charged, rotating black objects in einstein–maxwell-dilaton theory in d ≥ 5
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ID: 207264
2016
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Abstract
We show that the general framework proposed by Kleihaus et al. (2015) for the study of asymptotically flat vacuum black objects with k + 1 equal magnitude angular momenta in D ≥ 5 spacetime dimensions (with 0 ≤ k ≤ D - 5 2 ) can be extended to the case of Einstein–Maxwell-dilaton (EMd) theory. This framework can describe black holes with spherical horizon topology, the simplest solutions corresponding to a class of electrically charged (dilatonic) Myers–Perry black holes. Balanced charged black objects with S n + 1 × S 2 k + 1 horizon topology can also be studied (with D = 2 k + n + 4 ). Black rings correspond to the case k = 0 , while the solutions with k > 0 are black ringoids. The basic properties of EMd solutions are discussed for the special case of a Kaluza–Klein value of the dilaton coupling constant. We argue that all features of these solutions can be derived from those of the vacuum seed configurations.
| Reference Key |
kleihaus2016entropycharged,
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|---|---|
| Authors | ;Burkhard Kleihaus;Jutta Kunz;Eugen Radu |
| Journal | European journal of medicinal chemistry |
| Year | 2016 |
| DOI |
10.3390/e18050187
|
| URL | |
| Keywords | Keywords not found |
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