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1997 Class. Quantum Grav. 14 A331-A333 doi: 10.1088/0264-9381/14/1A/025
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Abstract. 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 numbers: 0420, 0240
Print publication: Issue 1A (January 1997) |
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