Testing Local Lorentz Invariance with Laser Tracking of the LAGEOS and LAGEOS II Satellites
David Lucchesi, Massimo Visco, Roberto Peron, José C. Rodriguez, Massimo Bassan, Giuseppe Pucacco, Luciano Anselmo, Graham Appleby, Marco Cinelli, Alessandro Di Marco, Marco Lucente, Carmelo Magnafico, Carmen Pardini, Feliciana Sapio
Abstract
Violations of Lorentz Invariance, a cornerstone of modern physics, are predicted by theories of quantum gravity and by extensions of General Relativity involving new vector or tensor fields. In the weak-field limit, such a violation would primarily manifest as a non-zero value for the post-Newtonian parameter $α_1$, which is identically zero in General Relativity. We present a new test of Local Lorentz Invariance by searching for this signature in the orbits of the LAGEOS and LAGEOS II satellites. By applying a Phase Sensitive Detection technique to the mean argument of latitude, derived from about 30 years of Satellite Laser Ranging data, we isolate the periodic signal potentially induced by a preferred reference frame aligned with the Cosmic Microwave Background. {Our analysis yields a new constraint $|α_1| \sim 2 \times 10^{-5}$. This result improves upon the previous best limit from Lunar Laser Ranging and provides the most stringent constraint to date on preferred-frame effects in Earth's gravity.}
