Particle acceleration in supernova remnants
Supernova remnants (SNR) are the most likely source of galactic cosmic rays (CRs) up to the 'knee' in the spectrum at a few PeV. The theory of diffusive shock acceleration nicely supplies a power law energy distribution with approximately the desired spectral index and with suitably high e...
Päätekijä: | Bell, A |
---|---|
Aineistotyyppi: | Conference item |
Julkaistu: |
2009
|
Samankaltaisia teoksia
-
Particle Acceleration by Shocks in Supernova Remnants
Tekijä: Bell, A
Julkaistu: (2014) -
Cosmic ray acceleration in young supernova remnants
Tekijä: Schure, K, et al.
Julkaistu: (2013) -
COSMIC-RAY ACCELERATION IN PULSAR-DRIVEN SUPERNOVA-REMNANTS
Tekijä: Bell, A
Julkaistu: (1992) -
Time-dependent particle acceleration in supernova remnants in different environments
Tekijä: Schure, K, et al.
Julkaistu: (2010) -
Cosmic-ray acceleration and escape from supernova remnants
Tekijä: Bell, A, et al.
Julkaistu: (2013)