Conserved charges of higher D Kerr-AdS spacetimes

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Deser S., Kanik I., Tekin B.

CLASSICAL AND QUANTUM GRAVITY, vol.22, no.17, pp.3383-3389, 2005 (SCI-Expanded) identifier identifier

  • Publication Type: Article / Article
  • Volume: 22 Issue: 17
  • Publication Date: 2005
  • Doi Number: 10.1088/0264-9381/22/17/001
  • Journal Indexes: Science Citation Index Expanded (SCI-EXPANDED), Scopus
  • Page Numbers: pp.3383-3389
  • Middle East Technical University Affiliated: Yes


Rotating solutions of cosmological Einstein gravity in D dimensions, R-mu v = (D - 1)Lambda g(mu v), have been constructed recently [1, 2], extending earlier A = 0 solutions of [3], themselves generalizations of the well-known D = 4 metrics of [4] and [5], and of [6] in D = 5. These geometries provide a useful application of our recent generalized 'conserved charge' definitions, which are also extensions-of the original ADM [7], and AD [9] charges-to cover wider classes of actions [9, 11]: we will compute the energy and angular momenta of these new solutions.