Preliminary bounds of the gravitational Local Position Invariance from Solar System planetary precessions
Lorenzo Iorio

TL;DR
This paper derives bounds on the Whitehead parameter , testing gravitational Local Position Invariance using Solar System planetary precessions, and finds no evidence for deviations from General Relativity within current measurement limits.
Contribution
It provides the first bounds on from planetary precession data and discusses how future missions could improve these constraints.
Findings
Bound on : || 5.8 7
Ratio of perihelion precessions constrains to zero
Current bounds are comparable to future mission sensitivities
Abstract
In the framework of the Parameterized Post-Newtonian (PPN) formalism, we calculate the long-term Preferred Location (PL) effects, proportional to the Whitehead parameter , affecting all the Keplerian orbital elements of a localized two-body system, apart from the semimajor axis . They violate the gravitational Local Position Invariance (LPI), fulfilled by General Relativity (GR). We obtain preliminary bounds on by using the latest results in the field of the Solar System planetary ephemerides. The non-detection of any anomalous perihelion precession for Mars allows us to indirectly infer . \textcolor{black}{Such a bound is close to the constraint, of the order of , expected from the future BepiColombo mission to Mercury. As a complementary approach, the PL effects should be explicitly included in the dynamical models fitted to…
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