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An issue with the classification of the scalar-tensor theories of gravity

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arxiv 1905.08177 v4 pith:AYDZCEPS submitted 2019-05-20 gr-qc astro-ph.COhep-th

classification gr-qcastro-ph.COhep-th
keywords scalar-tensortheoriesclassificationtheoryconformalconfusiondiscussiongiven
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In the bibliography a certain confusion arises in what regards to the classification of the gravitational theories into scalar-tensor theories and general relativity with a scalar field either minimally or non-minimally coupled to matter. Higher-derivatives Horndeski and beyond Horndeski theories that at first sight do not look like scalar-tensor theories only add to the confusion. To further complicate things, the discussion on the physical equivalence of the different conformal frames in which a given scalar-tensor theory may be formulated, makes even harder to achieve a correct classification. In this paper we propose a specific criterion for an unambiguous identification of scalar-tensor theories and discuss its impact on the conformal transformations issue. The present discussion carries not only pedagogical but also scientific interest since an incorrect classification of a given theory as a scalar-tensor theory of gravity may lead to conceptual issues and to the consequent misunderstanding of its physical implications.

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  1. Scalar-Tensor Gravity and DESI 2024 BAO data

    astro-ph.CO 2025-01 conditional novelty 6.0 of 10

    With Planck and DESI BAO data, the Brans-Dicke Galileon model prefers a nonzero Galileon term and yields H0 = 71.0 +1.5 -1.3 km/s/Mpc, consistent with SH0ES at 1.2 sigma.

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