Orbital effects of spatial variations of fundamental coupling constants
arXiv:1104.5192 · doi:10.1111/j.1365-2966.2011.19421.x
Abstract
We deal with the effects induced on the orbit of a test particle revolving around a central body by putative spatial variations of fundamental coupling constants . In particular, we assume a dipole gradient for $ζ(\bds r)/\barζ$ along a generic direction $\bds{\hat{k}}$ in space. We analytically work out the long-term variations of all the six standard Keplerian orbital elements parameterizing the orbit of a test particle in a gravitationally bound two-body system. It turns out that, apart from the semi-major axis , the eccentricity , the inclination , the longitude of the ascending node , the longitude of pericenter and the mean anomaly undergo non-zero long-term changes. By using the usual decomposition along the radial (), transverse () and normal () directions, we also analytically work out the long-term changes and experienced by the position and the velocity vectors $\bds r$ and $\bds v$ of the test particle. It turns out that, apart from , all the other five shifts do not vanish over one full orbital revolution. In the calculation we do not use \textit{a-priori} simplifying assumptions concerning and . Thus, our results are valid for a generic orbital geometry; moreover, they hold for any gradient direction (abridged).
Latex2e, 20 pages, 1 figure, 7 tables. Version accepted by Monthly Notices of the Royal Astronomical Society (MNRAS). Error in the caption of Table 5 corrected. References updated
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