A Magic Wavelength Trap for Ultracold KRb
POSTER
Abstract
Ultracold dipolar molecules provide tunable long-range, anisotropic interactions that enable the study of a multitude of spin-motion models, where spin is encoded in two rotational states of the molecule. To explore the novel quantum phases and dynamics predicted for such systems [1,2], long rotational coherence times are crucial. While one-body dephasing can be suppressed through dynamical decoupling [1,2], magic traps offer native dephasing suppression by minimizing the differential polarizability between the two involved states.
Here we present the development of a magic wavelength trap detuned from the X-b transition of 40K87Rb. Rotationally magic optical traps have been realized for 87Rb133Cs [3] and 23Na40K [4]. Compared to magic angle traps [5], such traps allow for more flexible trap geometries. Our preliminary work confirms the existence of a magic wavelength around 30 GHz detuned from the X-b transition. By implementing a magic trap, we expect to permit second-scale coherence times which will enhance future studies of many-body spin dynamics.
[1] A. N. Carroll, et al., Science 388, 6745 (2025)
[2] C. Miller, et al., Nature 633, 332–337 (2024)
[3] P.D. Gregory, et al., Nature Physics 20, 415-421 (2024)
[4] R. Bause, et al., PRL 125, 023201 (2020)
[5] B. Neyenhuis, et al., Phys. Rev. Lett. 109, 230403 (2012)
Here we present the development of a magic wavelength trap detuned from the X-b transition of 40K87Rb. Rotationally magic optical traps have been realized for 87Rb133Cs [3] and 23Na40K [4]. Compared to magic angle traps [5], such traps allow for more flexible trap geometries. Our preliminary work confirms the existence of a magic wavelength around 30 GHz detuned from the X-b transition. By implementing a magic trap, we expect to permit second-scale coherence times which will enhance future studies of many-body spin dynamics.
[1] A. N. Carroll, et al., Science 388, 6745 (2025)
[2] C. Miller, et al., Nature 633, 332–337 (2024)
[3] P.D. Gregory, et al., Nature Physics 20, 415-421 (2024)
[4] R. Bause, et al., PRL 125, 023201 (2020)
[5] B. Neyenhuis, et al., Phys. Rev. Lett. 109, 230403 (2012)
*This work was supported by the US DOE, Office of Science, NQIS Research Centers, Quantum Systems Accelerator. Support is also acknowledged from NSF OMA-2016244, NSF PHY-2317149, AFOSR MURI, ARO MURI and NIST. A.N.C. acknowledges support from the NSF GRFP under grant number DGE 2040434.
Presenters
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Nathan Song
- JILA