A 4D asymptotically flat rotating black hole solution including supertraslation correction

TL;DR

This paper derives a new 4D asymptotically flat rotating black hole solution with supertranslation corrections, extending previous static models and confirming its consistency with Einstein's equations.

Contribution

It introduces a linear-order supertranslation correction to the Kerr black hole in Boyer-Lindquist coordinates, generalizing supertranslated spacetime to rotating black holes.

Findings

The solution satisfies Einstein's equations.

The angular momentum including supertranslation correction is calculated.

The method extends supertranslation effects to rotating black holes.

Abstract

In this study, beginning with the 4D asymptotically flat Kerr black hole solution in the Boyer-Lindquist (BL) coordinate system, then by using the technique of frame-dragging and some coordinate transformation to incorporate the linear-order supertranslation correction, we finally obtain a 4D asymptotically flat black hole solution with an arbitrary $a$ in the linear-order supertranslated BL coordinate system. We can confirm that this satisfies the Einstein equation. At the end, we calculate the angular momentum of the spacetime we obtained in this study including the linear-order correction. Since the supertranslation is a type of the general coordinate transformation, which is usually defined by linear-order, the corrections we incorporate in this study is sufficient, considering the fact that $a$ is arbitrary. This work is interesting as a generalization of the supertranslated spacetime to the rotating system.