Embedding of the Kerr-Newman Black Hole Surface in Euclidean Space

TL;DR

This paper presents a method to embed the surface of a Kerr-Newman black hole into four-dimensional Euclidean space, providing a new geometric perspective on black hole horizons.

Contribution

It introduces a global embedding of the Kerr-Newman black hole surface in Euclidean space, which was not previously achieved.

Findings

Successful embedding of the black hole surface in 4D Euclidean space

Provides new geometric insights into black hole horizons

Potential applications in understanding black hole thermodynamics

Abstract

We obtain a global embedding of the surface of a rapidly rotating Kerr-Newman black hole in an Euclidean 4-dimensional space.