Imperial Ultracold Strontium Lab | Atom Interferometer Observatory and Network (AION)
This is the website for the Ultracold Strontium Lab at Imperial, which leads the UK’s AION collaboration (see our collaborators list).
We founded the Ultracold Strontium Lab and the Atom Interferometer Observatory and Network (AION) in 2021, driven by the goal to search for Ultra-Light Dark Matter and Gravitational Waves using clock-transition atom interferometry. In the lab we create interference between wave-packets of laser-cooled strontium atoms, split and recombined using the ultranarrow 1S0 to 3P0 transition — the same transition used to build the world’s most precise atomic clocks. We plan to scale this technology to a larger facility, with atom interferometers separated by ≫ 100 m (e.g. the AICE facility), ultimately hoping to see small wobbles in the relative phase of the interferometers due to passing gravitational waves or dark matter fields (see Figure 1).
In 2026, we demonstrated the first prototype clock-transition atom-interferometer detector at the lab scale [Nature 654, 622–628 (2026)]. Since then, we have demonstrated a record-high-flux source of cold strontium atoms [AVS Quantum Sci. 8, 033201 (2026)]. We are currently working towards Large Momentum Transfer (LMT), cavity-based squeezing, and continuous ultracold-atom sources – three techniques to improve the sensitivity of the detector.
Learn about the USOC project to develop ultra-precise, shock-resistant optical clocks using a continuous stream of ultracold strontium atoms in a moving optical lattice
Read about our latest work on clock-transition atom interferomtry, published in Nature
Learn more about the core vision of AION: a 4-stage project aiming to build gravitaional wave and dark matter detectors at the km-scale using cutting-edge techniques from quantum science.
The physics case for AION - our proposed sensitivity to dark matter and gravitational waves explained.