Relativistic particle acceleration using lasers and plasmas

1997 ◽  
Vol 39 (5A) ◽  
pp. A161-A175 ◽  
Author(s):  
G Matthieussent
2017 ◽  
Author(s):  
Markus Böttcher ◽  
Matthew Baring ◽  
Errol J. Summerlin

1987 ◽  
Vol 228 (4) ◽  
pp. 843-868 ◽  
Author(s):  
V. A. Dogiel ◽  
A. V. Gurevich ◽  
Y. N. Istomin ◽  
K. P. Zybin

2005 ◽  
Vol 192 ◽  
pp. 59-69
Author(s):  
Claes Fransson ◽  
Claes-Ingvar Björnsson

SummaryModeling of radio and X-ray observations of supernovae interacting with their circumstellar media are discussed, with special application to SN 1993J and SN 2002ap. We emphasize the importance of including all relevant physical mechanisms, especially for the modeling of the radio light curves. The different conclusions for the absorption mechanism (free-free or synchrotron self-absorption), as well as departures from an ρ ∝ r−2 CSM, as inferred by some authors, are discussed in detail. We conclude that the evidence for a variation in the mass loss rate with time is very weak. The results regarding the efficiencies of magnetic field generation and relativistic particle acceleration are summarized.


1994 ◽  
Vol 90 ◽  
pp. 797 ◽  
Author(s):  
Jonathan Arons ◽  
Marco Tavani

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