Abstract
We establish a class of area–angular momentum–charge inequalities satisfied by stable marginally outer trapped surfaces in 5-dimensional minimal supergravity which admit a \(U(1)^2\) symmetry. A novel feature is the fact that such surfaces can have the non-trivial topologies \(S^1 \times S^2\) and L(p, q). In addition to two angular momenta, they may be characterized by ‘dipole charge’ as well as electric charge. We show that the unique geometries which saturate the inequalities are the horizon geometries corresponding to extreme black hole solutions. Analogous inequalities which also include contributions from a positive cosmological constant are also presented.
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Communicated by Krzysztof Gawȩdzki.
Hari Kunduri: On sabbatical leave from Memorial University of Newfoundland.
A. Alaee acknowledges the support of a NSERC Postdoctoral Fellowship 502873 and PIMS Postdoctoral Fellowship. M. Khuri acknowledges the support of NSF Grants DMS-1308753 and DMS-1708798. H. Kunduri acknowledges the support of NSERC Grant 418537-2012.
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Alaee, A., Khuri, M. & Kunduri, H. Bounding Horizon Area by Angular Momentum, Charge, and Cosmological Constant in 5-Dimensional Minimal Supergravity. Ann. Henri Poincaré 20, 481–525 (2019). https://doi.org/10.1007/s00023-018-0749-4
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DOI: https://doi.org/10.1007/s00023-018-0749-4