Skip to main content
Home
Department Of Physics text logo
  • Research
    • Our research
    • Our research groups
    • Our research in action
    • Research funding support
    • Summer internships for undergraduates
  • Study
    • Undergraduates
    • Postgraduates
  • Engage
    • For alumni
    • For business
    • For schools
    • For the public
Menu
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 Oxford University Press (OUP) 449:4 (2015) 3693-3699

Authors:

G Giacinti, AR Bell
More details from the publisher

Cosmic ray origins in supernova blast waves

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 447:3 (2015) 2224-2234
More details from the publisher

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
More details from the publisher

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

Pagination

  • First page First
  • Previous page Prev
  • Page 1
  • Page 2
  • Page 3
  • Page 4
  • Current page 5
  • Page 6
  • Page 7
  • Page 8
  • Page 9
  • …
  • Next page Next
  • Last page Last

Footer Menu

  • Contact us
  • Giving to the Dept of Physics
  • Work with us
  • Media

User account menu

  • Log in

Follow us

FIND US

Clarendon Laboratory,

Parks Road,

Oxford,

OX1 3PU

CONTACT US

Tel: +44(0)1865272200

University of Oxfrod logo Department Of Physics text logo
IOP Juno Champion logo Athena Swan Silver Award logo

© University of Oxford - Department of Physics

Cookies | Privacy policy | Accessibility statement

Built by: Versantus

  • Home
  • Research
  • Study
  • Engage
  • Our people
  • News & Comment
  • Events
  • Our facilities & services
  • About us
  • Current students
  • Staff intranet