More Like this

1. Laser cooling of antihydrogen atoms

   https://doi.org/10.1038/s41586-021-03289-6  

   Baker, C. J.; Bertsche, W.; Capra, A.; Carruth, C.; Cesar, C. L.; Charlton, M.; Christensen, A.; Collister, R.; Mathad, A. Cridland; Eriksson, S.; et al (April 2021, Nature)

   null (Ed.)

   Abstract The photon—the quantum excitation of the electromagnetic field—is massless but carries momentum. A photon can therefore exert a force on an object upon collision 1 . Slowing the translational motion of atoms and ions by application of such a force 2,3 , known as laser cooling, was first demonstrated 40 years ago 4,5 . It revolutionized atomic physics over the following decades 6–8 , and it is now a workhorse in many fields, including studies on quantum degenerate gases, quantum information, atomic clocks and tests of fundamental physics. However, this technique has not yet been applied to antimatter. Here we demonstrate laser cooling of antihydrogen 9 , the antimatter atom consisting of an antiproton and a positron. By exciting the 1S–2P transition in antihydrogen with pulsed, narrow-linewidth, Lyman-α laser radiation 10,11 , we Doppler-cool a sample of magnetically trapped antihydrogen. Although we apply laser cooling in only one dimension, the trap couples the longitudinal and transverse motions of the anti-atoms, leading to cooling in all three dimensions. We observe a reduction in the median transverse energy by more than an order of magnitude—with a substantial fraction of the anti-atoms attaining submicroelectronvolt transverse kinetic energies. We also report the observation of the laser-driven 1S–2S transition in samples of laser-cooled antihydrogen atoms. The observed spectral line is approximately four times narrower than that obtained without laser cooling. The demonstration of laser cooling and its immediate application has far-reaching implications for antimatter studies. A more localized, denser and colder sample of antihydrogen will drastically improve spectroscopic 11–13 and gravitational 14 studies of antihydrogen in ongoing experiments. Furthermore, the demonstrated ability to manipulate the motion of antimatter atoms by laser light will potentially provide ground-breaking opportunities for future experiments, such as anti-atomic fountains, anti-atom interferometry and the creation of antimatter molecules. 

   more » « less
2. Four ppm measurement of the antihydrogen ground-state hyperfine splitting

   https://doi.org/10.1038/s41586-026-10556-x  

   Akbari, R; de_Araujo_Azevedo, L O; Baker, C J; Bertsche, W; Bhatt, N M; Bonomi, G; Capra, A; Carli, I; L_Cesar, C; Charlton, M; et al (May 2026, Nature)

   Abstract The hydrogen atom is a touchstone for the foundations, evolution and frontiers of quantum theory^1–9. Key spectral lines of this atom have been determined to remarkable precision^10,11. Our research focuses on the study of antihydrogen, the antimatter counterpart of hydrogen. We test fundamental symmetries of nature (such as simultaneous charge conjugation, parity inversion, and time reversal or CPT symmetry) through precision comparisons of these atomic systems¹². Recent 1S–2S spectroscopic measurements on trapped antihydrogen have achieved relative precisions of parts per trillion (refs. ^13,14). However, the ground-state hyperfine splitting, which is sensitive to the internal structure of the antiproton, has only been measured to 400 parts per million (ppm). Here we report a 4 ppm measurement of the antihydrogen ground-state hyperfine splitting energya_1S, advancing the state-of-the-art precision¹⁵by two orders of magnitude. From microwave spectroscopy experiments with roughly 24,000 anti-atoms, we determine$${a}_{1{\rm{S}}}/h=\mathrm{1,420,404.8}\pm 1.1(\mathrm{stat.})\pm 5.6\,(\mathrm{sys.})\,\text{kHz}$$ $a_{1S}/h=\mathrm{1,420,404.8}\pm 1.1\left(\mathrm{stat.}\right)\pm 5.6\left(\mathrm{sys.}\right)\text{kHz}$ in a 1-T magnetic field, consistent with expectations for hydrogen¹¹. At this level, our measurement is sensitive to the internal structure of the antiproton, which contributes at about 40 ppm and is approaching the limit of existing theoretical analyses¹⁶. The gains we report are the product of marked advances in magnetic trap field control, stabilization and characterization; anti-atom spin-state manipulation; and improved antihydrogen accumulation rate¹⁷. 

   more » « less
3. Ion-chain sympathetic cooling and gate dynamics

   https://doi.org/10.1103/PhysRevApplied.22.044033  

   Paul, A; Noel, C (October 2024, Physical Review Applied)

   Sympathetic cooling is a technique often employed to mitigate motional heating in trapped-ion quantum computers. However, choosing system parameters such as number of coolants and cooling duty cycle for optimal gate performance requires evaluating trade-offs between motional errors and other slower errors such as qubit dephasing. The optimal parameters depend on cooling power, heating rate, and ion spacing in a particular system. In this study, we aim to analyze best practices for sympathetic cooling of long chains of trapped ions using analytical and computational methods. We use a case study to show that optimal cooling performance is achieved when coolants are placed at the center of the chain and provide a perturbative upper bound on the cooling limit of a mode given a particular set of cooling parameters. In addition, using computational tools, we analyze the trade-off between the number of coolant ions in a chain and the center-of-mass mode heating rate. We also show that cooling as often as possible when running a circuit is optimal when the qubit coherence time is otherwise long. These results provide a roadmap for how to choose sympathetic cooling parameters to maximize circuit performance in trapped-ion quantum computers using long chains of ions. Published by the American Physical Society2024 

   more » « less
4. Adiabatic expansion cooling of antihydrogen

   https://doi.org/10.1103/PhysRevResearch.6.L032065  

   Ahmadi, M; Alves, B_X R; Baker, C J; Bertsche, W; Capra, A; Cohen, S; Torkzaban, C; Cesar, C L; Charlton, M; Collister, R; et al (September 2024, Physical Review Research)

   Magnetically trapped antihydrogen atoms can be cooled by expanding the volume of the trap in which they are confined. We report a proof-of-principle experiment in which antiatoms are deliberately released from expanded and static traps. Antiatoms escape at an average trap depth of $0.08\pm 0.01\mathrm{K}$ (statistical errors only) from the expanded trap while they escape at average depths of $0.22\pm 0.01$ and $0.17\pm 0.01\mathrm{K}$ from two different static traps. (We employ temperature-equivalent energy units.) Detailed simulations qualitatively agree with the escape times measured in the experiment and show a decrease of $38\%$ (statistical $\text{error}<0.2\%$ ) in the mean energy of the population after the trap expansion without significantly increasing antiatom loss compared to typical static confinement protocols. This change is bracketed by the predictions of one-dimensional and three-dimensional semianalytic adiabatic expansion models. These experimental, simulational, and model results are consistent with obtaining an adiabatically cooled population of antihydrogen atoms that partially exchanged energy between axial and transverse degrees of freedom during the trap expansion. This result is important for future antihydrogen gravitational experiments which rely on adiabatic cooling, and it will enable antihydrogen cooling beyond the fundamental limits of laser cooling. Published by the American Physical Society2024 

   more » « less
5. Simulated optical molasses cooling of trapped antihydrogen

   https://doi.org/10.1088/1361-6455/adaf88  

   Walsh, Spencer J; Rasmussen, C Ø; Robicheaux, F (February 2025, Journal of Physics B: Atomic, Molecular and Optical Physics)

   Abstract We theoretically and computationally investigate the cooling of antihydrogen, $\overline{\text{H}}$ , using optical molasses cooling. This updates the results in Donnanet al(2013J. Phys. B: At. Mol. Opt. Phys.46025302) to the current capabilities of the ALPHA experiment. Through Monte Carlo simulation, we show that $\overline{\text{H}}$ s do not give the standard cooling even in an ideal optical molasses because of their small mass and large transition frequency. For optical molasses cooling in the ALPHA trap, the photons are constrained to travel in one direction only. It is only through the phase space mixing in the trap that cooling in all directions can be achieved. We explore the nontrivial role that laser intensity plays in the cooling. We also investigate the possibility for simultaneously cooling atoms in either of the trapped ground states. 

   more » « less