Solar System tests in Brans–Dicke and Palatini f(R)-theories

We compare Mercury’s precession test in standard general relativity, Brans–Dicke theories (BD), and Palatini f ( R ) -theories. We avoid post-Newtonian approximation and compute exact precession in these theories. We show that the well-known mathematical equivalence between Palatini f ( R ) -theorie...

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Bibliographic Details
Published in:European physical journal plus Vol. 135; no. 12; p. 951
Main Authors: Bonino, A., Camera, S., Fatibene, L., Orizzonte, A.
Format: Journal Article
Language:English
Published: Berlin/Heidelberg Springer Berlin Heidelberg 01-12-2020
Springer Nature B.V
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Summary:We compare Mercury’s precession test in standard general relativity, Brans–Dicke theories (BD), and Palatini f ( R ) -theories. We avoid post-Newtonian approximation and compute exact precession in these theories. We show that the well-known mathematical equivalence between Palatini f ( R ) -theories and a specific subset of BD theories does not extend to a really physical equivalence among theories since equivalent models still allow a different incompatible precession for Mercury depending on the solution one chooses. As a result one cannot use BD equivalence to rule out Palatini f ( R ) -theories. On the contrary, we directly discuss that Palatini f ( R ) -theories can (and specific models do) easily pass Solar System tests as Mercury’s precession.
ISSN:2190-5444
2190-5444
DOI:10.1140/epjp/s13360-020-00982-9