The charged rotating metric in de Sitter space, derived by Mallett and used by Koberlein, is shown incorrect. Mallett’s metric and his energy\|momentum tensor do not satisfy the Einstein\|Maxwell field equations with...The charged rotating metric in de Sitter space, derived by Mallett and used by Koberlein, is shown incorrect. Mallett’s metric and his energy\|momentum tensor do not satisfy the Einstein\|Maxwell field equations with a cosmological term in the nonradiating and radiating Kerr\|Newman\|de Sitter case. The corresponding correct metric and the radiating energy\|momentum tensor are given.展开更多
文摘The charged rotating metric in de Sitter space, derived by Mallett and used by Koberlein, is shown incorrect. Mallett’s metric and his energy\|momentum tensor do not satisfy the Einstein\|Maxwell field equations with a cosmological term in the nonradiating and radiating Kerr\|Newman\|de Sitter case. The corresponding correct metric and the radiating energy\|momentum tensor are given.
