- Abstract:
-
We simulate time-dependent particle acceleration in the blast wave of a young supernova remnant (SNR), using a Monte Carlo approach for the diffusion and acceleration of the particles, coupled to a magnetohydrodynamics code. We calculate the distribution function of the cosmic rays concurrently with the hydrodynamic evolution of the SNR, and compare the results with those obtained using simple steady-state models. The surrounding medium into which the SNR evolves turns out to be of great infl...
Expand abstract - Publication status:
- Published
- Publisher copy:
- 10.1111/j.1365-2966.2010.16857.x
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- Journal:
- MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
- Volume:
- 406
- Issue:
- 4
- Pages:
- 2633-2649
- Publication date:
- 2010-08-21
- DOI:
- EISSN:
-
1365-2966
- ISSN:
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0035-8711
- URN:
-
uuid:bf10af54-34f7-47e6-8f17-66736fedd9e7
- Source identifiers:
-
161671
- Local pid:
- pubs:161671
- Language:
- English
- Keywords:
- Copyright date:
- 2010
Journal article
Time-dependent particle acceleration in supernova remnants in different environments
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