Relativistic theory for time and frequency transfer to order c^{-3}
Luc Blanchet, Christophe Salomon, Pierre Teyssandier, Peter Wolf

TL;DR
This paper extends the relativistic theory of time and frequency transfer to order 1/c^3, crucial for high-precision space experiments involving atomic clocks, by including higher-order Doppler, gravitational, and Sagnac effects.
Contribution
It provides the first comprehensive derivation of relativistic corrections up to order 1/c^3 for time and frequency transfer in space experiments, including two-way configurations.
Findings
Frequency transfer includes first and second-order Doppler effects, gravitational red-shift, and their mixture.
Time transfer accounts for Shapiro delay and first and second-order Sagnac corrections.
Higher-order corrections beyond 1/c^3 are negligible at current experimental accuracies.
Abstract
This paper is motivated by the current development of several space missions (e.g. ACES on International Space Station) that will fly on Earth orbit laser cooled atomic clocks, providing a time-keeping accuracy of the order of 5~10^{-17} in fractional frequency. We show that to such accuracy, the theory of frequency transfer between Earth and Space must be extended from the currently known relativistic order 1/c^2 (which has been needed in previous space experiments such as GP-A) to the next relativistic correction of order 1/c^3. We find that the frequency transfer includes the first and second-order Doppler contributions, the Einstein gravitational red-shift and, at the order 1/c^3, a mixture of these effects. As for the time transfer, it contains the standard Shapiro time delay, and we present an expression also including the first and second-order Sagnac corrections. Higher-order…
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.
