:

JP Chittenden, SV Lebedev, J Ruiz-Camacho, FN Beg, SN Bland, CA Jennings, AR Bell, HG Haines, SA Pikuz, TA Shelkovenko, DA Hammer

Magnetic focusing and trapping of high-intensity laser-generated fast electrons at the rear of solid targets.

Phys Rev E Stat Phys Plasmas Fluids Relat Interdiscip Topics 59:5 Pt B (1999) 6032-6036

Authors:

JR Davies, AR Bell, M Tatarakis

Abstract:

The transport of fast electrons generated by a 1 ps, 20 J, 10(19) W cm(-2), 1 microm wavelength laser pulse through 70-250 microm thick deuterated polyethylene (CD2) targets is modeled with a Fokker-Planck hybrid code in r-z geometry. Initially, electric field generation inhibits propagation, which then proceeds by the formation of a low resistivity channel due to Ohmic heating. The magnetic field generated at the edge of the channel leads to strong collimation. This is observed for a wide range of parameters. Reflection of electrons at the rear surface forms a magnetic field which focuses the incident electrons on to the rear surface and forces the reflected electrons outwards. This would lead to the formation of a small diameter plasma on the rear surface, as observed in experiments. The reflected electrons are confined to a cone by a self-generated magnetic field, enhancing energy deposition at the rear of the target.

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