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On Rastall gravity formulation as a f (R, Lm) and a f (R, T) theory

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EUROPEAN PHYSICAL JOURNAL PLUS
卷 138, 期 3, 页码 -

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SPRINGER HEIDELBERG
DOI: 10.1140/epjp/s13360-023-03845-1

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Rastall introduced a stress-energy tensor which changes the form of the field equations of General Relativity while preserving the number of degrees of freedom. The Rastall field equations can be interpreted as GR with a redefined SET or imply different physical consequences in the matter sector. The study investigates the direct derivation of the Rastall field equations from two f (R)-gravity extensions, revealing similarities between these theories but limitations in fully recovering the Rastall SET.
Rastall introduced a stress-energy tensor whose divergence is proportional to the gradient of the Ricci scalar. This proposal leads to a change in the form of the field equations of General Relativity, but it preserves the number of degrees of freedom. Rastall's field equations can be either interpreted as GR with a redefined SET, or it can imply different physical consequences inside the matter sector. We investigate limits under which the Rastall field equations can be directly derived from an action, in particular from two f (R)-gravity extensions: f (R, L-m) and f (R, T). We show that there are similarities between these theories, but the Rastall SET cannot be fully recovered from them, apart from certain particular cases here discussed. It is remarkable that a simple, covariant and invertible redefinition of the SET, as the one proposed by Rastall, is hard to be directly implemented in the action.

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