Abstract

The problem of the proper formulation of the conservation laws of energy and linear momentum in general relativity is discussed. The Komar expression, taken as a generally covariant conservation law generator, is considered in light of the problem which Moller found with his energy-momentum complex. The conservation laws as formulated here from the Komar generator are shown to be devoid of such difficulties. Also, a generally covariant formulation of the conservation laws, which are differentiated from a covariant conservation-law generator, is effectively achieved without the necessity of introducing a tetrad structure. In this formulation the conservation lawsper se are noncovariant quantities; however, one may always return to the Komar generator and transform in a generally covariant manner any given conservation law, through its underlying symmetry representation, to any space-time co-ordinate system of interest. It is also possible, at least in some simple space-time systems, to formulate the energy and momentum when they are not rigorously conserved entities. Such expressions can have possible application, for example, in radiating gravitational systems.

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