Formation of ultracold<sup> 223</sup>Fr<sup>107</sup>Ag molecules with greatly enhanced sensitivity.
POSTER
Abstract
We theoretically studied the formation the 223Fr107Ag molecule from laser-cooled Fr and Ag atoms by performing fully relativistic electronic-structure calculations of ground and excited states to account for strong spin-dependent relativistic effects in this heavy molecule. We used coupled-cluster CCSD(T) and EOM-CCSD theory of the DIRAC computational suite.
In addition, we performed couple-channel calculations to describe the scattering between ultracold 223Fr and 107Ag atoms in an external magnetic field. In these simulations, we couple the nonzero electron and nuclear spins of these isotopes through spin-spin coupling due to molecular forces as well as atomic hyperfine and Zeeman interactions. We then predicted the nearest-neighbor level density of Feshbach resonances. These resonances can be used for magneto-association into ultracold weakly and strongly bound FrAg.
We also performed calculations of the dynamic polarizability of rotational states of FrAg in its ground ν=0 vibrational level of the X electronic state and located magic conditions assuming either linearly or circularly polarized light. Magic conditions occur when the polarizabilities of two rotational states are equal.
In addition, we performed couple-channel calculations to describe the scattering between ultracold 223Fr and 107Ag atoms in an external magnetic field. In these simulations, we couple the nonzero electron and nuclear spins of these isotopes through spin-spin coupling due to molecular forces as well as atomic hyperfine and Zeeman interactions. We then predicted the nearest-neighbor level density of Feshbach resonances. These resonances can be used for magneto-association into ultracold weakly and strongly bound FrAg.
We also performed calculations of the dynamic polarizability of rotational states of FrAg in its ground ν=0 vibrational level of the X electronic state and located magic conditions assuming either linearly or circularly polarized light. Magic conditions occur when the polarizabilities of two rotational states are equal.
*Work supported by Gordon and Betty Moore Foundation Grant No. GBMF12330 and the US NSF Grant No. PHY-2409425
Publication: J. Klos et al New J. Phys. 24 (2022) 025005
Presenters
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Jacek Klos
- University of Maryland College Park
- Physics/JQI/NIST, University of Maryland, College Park MD and Physics, Temple University, Philadelphia, PA