Theory and Applications of Non-Relativistic and Relativistic Turbulent Reconnection
A. Lazarian, G. Kowal, M. Takamoto, E. M. de Gouveia Dal Pino, and J., Cho

TL;DR
This paper reviews the role of turbulence in magnetic reconnection in astrophysical environments, extending non-relativistic theories to relativistic cases, supported by simulations and observational considerations.
Contribution
It extends magnetic reconnection theory from non-relativistic to relativistic turbulence and provides numerical evidence supporting this extension.
Findings
Turbulent reconnection violates magnetic flux freezing.
Numerical simulations support the extension of non-relativistic theory to relativistic cases.
Implications include particle acceleration and astrophysical phenomena like gamma-ray bursts.
Abstract
Realistic astrophysical environments are turbulent due to the extremely high Reynolds numbers. Therefore, the theories of reconnection intended for describing astrophysical reconnection should not ignore the effects of turbulence on magnetic reconnection. Turbulence is known to change the nature of many physical processes dramatically and in this review we claim that magnetic reconnection is not an exception. We stress that not only astrophysical turbulence is ubiquitous, but also magnetic reconnection itself induces turbulence. Thus turbulence must be accounted for in any realistic astrophysical reconnection setup. We argue that due to the similarities of MHD turbulence in relativistic and non-relativistic cases the theory of magnetic reconnection developed for the non-relativistic case can be extended to the relativistic case and we provide numerical simulations that support this…
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