Laser cooling of molecules has so far been limited to species with a ²Σ⁺ ground electronic state, such as SrF, CaF, and YO. These molecules are chemically reactive, difficult to produce, and unstable in collisions. Molecules with a ¹Σ⁺ state, by contrast, are deeply bound and stable, but their cooling transitions lie in the deep ultraviolet. This work stands apart: its nearest neighbors in the archive are traps for atoms and molecules with ²Σ⁺ states, as well as studies of optical transitions in AlF and Cd.
A beam of cold AlF molecules was produced in a cryogenic buffer gas cell: laser ablation of an aluminum target in an NF₃ atmosphere yielded molecules that were cooled by collisions with helium at 3 K. After exiting the cell, the beam was slowed by a frequency-chirped laser over a 50 cm length and loaded into a magneto-optical trap. The trap operated on the A¹Π ← X¹Σ⁺ transition (227.5 nm) using four laser systems: two at the main frequency and two for repumping from vibrational levels v″=1 and v″=2. The magnetic field was generated by neodymium ring magnets with a gradient of 1.0 kG/cm.
The trap held about 6.4×10⁴ AlF molecules in rotational level J=1, with a peak density of 1.4×10⁶ cm⁻³. For J=2 and J=3, the number of molecules exceeded 10⁴. The cloud temperature was 14–16 mK, noticeably above the Doppler limit (2 mK) but typical for red detunings in molecular traps. The trap lifetime reached 27 ms with beam expansion to 13 mm. Switching between rotational levels was achieved by simply retuning the slowing and trapping laser frequencies.
This work differs from its neighbors in that it is the first to trap a molecule with a singlet ground state. Previous traps were limited to chemically aggressive radicals, whereas AlF is stable and deeply bound (6.9 eV). This opens the possibility of using the spin-forbidden a³Π ← X¹Σ⁺ transition for narrow-line cooling and precision spectroscopy, analogous to alkaline-earth atoms. Such a transition promises sub-millikelvin temperatures and precise measurements.
The next step is cooling AlF below 1 mK using the narrow a³Π ← X¹Σ⁺ line. This would allow loading molecules into optical dipole traps and lattices, where quantum simulations and precise measurements become possible. Also promising is extension to higher rotational levels and other molecules with a ¹Σ⁺ state, such as BH and TlF.
The method will impact quantum chemistry, precision spectroscopy, and the search for new physics beyond the Standard Model. Stable cold molecules could serve as platforms for qubits and sensors.
Build a second cooling stage on the a³Π ← X¹Σ⁺ transition and demonstrate loading into an optical dipole trap. Assess losses from collisions and photoionization at higher densities.
For molecular physics, the key unsolved problem is achieving quantum degeneracy and controlled collisions of chemically stable molecules. This work solves the initial trapping problem, but questions about collisional losses and precise control of internal states remain open.
This section is addressed to the author of the paper and their colleagues. Neighbouring works were found by meaning-based search across our archive, not by word overlap. We do not review: we show the field around the work.
What the work does
The work demonstrates a magneto-optical trap for AlF molecules on the A¹Π ← X¹Σ⁺ transition near 227.5 nm. The molecules were produced in a cryogenic buffer gas cell, slowed by a chirped laser, and captured in a trap with a magnetic field gradient of 1.0 kG/cm. About 6×10⁴ molecules were held at the J=1 level at a temperature of 14–16 mK with a lifetime of up to 27 ms.
Where its strength is
For the first time, a molecule with a singlet ground state ¹Σ⁺ has been trapped, opening the way to using the spin-forbidden transition a³Π ← X¹Σ⁺ for narrow-line cooling and precision spectroscopy, analogous to alkaline-earth atoms.
Where it could go next
Worth trying
Why this may matter
Trapping stable molecules with a singlet ground state opens the path to a new class of quantum systems for precise measurements and studies of fundamental interactions, where the chemical stability of AlF may offer advantages over the radicals currently used.
Nearby works in our archive
The archive is sparse around this work: the closest review is only 0.55, against a usual 0.64. It looks like few have drilled nearby.
AlF is found in space: both stable ²⁷AlF in the shell of the star IRC +10216 and radioactive ²⁶AlF in the remnant of an ancient explosion. The same molecule trapped in the lab serves as an indicator of nucleosynthesis in astrophysics.