For a Sweet-Parker pair-plasma current sheet, gravitational curvature changes the fast reconnection rate only infinitesimally on local scales, but observer motion can reduce the observed rate by powers of the Lorentz factor.
Quasi-Periodic Pulsations in Solar and Stellar Flares: A Review of Underpinning Physical Mechanisms and Their Predicted Observational Signatures,
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Generally relativistic description of fast magnetic reconnection induced by thermal electromotive force
For a Sweet-Parker pair-plasma current sheet, gravitational curvature changes the fast reconnection rate only infinitesimally on local scales, but observer motion can reduce the observed rate by powers of the Lorentz factor.