Abstract
The components of the energy-momentum pseudotensors of Einstein, Tolman, Landau and Lifshitz, and Moller are evaluated for the Vaidya radiating spacetime. These pseudotensors are found to be traceless for this spacetime. The pseudotensors of Einstein and Tolman give exactly same result for all their components. Unlike in the case of the Kerr-Newman field, the pseudotensor of Moller gives the same energy as given by that of the Einstein, Tolman or Landau and Lifshitz.
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