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Time and Space

Time and Space is an international, peer-reviewed, open access journal on all aspects of time and space in physics published quarterly online by MDPI.

All Articles (6)

Clock Synchronization with Kuramoto Oscillators for Space Systems

  • Nathaniel Ristoff,
  • Hunter Kettering and
  • James Camparo

As space systems evolve towards cis-lunar missions and beyond, the demand for precise yet low-size, -weight, and -power (SWaP) clocks and synchronization methods becomes increasingly critical. We introduce a novel clock synchronization approach based on the Kuramoto oscillator model that facilitates the creation of an ensemble timescale for satellite constellations. Unlike traditional ensembling algorithms, the proposed Kuramoto method leverages nearest-neighbor interactions to achieve collective synchronization. This method simplifies the communication architecture and data-sharing requirements, making it well suited for dynamically connected networks such as proliferated low Earth orbit (pLEO) and lunar or Martian constellations, where intersatellite links may frequently change. Through simulations incorporating realistic noise models for small-scale atomic clocks, we demonstrate that the Kuramoto ensemble can yield an improvement in stability on the order of 1/√N, while mitigating the impact of constellation fragmentation and defragmentation. The results indicate that the Kuramoto oscillator-based algorithm can potentially deliver performance comparable to established techniques like Equal Weights Frequency Averaging (EWFA), yet with enhanced scalability and resource efficiency critical for future spaceborne PNT and communication systems.

15 January 2026

These diagrams show information flow for traditional ensembling algorithms (a) and a simple Kuramoto ensembling algorithm (b). The complexity of informational flow for traditional ensembling algorithms is apparent and increases geometrically as satellite constellations grow. Alternatively, the informational flow for a Kuramoto algorithm can be much simpler. Though a chain is shown, connecting the two end nodes (C0 and C9) turns the linear chain into a closed loop. Of course, one can create an ensemble by passing all of the information to a centralized node (e.g., a ground station) where ensemble computations are performed. Corrections for each ensemble member can then be “uploaded” to the constellation. Though different from what we have referred to as “traditional” ensembling, the complications of data flow (i.e., all ensemble members to ground and then ground to all ensemble members) are the same.

This paper presents a theoretical framework modeling space-time as a quantized elastic medium. This elastic model is not intended to replace general relativity, but to offer a complementary mechanical interpretation in the approximation of the weak gravitational field. The goal is not to redefine gravity, but to explore whether this elastic formalism can simplify certain aspects of space-time dynamics, provide new insights, and generate falsifiable predictions—particularly in contexts where analytical solutions in general relativity are difficult to obtain. As originally envisaged by A. Sakharov, who associated general relativity with the concept of space-time behaving like an elastic medium, this paper introduces the notion of the “elasther” and reinterprets gravitational effects, time dilation, and phenomena commonly attributed to dark energy and dark matter through analogies with established mechanical principles such as Hooke’s law, thermal expansion, and creep.

18 December 2025

Representation of the “elasther” in 4 dimensions in the framework of the model of the elastic medium made up of small quantum-dimensional beams (link with A Sakharov)—the dashed lines represent the deformations associated with time propagating at the speed of light arriving with a delay, and the instantaneous deformations related to space are represented in solid lines.

In vapor-cell atomic clocks, a buffer gas is employed to slow the collision rate of atoms with the vapor-cell’s walls, which dephases the atomic coherence and thereby contributes to the 0-0 hyperfine transition’s linewidth. However, the buffer gas also gives rise to a temperature-dependent pressure shift in the hyperfine transition, Δνhfs. As a consequence, the clock’s frequency develops a temperature dependence, manifesting as a clock environmental sensitivity, which can degrade the clock’s long-term frequency stability. To mitigate this problem, it is routine to employ a buffer-gas mixture in a vapor cell. With an appropriate choice of buffer gases, d[Δνhfs]/dT = 0 at a vapor temperature Tc, “zeroing out” the clock’s buffer-gas temperature sensitivity. Unfortunately, Tc depends on the exact mix of buffer-gas partial pressures, and if not properly achieved, Tc will be far from the vapor temperature that yields useful atomic clock signals, To. Therefore, understanding buffer-gas partial pressures in sealed vapor cells is crucial for optimizing a vapor cell clock’s performance, yet, to date, there have been no easy means for measuring buffer-gas partial pressures non-destructively in sealed glass vapor cells. Here, we demonstrate an optical technique that can accurately assess partial pressures in binary buffer-gas mixtures. Moreover, this technique is relatively simple and can be easily implemented.

24 October 2025

Experimental block diagram. A single VCSEL diode laser’s output is split between a reference and a measurement cell. Transmission is detected with a photodiode and recorded by an averaging oscilloscope for analysis.

The instabilities in time and frequency transfer systems, a form of residual noise, can contribute significantly to the total uncertainty in time or frequency comparisons. Understanding the characteristics of transfer instabilities is increasingly important with the new high-stability optical frequency standards being developed. First-difference statistics such as the rms Time Interval Error (TIErms), the Frequency Transfer Uncertainty (FTU), and ADEVS (a novel use of the Allan deviation equation) provide a more direct and accurate measure of residual noise than second-difference statistics such as the Allan Deviation (ADEV), the Modified Allan Deviation (MDEV), and the Time Deviation (TDEV). A unifying discussion on the use of existing first-difference statistics with residual noise, introduced individually in two previous publications, is presented here. Simulated noise data is then analyzed to illustrate the differences in the various statistics. Their strengths and weaknesses are discussed. The impact of pre-averaging phase (time) data is also shown.

8 June 2025

Simulate residual noise data in black and with a linear drift added in gray. The vertical axis represents the residual noise d in arbitrary units of time and the horizontal axis is the epoch t in arbitrary units of time. A linear drift of +4.5 × 10−4 d/t was added.

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Time Space - ISSN 2813-9526