Journal article icon

Journal article

Turbulent dynamo in a collisionless plasma

Abstract:
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 observations. Extragalactic plasmas are weakly collisional (as opposed to collisional magnetohydrodynamic fluids), and whether magnetic-field growth and its sustainment through an efficient dynamo instability driven by chaotic motions is possible in such plasmas is not known. Fully kinetic numerical simulations of the Vlasov equation in a six-dimensional phase space necessary to answer this question have until recently remained beyond computational capabilities. Here, we show by means of such simulations that magnetic-field amplification via a turbulent dynamo instability does occur in a stochastically-driven, non-relativistic subsonic flow of initially unmagnetized collisionless plasma. We also find that this collisionless dynamo self-accelerates and becomes entangled with kinetic instabilities as the plasma magnetization increases. These results suggest that a turbulent "plasma dynamo" can magnetize the intracluster medium up to near-equipartition levels on a timescale much shorter than the Hubble time, and emphasize the crucial role of multiscale kinetic physics in high-energy astrophysical plasmas.
Publication status:
Published
Peer review status:
Peer reviewed

Actions

Access Document

Files:
Publisher copy:
10.1073/pnas.1525194113

Authors

More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Theoretical Physics
Role:
Author


Publisher:
National Academy of Sciences
Journal:
Proceedings of the National Academy of Sciences More from this journal
Volume:
113
Issue:
15
Pages:
3950-3953
Publication date:
2016-04-12
Acceptance date:
2016-03-01
DOI:
EISSN:
1091-6490


Keywords:
Pubs id:
pubs:580971
UUID:
uuid:2e4369c3-c7fb-4f91-9ae8-b95e5aec15c5
Local pid:
pubs:580971
Source identifiers:
580971
Deposit date:
2016-04-05
ARK identifier:

Terms of use


Views and Downloads






If you are the owner of this record, you can report an update to it here: Report update to this record

TO TOP