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arxiv: 1607.02356 · v2 · submitted 2016-07-08 · 🌀 gr-qc · astro-ph.CO· hep-ph· hep-th

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Post-Newtonian parameter γ for multiscalar-tensor gravity with a general potential

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classification 🌀 gr-qc astro-ph.COhep-phhep-th
keywords generalgravitygammacasefieldsmultiscalar-tensorparameterpost-newtonian
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We compute the parametrized post-Newtonian parameter $\gamma$ in the case of a static point source for multiscalar-tensor gravity with completely general nonderivative couplings and potential in the Jordan frame. Similarly to the single massive field case $\gamma$ depends exponentially on the distance from the source and is determined by the length of a vector of non-minimal coupling in the space of scalar fields and its orientation relative to the mass eigenvectors. Using data from the Cassini tracking experiment, we estimate bounds on a general theory with two scalar fields. Our formalism can be utilized for a wide range of models, which we illustrate by applying it to nonminimally coupled Higgs SU(2) doublet, general hybrid metric-Palatini gravity, linear ($\Box^{-1}$) and quadratic ($\Box^{-2}$) nonlocal gravity.

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  1. First-order thermodynamics of multi-scalar-tensor gravity

    gr-qc 2026-04 unverdicted novelty 7.0

    Multi-scalar-tensor gravity admits an exact covariant thermodynamic interpretation as an imperfect fluid whose heat flux involves a coupling-derived factor χ and a residual gradient sector, yielding multi-field therma...