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On the Bel - Robinson tensor

Ivor Robinson

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A completely symmetrical form of the Bel - Robinson (BR) tensor is shown to give rise, in n-dimensional Lorentzian space, to a gravitational density. For n = 4, a physical identification is proposed.


PACS

04.20.-q Classical general relativity

02.40.-k Geometry, differential geometry, and topology

MSC

83Cxx General relativity

30Fxx Riemann surfaces

Subjects

Mathematical physics

Gravitation and cosmology

Dates

Issue 1A (January 1997)



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