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  The Theory of Synchrotron Emission of Supernova Remnants

Berezhko, E., & Völk, H. (2005). The Theory of Synchrotron Emission of Supernova Remnants. In J. Blümer (Ed.), Contributions to the 29th International Cosmic Ray Conference (pp. 219-222). Karlsruhe: Forschungszentrum Karlsruhe.

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 Creators:
Berezhko, Evgeni1, Author
Völk, Heinrich2, Author              
Affiliations:
1Yu.G.Shafer Institute of Cosmophysical Research and Aeronomy, 31 Lenin Ave., 677980 Yakutsk, Russia, ou_persistent22              
2Prof. Heinrich J. Völk, Emeriti, MPI for Nuclear Physics, Max Planck Society, ou_907548              

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Free keywords: Supernova Remnants
 Abstract: Time-dependent nonlinear kinetic theory for cosmic ray (CR) acceleration in supernova remnants (SNRs) is applied in order to study the properties of the synchrotron emission from SNRs, in particular, the surface brightness-diameter relation. Detailed numerical calculations are performed for the expected range of the relevant physical parameters, namely the ambient density and the supernova explosion energy. The magnetic field in SNRs is assumed to be significantly amplified by the efficiently accelerating nuclear CR component. The theoretically predicted brightness-diameter relation in the radio range fits the observational data in a very satisfactory way.

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Language(s): eng - English
 Dates: 2005-12
 Publication Status: Published in print
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Type: -
 Identifiers: eDoc: 277791
URI: http://icrc2005.tifr.res.in/
 Degree: -

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Title: 29th International Cosmic Ray Conference
Place of Event: Pune, Mumbai
Start-/End Date: 2005-08-03 - 2005-08-10

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Title: Contributions to the 29th International Cosmic Ray Conference
Source Genre: Proceedings
 Creator(s):
Blümer, Johannes, Editor
Affiliations:
-
Publ. Info: Karlsruhe : Forschungszentrum Karlsruhe
Pages: - Volume / Issue: - Sequence Number: - Start / End Page: 219 - 222 Identifier: -