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Main Authors: Lucchesi, David, Visco, Massimo, Peron, Roberto, Rodriguez, José C., Bassan, Massimo, Pucacco, Giuseppe, Anselmo, Luciano, Appleby, Graham, Cinelli, Marco, Di Marco, Alessandro, Lucente, Marco, Magnafico, Carmelo, Pardini, Carmen, Sapio, Feliciana
Format: Preprint
Published: 2025
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Online Access:https://arxiv.org/abs/2501.10588
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author Lucchesi, David
Visco, Massimo
Peron, Roberto
Rodriguez, José C.
Bassan, Massimo
Pucacco, Giuseppe
Anselmo, Luciano
Appleby, Graham
Cinelli, Marco
Di Marco, Alessandro
Lucente, Marco
Magnafico, Carmelo
Pardini, Carmen
Sapio, Feliciana
author_facet Lucchesi, David
Visco, Massimo
Peron, Roberto
Rodriguez, José C.
Bassan, Massimo
Pucacco, Giuseppe
Anselmo, Luciano
Appleby, Graham
Cinelli, Marco
Di Marco, Alessandro
Lucente, Marco
Magnafico, Carmelo
Pardini, Carmen
Sapio, Feliciana
contents 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.}
format Preprint
id arxiv_https___arxiv_org_abs_2501_10588
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Testing Local Lorentz Invariance with Laser Tracking of the LAGEOS and LAGEOS II Satellites
Lucchesi, David
Visco, Massimo
Peron, Roberto
Rodriguez, José C.
Bassan, Massimo
Pucacco, Giuseppe
Anselmo, Luciano
Appleby, Graham
Cinelli, Marco
Di Marco, Alessandro
Lucente, Marco
Magnafico, Carmelo
Pardini, Carmen
Sapio, Feliciana
General Relativity and Quantum Cosmology
83
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.}
title Testing Local Lorentz Invariance with Laser Tracking of the LAGEOS and LAGEOS II Satellites
topic General Relativity and Quantum Cosmology
83
url https://arxiv.org/abs/2501.10588