Stable surfaces in electrostatic space-times have charged Hawking mass bounded below by an explicit formula in area, charge, and the cosmological constant, with equality cases realized by photon spheres and black hole horizons.
A Quasi-Local Mass
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abstract
We define a new gauge independent quasi-local mass and energy, and show its relation to the Brown-York Hamilton-Jacobi analysis. A quasi-local proof of the positivity, based on spacetime harmonic functions, is given for admissible closed spacelike 2-surfaces which enclose an initial data set satisfying the dominant energy condition. Like the Wang-Yau mass, the new definition relies on isometric embeddings into Minkowski space, although our notion of admissibility is different from that of Wang-Yau. Rigidity is also established, in that vanishing energy implies that the 2-surface arises from an embedding into Minkowski space, and conversely the mass vanishes for any such surface. Furthermore, we show convergence to the ADM mass at spatial infinity, and provide the equation associated with optimal isometric embedding.
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Sharp lower bound for the charged Hawking mass in the electrostatic space
Stable surfaces in electrostatic space-times have charged Hawking mass bounded below by an explicit formula in area, charge, and the cosmological constant, with equality cases realized by photon spheres and black hole horizons.