Radiating charged rotating metric in de Sitter space in retarded time coordinates and the energy-momentum tensor

Details Radiating charged rotating metric in de Sitter space in retarded time coordinates and the energy-momentum tensor Radiating charged rotating metric in de Sitter space in retarded time coordinates and the energy-momentum tensor

Jan 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998cqgra..15..153x&link_type=abstract

Classical and Quantum Gravity, Volume 15, Issue 1, pp. 153-165 (1998).

Mathematics

Logic

10

Scientific paper

We show that the charged rotating metric in de Sitter space, derived by Mallett and used by Koberlein, is incorrect. Mallett's metric and his energy-momentum tensor do not satisfy the Einstein-Maxwell field equations with a cosmological term, in the non-radiating and radiating Kerr-Newman-de Sitter cases. We give the corresponding correct metric and the radiating energy-momentum tensor.

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