Fast magnetic reconnection in Kerr spacetime

TL;DR

This paper investigates how the curvature of spacetime around Kerr black holes affects the rate of magnetic reconnection, revealing that black hole rotation and observer frame significantly influence reconnection dynamics.

Contribution

It generalizes the Petschek model to Kerr spacetime, analyzing reconnection rates in different frames and configurations, highlighting the impact of black hole rotation.

Findings

Reconnection rate decreases in ZAMO frame due to spacetime curvature.

Asymmetric reconnection rates occur in non-ZAMO frames for slow black hole rotation.

Results clarify rotation effects on reconnection in flat spacetime limit.

Abstract

We develop a relativistic scenario of fast magnetic reconnection process, for general magnetohydrodynamical plasmas around Kerr black holes. Generalizing the Petschek model, we study various properties of the reconnection layer in distinct configurations. When current sheet forms in the zero-angular-momentum (ZAMO) frame which corotates with the black hole, the reconnection rate for both radial and azimuthal configurations is decreased by spacetime curvature. However, when the current sheet forms in a non-ZAMO frame, which rotates either faster or slower than the black hole, detail analysis establishes that for any given slow rotations (subrelativistic at most) and mildly relativistic inflow, the ZAMO observer will find asymmetric reconnection rates for radial configuration: it is decreased on one side of the current sheet and is increased on the other side in comparison to the unrotation limit. This is valid to both the Sweet-Parker and the Petschek scenario. The results clarify the effects of rotation on the reconnection layer in the laboratory frame in the flat spacetime limit.