Abstract
We construct a time-symmetric asymptotically flat initial data set to the Einstein-Maxwell Equations which satisfies m -1/2 (R + Q^2 / R) > 0
where m is the total mass, R = \sqrt A / 4 pi is the area radius of the outermost horizon and Q is the total charge. This yields a counter-example to a natural extension of the Penrose Inequality for charged black holes
Original language | English |
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Pages (from-to) | 703 - 723 |
Number of pages | 21 |
Journal | Communications in Mathematical Physics |
Volume | 257 |
Issue number | 3 |
DOIs | |
Publication status | Published - 2005 |
Externally published | Yes |