{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2026,4,9]],"date-time":"2026-04-09T02:46:38Z","timestamp":1775702798463,"version":"3.50.1"},"reference-count":29,"publisher":"MDPI AG","issue":"5","license":[{"start":{"date-parts":[[2016,5,16]],"date-time":"2016-05-16T00:00:00Z","timestamp":1463356800000},"content-version":"vor","delay-in-days":0,"URL":"https:\/\/creativecommons.org\/licenses\/by\/4.0\/"}],"content-domain":{"domain":[],"crossmark-restriction":false},"short-container-title":["Entropy"],"abstract":"<jats:p>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 \u2265 5     spacetime dimensions (with     0 \u2264 k \u2264    D - 5  2      ) can be extended to the case of Einstein\u2013Maxwell-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\u2013Perry black holes. Balanced charged black objects with      S  n + 1   \u00d7  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 &gt; 0     are black ringoids. The basic properties of EMd solutions are discussed for the special case of a Kaluza\u2013Klein value of the dilaton coupling constant. We argue that all features of these solutions can be derived from those of the vacuum seed configurations.<\/jats:p>","DOI":"10.3390\/e18050187","type":"journal-article","created":{"date-parts":[[2016,5,17]],"date-time":"2016-05-17T10:20:11Z","timestamp":1463480411000},"page":"187","update-policy":"https:\/\/doi.org\/10.3390\/mdpi_crossmark_policy","source":"Crossref","is-referenced-by-count":2,"title":["Charged, Rotating Black Objects in Einstein\u2013Maxwell-Dilaton Theory in D \u2265 5"],"prefix":"10.3390","volume":"18","author":[{"given":"Burkhard","family":"Kleihaus","sequence":"first","affiliation":[{"name":"Institut f\u00fcr Physik, Universit\u00e4t Oldenburg, Postfach 2503 D-26111 Oldenburg, Germany"}]},{"given":"Jutta","family":"Kunz","sequence":"additional","affiliation":[{"name":"Institut f\u00fcr Physik, Universit\u00e4t Oldenburg, Postfach 2503 D-26111 Oldenburg, Germany"}]},{"given":"Eugen","family":"Radu","sequence":"additional","affiliation":[{"name":"CIDMA, Departamento de Fisica, Universidade de Aveiro, Campus de Santiago, 3810-183 Aveiro, Portugal"}]}],"member":"1968","published-online":{"date-parts":[[2016,5,16]]},"reference":[{"key":"ref_1","doi-asserted-by":"crossref","first-page":"101101","DOI":"10.1103\/PhysRevLett.88.101101","article-title":"A rotating black ring solution in five dimensions","volume":"88","author":"Emparan","year":"2002","journal-title":"Phys. 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