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Auteur principal: Toth, Viktor T.
Format: Preprint
Publié: 2025
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Accès en ligne:https://arxiv.org/abs/2501.06106
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author Toth, Viktor T.
author_facet Toth, Viktor T.
contents Building upon earlier work, we explore the limits of using a configuration of satellites to measure the trace of the gravitational gradient tensor using intersatellite laser ranging and timing observables without relying on high-precision external observables such as deep space radio navigation or astrometry with unrealistic accuracy. A refined model, calculated with extended numerical precision, confirms that exceptional sensitivity is possible, placing within reach observational tests of certain modified gravity theories (e.g., Yukawa terms, galileons) using heliocentric orbits in the vicinity of the Earth. The sensitivity of the experiment improves at larger heliocentric distances. A constellation placed at 30 astronomical units, still well within the domain of feasibility using available propulsion and deep space communication technologies, may approach sensitivities that are sufficient to detect not just the gravitational contribution of the interplanetary medium but perhaps even cosmological dark matter and dark energy constituents.
format Preprint
id arxiv_https___arxiv_org_abs_2501_06106
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Pushing limits: Probing new gravity using a satellite constellation
Toth, Viktor T.
General Relativity and Quantum Cosmology
Building upon earlier work, we explore the limits of using a configuration of satellites to measure the trace of the gravitational gradient tensor using intersatellite laser ranging and timing observables without relying on high-precision external observables such as deep space radio navigation or astrometry with unrealistic accuracy. A refined model, calculated with extended numerical precision, confirms that exceptional sensitivity is possible, placing within reach observational tests of certain modified gravity theories (e.g., Yukawa terms, galileons) using heliocentric orbits in the vicinity of the Earth. The sensitivity of the experiment improves at larger heliocentric distances. A constellation placed at 30 astronomical units, still well within the domain of feasibility using available propulsion and deep space communication technologies, may approach sensitivities that are sufficient to detect not just the gravitational contribution of the interplanetary medium but perhaps even cosmological dark matter and dark energy constituents.
title Pushing limits: Probing new gravity using a satellite constellation
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2501.06106