Kleihaus, Burkhard and Kunz, Jutta and Radu, Eugen (2016) Charged, rotating black objects in Einstein–Maxwelldilaton theory in D ≥ 5. Entropy, 18 (5). p. 187. ISSN 10994300

 Published Version
Volltext (729Kb) 
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 [formula]) can be extended to the case of Einstein–Maxwelldilaton (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 [formula] horizon topology can also be studied (with [formula]). 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.
Item Type:  Article 

Additional Information:  Publiziert mit Hilfe des DFGgeförderten Open AccessPublikationsfonds der Carl von Ossietzky Universität Oldenburg. 
Uncontrolled Keywords:  black holes; higher dimensions; Einstein–Maxwelldilaton theory 
Subjects:  Science and mathematics Science and mathematics > Astronomy, cartography Science and mathematics > Physics 
Divisions:  Faculty of Mathematics and Science > Institute of Physics (IfP) 
Date Deposited:  18 Sep 2017 12:15 
Last Modified:  15 Dec 2017 11:10 
URI:  https://oops.unioldenburg.de/id/eprint/3238 
URN:  urn:nbn:de:gbv:715oops33191 
DOI:  10.3390/e18050187 
Nutzungslizenz: 
Actions (login required)
View Item 