Bounds on area and charge for marginally trapped surfaces with cosmological constant
arXiv:1109.6140 · doi:10.1088/0264-9381/29/6/062001
Abstract
We sharpen the known inequalities and between the area and the electric charge of a stable marginally outer trapped surface (MOTS) of genus g in the presence of a cosmological constant . In particular, instead of requiring stability we include the principal eigenvalue of the stability operator. For we obtain a lower and an upper bound for in terms of as well as the upper bound for the charge, which reduces to in the stable case . For there remains only a lower bound on . In the spherically symmetric, static, stable case one of the area inequalities is saturated iff the surface gravity vanishes. We also discuss implications of our inequalities for "jumps" and mergers of charged MOTS.
minor corrections to previous version and to published version
References in corpus (5)
Cited by in corpus (12)
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