A comment on the new non-conventional gravitational mechanism proposed by Jaekel and Reynaud to accommodate the Pioneer anomaly
Lorenzo Iorio

TL;DR
This paper tests a gravitational mechanism proposed to explain the Pioneer anomaly, finding it inconsistent with planetary observations and thus unlikely to be the correct explanation.
Contribution
It critically evaluates a recent non-conventional gravitational model for the Pioneer anomaly against observational data, ruling out certain proposed potentials.
Findings
The proposed quadratic potential causes large perihelion shifts incompatible with observations.
The linear potential is ruled out by residual perihelion rate measurements.
The gravitational mechanism cannot account for the Pioneer anomaly without conflicting with planetary data.
Abstract
In this paper we put on the test the new mechanism of gravitational origin recently put forth by Jaekel and Reynaud in order to explain the Pioneer anomaly in the framework of their post-Einsteinian metric extension of general relativity. According to such a proposal, the secular part of the anomalous acceleration experienced by the twin spacecraft of about 1 nm s^-2 could be caused by an extra-potential \delta\Phi_P=c^2\chi r^2, with \chi=4 10^-8 AU^-2, coming from the second sector of the considered model. When applied to the motion of the planets of the Solar System, it would induce anomalous secular perihelion advances which amount to tens-hundreds of arcseconds per century for the outer planets. As for other previously proposed non-conventional gravitational explanations of the Pioneer anomaly, the answer of the latest observational determinations of the residual perihelion rates…
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Taxonomy
TopicsAstro and Planetary Science · Stellar, planetary, and galactic studies · Planetary Science and Exploration
