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Springer series in optical sciences/SPringer series in optical sciences

Magic Angle Line Narrowing in Optical Spectroscopy

Stephen Colby Rand, Alexander J. Wokaun, Ralph G. DeVoe, Richard G. Brewer

Published Jan 1, 1981• 42 citations
Publisher
DOI
10.1007/978-3-540-38609-4_12

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Magic-Angle Line Narrowing in Optical Spectroscopy

Stephen Colby Rand, Alexander J. Wokaun, Ralph G. DeVoe +1 more

Spin decoupling and line narrowing are observed for the first time in an optical transition, $^{3}H_{4}\ensuremath{\leftrightarrow}^{1}D_{2}$ of ${\mathrm{Pr}}^{3+}$ in La${\mathrm{F}}_{3}$ at 2\ifmmode^\circ\else\textdegree\fi{}K, with use of optical free-induction decay. The $^{19}\mathrm{F}$ nuclei, when irradiated by an appropriate rf field, undergo forced precession about an effective field at the magic angle in the rotating frame. The fluctuating $^{19}\mathrm{F}$-$^{19}\mathrm{F}$ dipolar interaction is thereby quenched and the optical linewidth drops from \ensuremath{\sim}10 to \ensuremath{\sim}2 kHz, as predicted in a theory of spin diffusion.

Physical Review Letters•Dec 17, 1979•66 citations

Narrow-line Cooling and Determination of the Magic Wavelength of Cd

Atsushi Yamaguchi, Marianna S. Safronova, Kurt Gibble +1 more

We experimentally and theoretically determine the magic wavelength of the (5s^{2})^{1}S_{0}-(5s5p)^{3}P_{0} clock transition of ^{111}Cd to be 419.88(14) and 420.1(7) nm. To perform Lamb-Dicke spectroscopy of the clock transition, we use narrow-line laser cooling on the ^{1}S_{0}-^{3}P_{1} transition to cool the atoms to 6 μK and load them into an optical lattice. Cadmium is an attractive candidate for optical lattice clocks because it has a small sensitivity to blackbody radiation and its efficient narrow-line cooling mitigates higher order light shifts. We calculate the blackbody shift, including the dynamic correction, to be fractionally 2.83(8)×10^{-16} at 300 K, an order of magnitude smaller than that of Sr and Yb. We also report calculations of the Cd ^{1}P_{1} lifetime and the ground state C_{6} coefficient.

arXiv:1909.07931•Physical Review Letters•Sep 13, 2019•64 citations
Spin decoupling and line narrowing are observed for the first time in an optical transition, $^{3}H_{4}\ensuremath{\leftrightarrow}^{1}D_{2}$ of Pr3+{\mathrm{Pr}}^{3+}Pr3+ in LaF3{\mathrm{F}}_{3}F3​ at 2\ifmmode^\circ\else\textdegree\fi{}K, with use of optical free-induction decay. The 19F^{19}\mathrm{F}19F nuclei, when irradiated by an appropriate rf field, undergo forced precession about an effective field at the magic angle in the rotating frame. The fluctuating 19F^{19}\mathrm{F}19F-19F^{19}\mathrm{F}19F dipolar interaction is thereby quenched and the optical linewidth drops from \ensuremath{\sim}10 to \ensuremath{\sim}2 kHz, as predicted in a theory of spin diffusion.
We experimentally and theoretically determine the magic wavelength of the (5s^{2})^{1}S_{0}-(5s5p)^{3}P_{0} clock transition of ^{111}Cd to be 419.88(14) and 420.1(7) nm. To perform Lamb-Dicke spectroscopy of the clock transition, we use narrow-line laser cooling on the ^{1}S_{0}-^{3}P_{1} transition to cool the atoms to 6 μK and load them into an optical lattice. Cadmium is an attractive candidate for optical lattice clocks because it has a small sensitivity to blackbody radiation and its efficient narrow-line cooling mitigates higher order light shifts. We calculate the blackbody shift, including the dynamic correction, to be fractionally 2.83(8)×10^{-16} at 300 K, an order of magnitude smaller than that of Sr and Yb. We also report calculations of the Cd ^{1}P_{1} lifetime and the ground state C_{6} coefficient.