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Some remarks on the Bel-Robinson Tensor

Authors
  • Garecki, Janusz
Type
Published Article
Publication Date
Mar 02, 2000
Submission Date
Mar 02, 2000
Identifiers
DOI: 10.1002/1521-3889(200111)10:11/12<911::AID-ANDP911>3.0.CO
arXiv ID: gr-qc/0003006
Source
arXiv
License
Unknown
External links

Abstract

In this paper we present our point of view on correct physical interpretation of the Bel-Robinson tensor within the framework of the standard General Relativity ({\bf GR}), i.e., within the framework of the {\bf GR} without supplementary elements like arbitrary vector field, distinguished tetrads field or second metric. We show that this tensor arises as a consequence of the Bianchi identities and, in a natural manner, it is linked to the differences of the canonical gravitational energy-momentum calculated in normal coordinates {\bf NC(P)}.

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