Maxwell fields in boosted Kerr black holes

The spacetime of a boosted Bondi-Sachs rotating black hole is considered as proper background to examine electromagnetic configurations connected analytic solutions Maxwell equations. In our analysis, we first use the transformations in order bring metric into Kerr-Schild form, from which zero angular momentum observers (ZAMOs) are constructed via ADM formalism. coordinates obtain Killing fields sources electrodynamics, and fix ZAMO evaluate components electric magnetic fields, nonsingular patterns an eventual momentum-energy emission hole. Distinct examined discussed case variations boost parameter $\gamma$. We extend analysis by considering framework hole, it moves at relativistic speeds. also discuss possible mechanisms that may resemble magnetospheres holes give rise hydromagnetic flows accretion discs production jets.