Magnetic fields pervade the entire Universe and, through their dynamical interactions with matter, affect the formation and evolution of astrophysical systems from cosmological to planetary scales. How primordial cosmological seed fields arose and were further amplified to $\mu$Gauss levels reported in nearby galaxy clusters, near equipartition with kinetic energy of plasma motions and on scales of at least tens of kiloparsecs, is a major theoretical puzzle still largely unconstrained by obse...Expand abstract
- Publication status:
- Peer review status:
- Peer reviewed
- National Academy of Sciences Publisher's website
- Proceedings of the National Academy of Sciences Journal website
- Publication date:
- Source identifiers:
- Local pid:
- Copyright holder:
- Rincon et al.
- Copyright date:
- Copyright Rincon et al.
Turbulent dynamo in a collisionless plasma
If you are the owner of this record, you can report an update to it here: Report update to this record