Testing scalar-tensor theories and PPN parameters in Earth orbit
Andreas Sch\"arer, Raymond Ang\'elil, Ruxandra Bondarescu, Philippe, Jetzer, Andrew Lundgren

TL;DR
This paper calculates PPN parameters for scalar-tensor theories in Earth orbit, proposing a satellite experiment with atomic clocks to detect deviations from general relativity.
Contribution
It introduces a formalism for scalar-tensor theories in the Einstein frame and assesses the potential of satellite-based atomic clock experiments to test these theories.
Findings
Potential detection of PPN deviations at the level of 10^{-6} using existing atomic clock technology.
Satellite experiments could observe environment-dependent PPN parameters predicted by chameleon and symmetron theories.
Constraints on scalar-tensor theories from the Cassini experiment are incorporated into the analysis.
Abstract
We compute the PPN parameters and for general scalar-tensor theories in the Einstein frame, which we compare to the existing PPN formulation in the Jordan frame for alternative theories of gravity. This computation is important for scalar-tensor theories that are expressed in the Einstein frame, such as chameleon and symmetron theories, which can incorporate hiding mechanisms that predict environment-dependent PPN parameters. We introduce a general formalism for scalar-tensor theories and constrain it using the limit on given by the Cassini experiment. In particular we discuss massive Brans-Dicke scalar fields for extended sources. Next, using a recently proposed Earth satellite experiment, in which atomic clocks are used for spacecraft tracking, we compute the observable perturbations in the redshift induced by PPN parameters deviating from their general…
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