The symmetric tensor field in the relativistic theory of gravitation

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Scientific paper

The system of a self-gravitating scalar field is frequently used in inflationary cosmological models. In the present paper we study a more complicated system containing an extra linear tensor field ψik=ψki with minimal coupling. We determine five of the six free parameters that occur in the most general expression for the actionS ψ of this field. In doing so we assume that in flat space-time the field ψik must be invariant under gauge transformations. In a special case theS ψ found becomes a known expression for the action of a massless tensor field ψik. We compute the metric energy-momentum tensor that determines the contribution of ψik to the Einstein equations. We also exhibit the equations of motion of ψik in curved space-time.

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