Journal
JOURNAL OF HIGH ENERGY PHYSICS
Volume -, Issue 11, Pages -Publisher
SPRINGER
DOI: 10.1088/1126-6708/2009/11/089
Keywords
Black Holes in String Theory; Black Holes
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Funding
- DSM CEA-Saclay
- ANR [BLAN 06-3-137168, 08-JCJC-0001-01]
- Marie Curie IRG [046430]
- DOE [DE-FG03-84ER-40168]
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We construct a four-parameter family of smooth, horizonless, stationary solutions of ungauged five-dimensional supergravity by using the four-dimensional Euclidean Schwarzschild metric as a base space and magnetizing its bolt. We then generalize this to a five-parameter family based upon the Euclidean Kerr-Taub-Bolt. These running Bolt solutions are necessarily non-static. They also have the same charges and mass as a non-extremal black hole with a classically-large horizon area. Moreover, in a certain regime their mass can decrease as their charges increase. The existence of these solutions supports the idea that the singularities of non-extremal black holes are resolved by low-mass modes that correct the singularity of the classical black hole solution on large (horizon-sized) scales.
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