Analytic study of the Maxwell electromagnetic invariant in spinning and charged Kerr-Newman black-hole spacetimes

TL;DR

This paper provides an analytical investigation of the Maxwell electromagnetic invariant in Kerr-Newman black-hole spacetimes, revealing how it varies with spin and charge, and identifying critical spin values that change its spatial behavior.

Contribution

It analytically characterizes the Maxwell invariant's behavior in Kerr-Newman spacetimes, identifying critical spin thresholds and their impact on the invariant's spatial properties.

Findings

Minimum Maxwell invariant occurs on the equator for all Kerr-Newman black holes.

Three regimes of spin parameter determine the invariant's behavior: negative definite, maximum at poles, and non-monotonic.

Critical spin values mark boundaries between different qualitative behaviors of the invariant.

Abstract

The Maxwell invariant plays a fundamental role in the mathematical description of electromagnetic fields in charged spacetimes. We present a detailed {\it analytical} study of the physical and mathematical properties of the Maxwell electromagnetic invariant ${\cal F}_{\text{KN}}(r,\theta;M,a,Q)$ which characterizes the Kerr-Newman black-hole spacetime. It is proved that, for all Kerr-Newman black-hole spacetimes, the spin and charge dependent minimum value of the Maxwell electromagnetic invariant is attained on the equator of the black-hole surface. Interestingly, we reveal the physically important fact that Kerr-Newman spacetimes are characterized by two critical values of the dimensionless rotation parameter ${\hat a}\equiv a/r_+$, ${\hat a}^{-}_{\text{crit}}=\sqrt{3-2\sqrt{2}}$ and ${\hat a}^{+}_{\text{crit}}= \sqrt{5-2\sqrt{5}}$, which mark the boundaries between three qualitatively different spatial functional behaviors of the Maxwell electromagnetic invariant: (i) Kerr-Newman black holes in the slow-rotation ${\hat a}<{\hat a}^{-}_{\text{crit}}$ regime are characterized by negative definite Maxwell electromagnetic invariants that increase monotonically towards spatial infinity, (ii) for black holes in the intermediate spin regime ${\hat a}^{-}_{\text{crit}}\leq {\hat a}\leq{\hat a}^{+}_{\text{crit}}$, the positive global maximum of the Kerr-Newman Maxwell electromagnetic invariant is located at the black-hole poles, and (iii) Kerr-Newman black holes in the super-critical regime ${\hat a}>{\hat a}^{+}_{\text{crit}}$ are characterized by a non-monotonic spatial behavior of the Maxwell electromagnetic invariant along the black-hole horizon with a spin and charge dependent global maximum whose polar angular location is characterized by the dimensionless functional relation ${\hat a}^2\cdot(\cos^2\theta)_{\text{max}}=5-2\sqrt{5}$.