Wang and Yau's Quasi-Local Energy for an Extreme Kerr Spacetime
Warner A. Miller, Shannon Ray, Mu-Tao Wang, Shing-Tung Yau

TL;DR
This paper investigates the Wang and Yau quasi-local energy in Kerr spacetimes, revealing critical points, explicit functional forms, and complex energy values, thereby advancing understanding of energy definitions in rotating black hole geometries.
Contribution
It provides an explicit analysis of the Wang and Yau quasi-local energy functional for Kerr surfaces, including critical points and complex energy regions, extending previous embedding-based energy concepts.
Findings
W-Y QLE reduces to B-Y QLE at the critical point τ=0.
The energy functional has a critical point at τ=0 for all constant radial surfaces.
An open region of complex energy values is identified in the functional analysis.
Abstract
There exist constant radial surfaces, , that may not be globally embeddable in for Kerr spacetimes with . To compute the Brown and York (B-Y) quasi-local energy (QLE), one must isometrically embed into . On the other hand, the Wang and Yau (W-Y) QLE embeds into Minkowski space. In this paper, we examine the W-Y QLE for surfaces that may or may not be globally embeddable in . We show that their energy functional, , has a critical point at for all constant radial surfaces in hypersurfaces using Boyer-Lindquist coordinates. For , the W-Y QLE reduces to the B-Y QLE. To examine the W-Y QLE in these cases, we write the functional explicitly in terms of under the assumption that is only a function of . We then use a Fourier expansion of…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
