Local gravitational physics of the Hubble expansion
Sergei Kopeikin (University of Missouri, USA)

TL;DR
This paper investigates how the Hubble expansion influences local measurements of space, time, and light in the solar system, revealing a potential method to measure the Hubble constant through radio wave experiments.
Contribution
It introduces a local inertial coordinate system in an expanding universe and shows how Hubble expansion causes measurable effects on light propagation in the solar system.
Findings
Light exhibits a systematic blue shift proportional to Hubble constant
Standard models assume uniform light motion, conflicting with cosmological effects
Potential to measure Hubble constant via solar system radio experiments
Abstract
We study physical consequences of the Hubble expansion of FLRW manifold on measurement of space, time and light propagation in the local inertial frame. We analyse the solar system radar ranging and Doppler tracking experiments, and time synchronization. FLRW manifold is covered by global coordinates (t,y^i), where t is the cosmic time coinciding with the proper time of the Hubble observers. We introduce local inertial coordinates x^a=(x^0,x^i) in the vicinity of a world line of a Hubble observer with the help of a special conformal transformation. The local inertial metric is Minkowski flat and is materialized by the congruence of time-like geodesics of static observers being at rest with respect to the local spatial coordinates x^i. We consider geodesic motion of test particles and notice that the local coordinate time x^0=x^0(t) taken as a parameter along the world line of particle,…
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