Towards a network of 43Ca+ optical clocks for entanglement-enhanced metrology

21 May 2026, 12:00
30m
Festsaal, Theatersaal (ÖAW)

Festsaal, Theatersaal

ÖAW

Dr. Ignaz Seipel-Platz 2, 1010 Vienna (Mon-Wed) Sonnenfelsgasse 19, 1010 Vienna (Thu, Fri) (home symbol on map linked below)
Talk Session 14

Speaker

Ayush Agrawal (University of Oxford)

Description

Over the past few decades, advancements in optical atomic clocks have enabled measurements of time and frequency with unprecedented stability and systematic uncertainty [1,2]. Precision frequency comparisons between macroscopically separated clocks have applications in geodesy [3], probing variations in fundamental constants, and in dark matter searches [4]. Frequency comparisons between independent clock systems are limited by the standard quantum limit (SQL). In contrast, a set of N entangled atomic clocks can achieve a $\sqrt{N}$ stability improvement to surpass the SQL and approach the Heisenberg limit - the ultimate precision possible in quantum theory.

We previously demonstrated this enhancement in a network of two \ion{Sr}{88} clocks [5] on the 674 nm $5S_{1/2} \leftrightarrow 4D_{5/2}$ quadrupole transition using Ramsey spectroscopy, whose stability was mainly limited by the short probe duration of 20~ms due to magnetic field fluctuations. We are now setting up the next generation of the experiment wherein we map the remote Sr-Sr entanglement onto two $^{43}$Ca$^+$ ions. The 729 nm $^{43}$Ca$^+$ $\vert 4S_{1/2}, F=4, m_F=4 \rangle \leftrightarrow \vert 3D_{5/2}, F=4, m_F=3 \rangle$ optical clock transition is field-insensitive at 4.96 G, enabling probe durations at the excited state lifetime limit of $\sim$ 1 s (comparable to the start-of-the-art clocks [1]) and thus improve our stability.

We will present progress towards these clock experiments, including the setup of a 729 nm laser system locked to a high finesse cavity, as well as fibre noise cancellation on a 20~m fibre. We will further present some theoretical work on quantum metrology with Dicke states in the presence of spontaneous decay in larger networks of clocks.

[1] M. C. Marshall et al., Phys. Rev. Lett. 135, 033201 (2025).
[2] E. Oelker et al., Nature Photonics 13, 714–719 (2019).
[3] T. E. Mehlstaubler et al., Reports on Progress in Physics 81, 064401 (2018).
[4] M. S. Safronova et al., Rev. Mod. Phys. 90, 025008 (2018).
[5] B. C. Nichol et al., Nature 609, 689–694 (2022)

Author

Ayush Agrawal (University of Oxford)

Co-authors

Ms Ellis Ainley (University of Oxford) Mr Adam Martinez (University of Oxford) Ms Erin Malinowski (University of Oxford) Dr Jacob Blackmore (University of Oxford) Ms Marion Mallweger (University of Oxford) Dr David Nadlinger (University of Oxford) Dr Peter Drmota (University of Oxford) Dr Gabriel Araneda (University of Oxford) Dr David Hume (Time and Frequency Division, National Institute of Standards and Technology) Prof. David Lucas (University of Oxford) Dr Raghavendra Srinivas (University of Oxford)

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