Abstract
The components of the energy-momentum pseudotensors of Einstein, Tolman, Landau and Lifshitz, and Møller 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 Møller gives the same energy as given by that of the Einstein, Tolman or Landau and Lifshitz.
Similar content being viewed by others
References
Bondi H 1990Proc. R. Soc. London A427 249
Cooperstock F I and Sarracino R S 1978J. Phys. A11 877
Kovacs D 1985Gen. Relativ. Gravit. 17 927
Landau L D and Lifshitz E M 1985The classical theory of fields, (Oxford: Pergamon Press) p. 280
Lindquist R W, Schwartz R A and Misner C W 1965Phys. Rev. 137 B1364
Misner C W, Thorne K S and Wheeler J A 1973Gravitation (San Francisco: W. H. Freeman and Co.) p. 466
Møller C 1958Ann. Phys. (N Y) 4 347
Møller C 1961Ann. Phys. (N Y) 12 118
Novotny J 1987Gen. Relativ. Gravit. 19 1043
Palmer T N 1980Gen. Relativ. Gravit. 12 149
Vaidya P C 1951Proc. Indian Acad. Sci. A33 264
Vaidya P C 1952J. Univ. Bombay (India) 21 1
Vaidya P C 1953Nature (London) 171 260
Virbhadra K S 1990aPhys. Rev. D41 1086
Virbhadra K S 1990bPhys. Rev. D42 1066
Virbhadra K S 1990cPhys. Rev. D42 2919
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Virbhadra, K.S. Energy and momentum in Vaidya spacetime. Pramana - J. Phys. 38, 31–35 (1992). https://doi.org/10.1007/BF02847902
Received:
Revised:
Issue Date:
DOI: https://doi.org/10.1007/BF02847902