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Physical Review A

Laser cooling of the alkaline-earth-metal monohydrides: Insights from anab initiotheory study

Yufeng Gao, Tao Gao

Published Nov 10, 2014• 70 citations
Publisher

Abstract

The feasibility of laser cooling $M\mathrm{H}$ ($M=\mathrm{Be},\phantom{\rule{0.16em}{0ex}}\mathrm{Mg},\phantom{\rule{0.16em}{0ex}}\mathrm{Ca},\phantom{\rule{0.16em}{0ex}}\mathrm{Sr},\phantom{\rule{0.16em}{0ex}}\mathrm{and}\phantom{\rule{0.16em}{0ex}}\mathrm{Ba}$) is investigated using ab initio quantum chemistry. The ground state $X\phantom{\rule{0.16em}{0ex}}{}^{2}{\ensuremath{\Sigma}}^{+}$ and first excited state $A\phantom{\rule{0.16em}{0ex}}{}^{2}\ensuremath{\Pi}$ of $M\mathrm{H}$ species are calculated using the multireference configuration interaction (MRCI) level of theory. For $\mathrm{CaH}$, $\mathrm{SrH}$, and $\mathrm{BaH}$, the spin-orbit coupling effects are also taken into account in electronic structure calculations at the MRCI level. Calculated spectroscopic constants for $^{9}\mathrm{BeH}$, $^{24}\mathrm{MgH}$, $^{40}\mathrm{CaH}$, $^{86}\mathrm{SrH}$, and $^{138}\mathrm{BaH}$ show good agreement with available theoretical and experimental results. The permanent dipole moments and transition dipole moments (TDMs) of the $X\phantom{\rule{0.16em}{0ex}}{}^{2}{\ensuremath{\Sigma}}^{+}$ and $A\phantom{\rule{0.16em}{0ex}}{}^{2}\ensuremath{\Pi}$ states of $M\mathrm{H}$ species are also calculated at the MRCI level of theory, and they are in good agreement with previous theoretical results. With the potential energy curves and TDMs obtained, the highly diagonally distributed Franck-Condon factors ${f}_{00}\left({}^{9}\mathrm{BeH}:0.998{,}^{24}\mathrm{MgH}:0.954{,}^{40}\mathrm{CaH}:0.961{,}^{86}\mathrm{SrH}:0.978,\phantom{\rule{0.16em}{0ex}}\phantom{\rule{0.16em}{0ex}}\phantom{\rule{0.16em}{0ex}}\mathrm{and}\phantom{\rule{0.16em}{0ex}}\phantom{\rule{0.16em}{0ex}}\phantom{\rule{0.16em}{0ex}}\phantom{\rule{0.16em}{0ex}}{\phantom{\rule{0.16em}{0ex}}}^{138}\mathrm{BaH}:0.971\right)$ for the $A\phantom{\rule{0.16em}{0ex}}{}^{2}\ensuremath{\Pi}\left({v}^{\ensuremath{'}}=0\right)\ensuremath{\rightarrow}X\phantom{\rule{0.16em}{0ex}}{}^{2}{\ensuremath{\Sigma}}^{+}\left(v=0\right)$ transition are determined. Radiative lifetime calculations of the $A\phantom{\rule{0.16em}{0ex}}{}^{2}\ensuremath{\Pi}\left({v}^{\ensuremath{'}}=0\right)$ state (${}^{9}\mathrm{BeH}:82.0\phantom{\rule{0.16em}{0ex}}\mathrm{ns}$, ${}^{24}\mathrm{MgH}:48.6\phantom{\rule{0.16em}{0ex}}\mathrm{ns}$, ${}^{40}\mathrm{CaH}:33.3\phantom{\rule{0.16em}{0ex}}\mathrm{ns}$, ${}^{86}\mathrm{SrH}:33.2\phantom{\rule{0.16em}{0ex}}\mathrm{ns}$, and $^{138}\mathrm{BaH}$: 68.6 ns) are found to be short enough for rapid laser cooling. The proposed main cycling laser drives the $X\phantom{\rule{0.16em}{0ex}}{}^{2}{\ensuremath{\Sigma}}^{+}\left(v=0\right)\ensuremath{\rightarrow}A\phantom{\rule{0.16em}{0ex}}{}^{2}\ensuremath{\Pi}\left({v}^{\ensuremath{'}}=0\right)$ transition at wavelength ${\ensuremath{\lambda}}_{00}\left({}^{9}\mathrm{BeH}:497.2\phantom{\rule{0.16em}{0ex}}\mathrm{nm}{,}^{24}\mathrm{MgH}:525.5\phantom{\rule{0.16em}{0ex}}\mathrm{nm}{,}^{40}\mathrm{CaH}:675.4\phantom{\rule{0.16em}{0ex}}\mathrm{nm}{,}^{86}\mathrm{SrH}:740.3\phantom{\rule{0.16em}{0ex}}\mathrm{nm},\phantom{\rule{0.16em}{0ex}}\mathrm{and}\phantom{\rule{0.28em}{0ex}}{\phantom{\rule{0.16em}{0ex}}}^{138}\mathrm{BaH}:952.6\phantom{\rule{0.16em}{0ex}}\mathrm{nm}\right)$. The results demonstrate the possibility of laser cooling $M\mathrm{H}$ species, and provide a promising theoretical reference for further theoretical and experimental research on alkaline-earth-metal monohydrides.

DOI
10.1103/physreva.90.052506

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The feasibility of laser cooling MHM\mathrm{H}MH (M=Be,Mg,Ca,Sr,andBaM=\mathrm{Be},\phantom{\rule{0.16em}{0ex}}\mathrm{Mg},\phantom{\rule{0.16em}{0ex}}\mathrm{Ca},\phantom{\rule{0.16em}{0ex}}\mathrm{Sr},\phantom{\rule{0.16em}{0ex}}\mathrm{and}\phantom{\rule{0.16em}{0ex}}\mathrm{Ba}M=Be,Mg,Ca,Sr,andBa) is investigated using ab initio quantum chemistry. The ground state X2\ensuremathΣ+X\phantom{\rule{0.16em}{0ex}}{}^{2}{\ensuremath{\Sigma}}^{+}X2\ensuremathΣ+ and first excited state A2\ensuremathΠA\phantom{\rule{0.16em}{0ex}}{}^{2}\ensuremath{\Pi}A2\ensuremathΠ of MHM\mathrm{H}MH species are calculated using the multireference configuration interaction (MRCI) level of theory. For CaH\mathrm{CaH}CaH, SrH\mathrm{SrH}SrH, and BaH\mathrm{BaH}BaH, the spin-orbit coupling effects are also taken into account in electronic structure calculations at the MRCI level. Calculated spectroscopic constants for 9BeH^{9}\mathrm{BeH}9BeH, 24MgH^{24}\mathrm{MgH}24MgH, 40CaH^{40}\mathrm{CaH}40CaH, 86SrH^{86}\mathrm{SrH}86SrH, and 138BaH^{138}\mathrm{BaH}138BaH show good agreement with available theoretical and experimental results. The permanent dipole moments and transition dipole moments (TDMs) of the X2\ensuremathΣ+X\phantom{\rule{0.16em}{0ex}}{}^{2}{\ensuremath{\Sigma}}^{+}X2\ensuremathΣ+ and A2\ensuremathΠA\phantom{\rule{0.16em}{0ex}}{}^{2}\ensuremath{\Pi}A2\ensuremathΠ states of MHM\mathrm{H}MH species are also calculated at the MRCI level of theory, and they are in good agreement with previous theoretical results. With the potential energy curves and TDMs obtained, the highly diagonally distributed Franck-Condon factors f00(9BeH:0.998,24MgH:0.954,40CaH:0.961,86SrH:0.978,and138BaH:0.971){f}_{00}\left({}^{9}\mathrm{BeH}:0.998{,}^{24}\mathrm{MgH}:0.954{,}^{40}\mathrm{CaH}:0.961{,}^{86}\mathrm{SrH}:0.978,\phantom{\rule{0.16em}{0ex}}\phantom{\rule{0.16em}{0ex}}\phantom{\rule{0.16em}{0ex}}\mathrm{and}\phantom{\rule{0.16em}{0ex}}\phantom{\rule{0.16em}{0ex}}\phantom{\rule{0.16em}{0ex}}\phantom{\rule{0.16em}{0ex}}{\phantom{\rule{0.16em}{0ex}}}^{138}\mathrm{BaH}:0.971\right)f00​(9BeH:0.998,24MgH:0.954,40CaH:0.961,86SrH:0.978,and138BaH:0.971) for the A2\ensuremathΠ(v\ensuremath′=0)\ensuremath→X2\ensuremathΣ+(v=0)A\phantom{\rule{0.16em}{0ex}}{}^{2}\ensuremath{\Pi}\left({v}^{\ensuremath{'}}=0\right)\ensuremath{\rightarrow}X\phantom{\rule{0.16em}{0ex}}{}^{2}{\ensuremath{\Sigma}}^{+}\left(v=0\right)A2\ensuremathΠ(v\ensuremath′=0)\ensuremath→X2\ensuremathΣ+(v=0) transition are determined. Radiative lifetime calculations of the A2\ensuremathΠ(v\ensuremath′=0)A\phantom{\rule{0.16em}{0ex}}{}^{2}\ensuremath{\Pi}\left({v}^{\ensuremath{'}}=0\right)A2\ensuremathΠ(v\ensuremath′=0) state (9BeH:82.0ns{}^{9}\mathrm{BeH}:82.0\phantom{\rule{0.16em}{0ex}}\mathrm{ns}9BeH:82.0ns, 24MgH:48.6ns{}^{24}\mathrm{MgH}:48.6\phantom{\rule{0.16em}{0ex}}\mathrm{ns}24MgH:48.6ns, 40CaH:33.3ns{}^{40}\mathrm{CaH}:33.3\phantom{\rule{0.16em}{0ex}}\mathrm{ns}40CaH:33.3ns, 86SrH:33.2ns{}^{86}\mathrm{SrH}:33.2\phantom{\rule{0.16em}{0ex}}\mathrm{ns}86SrH:33.2ns, and 138BaH^{138}\mathrm{BaH}138BaH: 68.6 ns) are found to be short enough for rapid laser cooling. The proposed main cycling laser drives the X2\ensuremathΣ+(v=0)\ensuremath→A2\ensuremathΠ(v\ensuremath′=0)X\phantom{\rule{0.16em}{0ex}}{}^{2}{\ensuremath{\Sigma}}^{+}\left(v=0\right)\ensuremath{\rightarrow}A\phantom{\rule{0.16em}{0ex}}{}^{2}\ensuremath{\Pi}\left({v}^{\ensuremath{'}}=0\right)X2\ensuremathΣ+(v=0)\ensuremath→A2\ensuremathΠ(v\ensuremath′=0) transition at wavelength \ensuremathλ00(9BeH:497.2nm,24MgH:525.5nm,40CaH:675.4nm,86SrH:740.3nm,and138BaH:952.6nm){\ensuremath{\lambda}}_{00}\left({}^{9}\mathrm{BeH}:497.2\phantom{\rule{0.16em}{0ex}}\mathrm{nm}{,}^{24}\mathrm{MgH}:525.5\phantom{\rule{0.16em}{0ex}}\mathrm{nm}{,}^{40}\mathrm{CaH}:675.4\phantom{\rule{0.16em}{0ex}}\mathrm{nm}{,}^{86}\mathrm{SrH}:740.3\phantom{\rule{0.16em}{0ex}}\mathrm{nm},\phantom{\rule{0.16em}{0ex}}\mathrm{and}\phantom{\rule{0.28em}{0ex}}{\phantom{\rule{0.16em}{0ex}}}^{138}\mathrm{BaH}:952.6\phantom{\rule{0.16em}{0ex}}\mathrm{nm}\right)\ensuremathλ00​(9BeH:497.2nm,24MgH:525.5nm,40CaH:675.4nm,86SrH:740.3nm,and138BaH:952.6nm). The results demonstrate the possibility of laser cooling MHM\mathrm{H}MH species, and provide a promising theoretical reference for further theoretical and experimental research on alkaline-earth-metal monohydrides.
An optical scheme to create the simplest heteronuclear metal ultracold LiBe molecule is proposed based on ab initio quantum chemistry calculations. The potential energy curves, dipole moments, and transition dipole moments of $1\phantom{\rule{0.16em}{0ex}}^{2}\mathrm{\ensuremath{\Sigma}}^{+}, 2\phantom{\rule{0.16em}{0ex}}^{2}\mathrm{\ensuremath{\Sigma}}^{+}, 1\phantom{\rule{0.16em}{0ex}}^{2}\mathrm{\ensuremath{\Pi}}$, and $2\phantom{\rule{0.16em}{0ex}}^{2}\mathrm{\ensuremath{\Pi}}$ states are calculated using the multireference configuration interaction and large basis sets. The analytical functions deduced from the obtained curves are used to determine the rovibrational energy levels, the Franck-Condon factors, and the Einstein coefficients of the states through solving the Schr\"odinger equation of nuclear movement. The spectroscopic parameters are deduced with the obtained rovibrational energy levels. The Franck-Condon factors (f00:0.998,f11:0.986,f22:0.920)({f}_{00}:0.998, {f}_{11}:0.986, {f}_{22}:0.920)(f00​:0.998,f11​:0.986,f22​:0.920) for the $2\phantom{\rule{0.16em}{0ex}}^{2}\mathrm{\ensuremath{\Sigma}}^{+}\phantom{\rule{0.28em}{0ex}}(v=0)\ensuremath{\leftrightarrow}1\phantom{\rule{0.16em}{0ex}}^{2}\mathrm{\ensuremath{\Sigma}}^{+}\phantom{\rule{0.28em}{0ex}}({v}^{\ensuremath{'}}=0)$ transition are highly diagonally distributed, and the calculated radiative lifetime (74.87 ns) of the $2\phantom{\rule{0.16em}{0ex}}^{2}\mathrm{\ensuremath{\Sigma}}^{+}$ state is found to be short enough for rapid laser cooling. The results demonstrate that LiBe could be a very promising candidate for laser cooling and a three-cycle laser cooling scheme for the molecule has been proposed.
High Resolution Image Download MS PowerPoint Slide Alkaline-earth-metal monohydrides M H ( M = Be, Mg, Ca, Sr, Ba) have long been regarded as promising candidates toward laser cooling and trapping; however, their rich internal level structures that are amenable to magneto-optical trapping have not been completely explored. Here, we first systematically evaluated Franck–Condon factors of these alkaline-earth-metal monohydrides in the A 2 Π 1/2 ← X 2 Σ + transition, exploiting three respective methods (the Morse potential, the closed-form approximation, and the Rydberg–Klein–Rees method). The effective Hamiltonian matrix was introduced for MgH, CaH, SrH, and BaH individually in order to figure out their molecular hyperfine structures of X 2 Σ +, the transition wavelengths in the vacuum, and hyperfine branching ratios of A 2 Π 1/2 ( J ′ = 1/2,+) ← X 2 Σ + ( N = 1,−), followed by possible sideband modulation proposals to address all hyperfine manifolds. Lastly, the Zeeman energy level structures and associated magnetic g factors of the ground state X 2 Σ + ( N = 1,−) were also presented. Our theoretical results here not only shed more light on the molecular spectroscopy of alkaline-earth-metal monohydrides toward laser cooling and magneto-optical trapping but also can contribute to research in molecular collisions involving few-atom molecular systems, spectral analysis in astrophysics and astrochemistry, and even precision measurement of fundamental constants such as the quest for nonzero detection of electron’s electric dipole moment.
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The feasibility of laser cooling AlH and AlF is investigated using ab initio quantum chemistry. All the electronic states corresponding to the ground and lowest two excited states of the Al atom are calculated using multi-reference configuration interaction (MRCI) and the large AV6Z basis set for AlH. The smaller AVQZ basis set is used to calculate the valence electronic states of AlF. Theoretical Franck-Condon factors are determined for the A(1)Π→ X(1)Σ(+) transitions in both radicals and found to agree with the highly diagonal factors found experimentally, suggesting computational chemistry is an effective method for screening suitable laser cooling candidates. AlH does not appear to have a transition quite as diagonal as that in SrF (which has been laser cooled) but the A(1)Π→ X(1)Σ(+) transition transition of AlF is a strong candidate for cooling with just a single laser, though the cooling frequency is deep in the UV. Furthermore, the a(3)Π→ X(1)Σ(+) transitions are also strongly diagonal and in AlF is a practical method for obtaining very low final temperatures around 3 μK.