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Conserved charges of higher D Kerr-AdS spacetimes
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Date
2005-09-07
Author
Deser, S
Kanik, I
Tekin, Bayram
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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.
Subject Keywords
Physics and Astronomy (miscellaneous)
URI
https://hdl.handle.net/11511/40239
Journal
CLASSICAL AND QUANTUM GRAVITY
DOI
https://doi.org/10.1088/0264-9381/22/17/001
Collections
Department of Physics, Article
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S. Deser, I. Kanik, and B. Tekin, “Conserved charges of higher D Kerr-AdS spacetimes,”
CLASSICAL AND QUANTUM GRAVITY
, pp. 3383–3389, 2005, Accessed: 00, 2020. [Online]. Available: https://hdl.handle.net/11511/40239.