Hostname: page-component-745bb68f8f-lrblm Total loading time: 0 Render date: 2025-01-14T13:15:25.054Z Has data issue: false hasContentIssue false
  • English
  • Français

Particle acceleration processes in the cosmic large-scale structure

Published online by Cambridge University Press:  01 August 2006

Torsten A. Enßlin  and
Christoph Pfrommer
Torsten A. Enßlin
Affiliation:
Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Straße 1, D85741 Garching, Germany email: [email protected]
Christoph Pfrommer
Affiliation:
Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Straße 1, D85741 Garching, Germany email: [email protected] Canadian Institute for Theoretical Astrophysics, 60 St. George Street, Toronto, Ontario, M5S 3H8Canada
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The energetic shock waves associated with the violent large-scale structure formation process are able to accelerate relativistic electrons and protons. The induced non-thermal emission, especially at long radio wavelength, provides a fascinating perspective into structure formation, the relativistic Universe, and cosmic magnetic fields.

Keywords

acceleration of particleslarge-scale structure of universe
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Highlights of Astronomy 14: Highlights of Astronomy , August 2006 , pp. 372 - 373
Copyright
Copyright © International Astronomical Union 2007

References

Dennison, B. 1980, ApJ (Letters), 239, L93CrossRefGoogle Scholar
Ensslin, T.A., Biermann, P.L., Klein, U., & Kohle, S. 1998, A&A, 332, 395Google Scholar
Ensslin, T.A., & Gopal-Krishna, 2001, A&A, 366, 26Google Scholar
Ensslin, T.A., & Brüggen, M. 2002, MNRAS, 331, 1011CrossRefGoogle Scholar
Pfrommer, C., Springel, V., Ensslin, T. A., & Jubelgas, M. 2006, MNRAS, 367, 113CrossRefGoogle Scholar