General relativistic observables for the ACES experiment
Slava G. Turyshev, Nan Yu, and Viktor T. Toth

TL;DR
This paper presents a high-precision relativistic model for the ACES experiment on the ISS, enabling accurate time and frequency transfer measurements crucial for testing fundamental physics.
Contribution
It develops comprehensive relativistic coordinate transformations and models for ACES observables, including effects of Earth's oblateness and nongravitational forces, achieving sub-picosecond accuracy.
Findings
Model accuracy up to <1 ps for time transfer
Frequency transfer accuracy around 4×10^{-17}
Demonstrated the pseudo-inertial nature of the ACES reference frame
Abstract
We develop a high-precision model for relativistic observables of the Atomic Clock Ensemble in Space (ACES) experiment on the International Space Station (ISS). We develop all relativistic coordinate transformations that are needed to describe the motion of ACES in Earth orbit and to compute observable quantities. We analyze the accuracy of the required model as it applies to the proper-to-coordinate time transformations, light time equation, and spacecraft equations of motion. We consider various sources of nongravitational noise and their effects on ACES. We estimate the accuracy of orbit reconstruction that is needed to satisfy the ACES science objectives. Based on our analysis, we derive models for the relativistic observables of ACES, which also account for the contribution of atmospheric drag on the clock rate. We include the Earth's oblateness coefficient and the effects of…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
