Some remarks on the Bel-Robinson Tensor
Janusz Garecki (University of Szczecin)

TL;DR
This paper discusses the physical interpretation of the Bel-Robinson tensor in standard General Relativity, emphasizing its derivation from Bianchi identities and its relation to gravitational energy-momentum in normal coordinates.
Contribution
It clarifies the Bel-Robinson tensor's interpretation without auxiliary structures, linking it to fundamental geometric identities and gravitational energy in GR.
Findings
The Bel-Robinson tensor arises from Bianchi identities.
It is connected to differences in gravitational energy-momentum.
The interpretation is consistent within standard GR without extra assumptions.
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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