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arXiv:1406.4365 · Physical Review A

Mass scaling and nonadiabatic effects in photoassociation spectroscopy of ultracold strontium atoms

Mateusz Borkowski, Piotr Morzyński, R. Ciuryło, Paul S. Julienne, Mi Yan, B. J. DeSalvo, T. C. Killian

Published Sep 16, 2014• 40 citations
arXivHTMLPDF

Abstract

We report photoassociation spectroscopy of ultracold $^{86}\mathrm{Sr}$ atoms near the intercombination line and provide theoretical models to describe the obtained bound-state energies. We show that using only the molecular states correlating with the ${}^{1}{S}_{0}+{}^{3}{P}_{1}$ asymptote is insufficient to provide a mass-scaled theoretical model that would reproduce the bound-state energies for all isotopes investigated to date: $^{84}\mathrm{Sr},^{86}\mathrm{Sr}$, and $^{88}\mathrm{Sr}$. We attribute that to the recently discovered avoided crossing between the ${}^{1}{S}_{0}+{}^{3}{P}_{1}$ ${0}_{u}^{+}$ $({}^{3}{\ensuremath{\Pi}}_{u})$ and ${}^{1}{S}_{0}+{}^{1}{D}_{2}$ ${0}_{u}^{+}$ $({}^{1}{\ensuremath{\Sigma}}_{u}^{+})$ potential curves at short range and we build a mass-scaled interaction model that quantitatively reproduces the available ${0}_{u}^{+}$ and ${1}_{u}$ bound-state energies for the three stable bosonic isotopes. We also provide isotope-specific two-channel models that incorporate the rotational (Coriolis) mixing between the ${0}_{u}^{+}$ and ${1}_{u}$ curves which, while not mass scaled, are capable of quantitatively describing the vibrational splittings observed in experiment. We find that the use of state-of-the-art ab initio potential curves significantly improves the quantitative description of the Coriolis mixing between the two $\ensuremath{-}8$-GHz bound states in $^{88}\mathrm{Sr}$ over the previously used model potentials. We show that one of the recently reported energy levels in $^{84}\mathrm{Sr}$ does not follow the long-range bound-state series and theorize on the possible causes. Finally, we give the Coriolis-mixing angles and linear Zeeman coefficients for all of the photoassociation lines. The long-range van der Waals coefficients ${C}_{6}({0}_{u}^{+})=3868(50)$ a.u. and ${C}_{6}({1}_{u})=4085(50)$ a.u. are reported.

DOI
10.1103/physreva.90.032713

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We report photoassociation spectroscopy of ultracold 86Sr^{86}\mathrm{Sr}86Sr atoms near the intercombination line and provide theoretical models to describe the obtained bound-state energies. We show that using only the molecular states correlating with the 1S0+3P1{}^{1}{S}_{0}+{}^{3}{P}_{1}1S0​+3P1​ asymptote is insufficient to provide a mass-scaled theoretical model that would reproduce the bound-state energies for all isotopes investigated to date: 84Sr,86Sr^{84}\mathrm{Sr},^{86}\mathrm{Sr}84Sr,86Sr, and 88Sr^{88}\mathrm{Sr}88Sr. We attribute that to the recently discovered avoided crossing between the 1S0+3P1{}^{1}{S}_{0}+{}^{3}{P}_{1}1S0​+3P1​ 0u+{0}_{u}^{+}0u+​ (3\ensuremathΠu)({}^{3}{\ensuremath{\Pi}}_{u})(3\ensuremathΠu​) and 1S0+1D2{}^{1}{S}_{0}+{}^{1}{D}_{2}1S0​+1D2​ 0u+{0}_{u}^{+}0u+​ (1\ensuremathΣu+)({}^{1}{\ensuremath{\Sigma}}_{u}^{+})(1\ensuremathΣu+​) potential curves at short range and we build a mass-scaled interaction model that quantitatively reproduces the available 0u+{0}_{u}^{+}0u+​ and 1u{1}_{u}1u​ bound-state energies for the three stable bosonic isotopes. We also provide isotope-specific two-channel models that incorporate the rotational (Coriolis) mixing between the 0u+{0}_{u}^{+}0u+​ and 1u{1}_{u}1u​ curves which, while not mass scaled, are capable of quantitatively describing the vibrational splittings observed in experiment. We find that the use of state-of-the-art ab initio potential curves significantly improves the quantitative description of the Coriolis mixing between the two \ensuremath−8\ensuremath{-}8\ensuremath−8-GHz bound states in 88Sr^{88}\mathrm{Sr}88Sr over the previously used model potentials. We show that one of the recently reported energy levels in 84Sr^{84}\mathrm{Sr}84Sr does not follow the long-range bound-state series and theorize on the possible causes. Finally, we give the Coriolis-mixing angles and linear Zeeman coefficients for all of the photoassociation lines. The long-range van der Waals coefficients C6(0u+)=3868(50){C}_{6}({0}_{u}^{+})=3868(50)C6​(0u+​)=3868(50) a.u. and C6(1u)=4085(50){C}_{6}({1}_{u})=4085(50)C6​(1u​)=4085(50) a.u. are reported.
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This dissertation describes two-photon photoassociation to the least-bound vibrational level of the X1Σg+^1\Sigma_g^+1Σg+​ electronic ground state of the 86^{86}86Sr2_22​ dimer, which represents the first observation of this naturally occurring halo molecule. We measure the binding energy of this state to be Eb=83.00(7)(20)E_b=83.00(7)(20)Eb​=83.00(7)(20)\,kHz. Using the precise determination of the halo state binding energy and the universal theory for a very weakly-bound state on a potential that asymptotes to a van der Waals form, we determine sss-wave scattering lengths for all strontium isotopes. Our results are consistent with, but substantially more accurate than the previously determined values found from spectroscopic determination of long-range coefficients using other strontium isotopes. With a radial expectation value of ⟨r⟩≈21\langle r \rangle \approx 21⟨r⟩≈21\,nm the halo state extends well into the classically forbidden region, which results in a large sensitivity of the dimer binding energy to light near-resonant with a bound-bound transition on the metastable 1S0−3P1^1S_0-{^3P_1}1S0​−3P1​ potential. This suggests that 86^{86}86Sr may be a promising candidate for manipulating atomic interactions via optical coupling of the molecular bound states and for probing naturally occurring Efimov states. Furthermore, we observe novel multi-photon spectral loss features due to strong coupling and small detuning of the photoassociation lasers. Numerical simulations of a simple three-level model undergoing a simultaneous two-frequency drive, shows that solutions of the time-dependent Schr\"{o}dinger equation accurately reproduce these additional loss features. A Floquet analysis of this model, yields analytic formulas for predicting the AC Stark shift of the halo molecule. Additionally, we report on the current state and recent modifications of our ultracold neutral strontium apparatus with a particular emphasis on the installation of a 532532532\,nm optical lattice. Characterization of this laser system and applications are discussed for further investigation of the strontium-868686 halo molecule and additional photoassociation experiments.
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