Collisionless Magnetic Reconnection in Curved Spacetime and the Effect of Black Hole Rotation

Abstract

Magnetic reconnection in curved spacetime is studied by adopting a general relativistic magnetohydrodynamic model that retains collisionless effects for both electron-ion and pair plasmas. A simple generalization of the standard Sweet-Parker model allows us to obtain the first order effects of the gravitational field of a rotating black hole. It is shown that the black hole rotation acts as to increase the length of azimuthal reconnection layers, per se leading to a decrease of the reconnection rate. However, when coupled to collisionless thermal-inertial effects, the net reconnection rate is enhanced with respect to what would happen in a purely collisional plasma due to a broadening of the reconnection layer. These findings identify an underlying interaction between gravity and collisionless magnetic reconnection in the vicinity of compact objects.

Accepted for publication in Physical Review D

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• Magnetic reconnection under centrifugal and gravitational electromotive forces
• Gravitational electromotive force in magnetic reconnection around Schwarzschild black holes
• Generalized Magnetofluid Connections in Curved Spacetime
• Yet Another Modification of Relativistic Magnetohydrodynamic Waves: Electron Thermal Inertia