
The conservation laws are examined from the transformation properties of the Lagrangian. The energy-momentum complex obtained has mixed indices, ${{T}_{\ensuremath{\mu}}}^{\ensuremath{\nu}}$, whereas a symmetric quantity ${\mathcal{T}}^{\ensuremath{\mu}\ensuremath{\nu}}$ is required for the definition of angular momentum. Such a symmetric quantity has been constructed by Landau and Lifshitz. In the course of examining the relationship between these quantities, two hierarchies of complexes ${{T}_{(n)\ensuremath{\mu}}}^{\ensuremath{\nu}}$ and ${{\mathcal{T}}_{(n)}}^{\ensuremath{\mu}\ensuremath{\nu}}$ are constructed. Under linear coordinate transformations the former are tensor densities of weight ($n+1$) and the latter of weight ($n+2$). For $n=0$ these reduce to the canonical ${{T}_{\ensuremath{\mu}}}^{\ensuremath{\nu}}$ and the Landau-Lifshitz ${\mathcal{T}}^{\ensuremath{\mu}\ensuremath{\nu}}$, respectively.By requiring the energy-momentum complex to generate the coordinate transformations, and the total energy and momentum to form a free vector, one can identify the canonical complex ${{T}_{\ensuremath{\mu}}}^{\ensuremath{\nu}}$ as the appropriate quantity to describe the energy and momentum of the field plus matter. Similarly, by requiring the total angular momentum to behave as a free antisymmetric tensor, one can construct, in the usual manner, an appropriate quantity from ${{\mathcal{T}}_{(\ensuremath{-}1)}}^{\ensuremath{\mu}\ensuremath{\nu}}$. The angular momentum complex so defined differs from that proposed by Landau and Lifshitz as well as from an independent construction by Bergmann and Thomson.
classical field theory, relativity theory
classical field theory, relativity theory
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