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  Supernova remnants and the effect of efficient cosmic ray acceleration

Reville, B. (2008). Supernova remnants and the effect of efficient cosmic ray acceleration. Talk presented at Canadian institute for Theoretical Astrophysics. Toronto, Canada. 2008-07-21.

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 Creators:
Reville, Brian1, Author           
Affiliations:
1Division Prof. Dr. Werner Hofmann, MPI for Nuclear Physics, Max Planck Society, ou_904550              

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 Abstract: It is well known that electrons and probably cosmic rays are accelerated in supernova remnants. To maintain the observed steady galactic cosmic-ray spectrum, it is necessary that they be very efficient accelerators. The back reaction of the high-energy particles on the shock structure and environment are reviewed with a particular emphasis on the amplification of magnetic fields.

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Language(s): eng - English
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 Publication Status: Not specified
 Pages: -
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 Rev. Type: -
 Identifiers: eDoc: 395706
 Degree: -

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Title: Canadian institute for Theoretical Astrophysics
Place of Event: Toronto, Canada
Start-/End Date: 2008-07-21
Invited: Yes

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