Wang and Yau's Quasi-Local Energy for an Extreme Kerr Spacetime
arXiv:1708.07532 · doi:10.1088/1361-6382/aaa625
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 to explore the values of in the space of coefficients. From our analysis, we discovered an open region of complex values for . We also study the physical properties of the smallest real value of , which lies on the boundary separating real and complex energies.
25 pages, 10 figures
References in corpus (6)
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Cited by in corpus (6)
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- Quasi-Local Energy of a Rotating Object Described by Kerr Spacetime
- Energy in critical collapse
- Black Holes, Complex Curves, and Graph Theory: Revising a Conjecture by Kasner
- Strong field behavior of Wang-Yau Quasi-local energy