Magic wavelengths of the Sr ($5s^2\;^1\!S_0$--$5s5p\;^3\!P_1$) intercombination transition near the $5s5p\;^3\!P_1$--$5p^2\;^3\!P_2$ transition
Phys. Rev. A 105, 012821 (2022) Predicting magic wavelengths accurately requires precise knowledge of electric-dipole matrix elements of nearby atomic transitions. As a result, measurements of magic wavelengths allow us to test theoretical predictions for the matrix elements that frequently can not...
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08.11.2021
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Abstract | Phys. Rev. A 105, 012821 (2022) Predicting magic wavelengths accurately requires precise knowledge of
electric-dipole matrix elements of nearby atomic transitions. As a result,
measurements of magic wavelengths allow us to test theoretical predictions for
the matrix elements that frequently can not be probed by any other methods.
Here, we calculate and measure a magic wavelength near $473$ nm of the
$5s^2\,^1\!S_0 - 5s5p\,^3\!P_1$ intercombination transition of ^{88}$Sr.
Experimentally, we find $473.361(4)$ nm for $\Delta m=0$ ($\pi$ transition) and
$473.133(14)$ nm for $\Delta m=-1$ ($\sigma^{-}$ transition). Theoretical
calculations yield $473.375(22)$~nm and $473.145(20)$ nm, respectively. The
$^3\!P_1$ polarizability is dominated by the contributions to the $5p^2\,
^3\!P$ levels and excellent agreement of theory and experiment validates both
theoretical values of these matrix elements and estimates of their
uncertainties. |
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AbstractList | Phys. Rev. A 105, 012821 (2022) Predicting magic wavelengths accurately requires precise knowledge of
electric-dipole matrix elements of nearby atomic transitions. As a result,
measurements of magic wavelengths allow us to test theoretical predictions for
the matrix elements that frequently can not be probed by any other methods.
Here, we calculate and measure a magic wavelength near $473$ nm of the
$5s^2\,^1\!S_0 - 5s5p\,^3\!P_1$ intercombination transition of ^{88}$Sr.
Experimentally, we find $473.361(4)$ nm for $\Delta m=0$ ($\pi$ transition) and
$473.133(14)$ nm for $\Delta m=-1$ ($\sigma^{-}$ transition). Theoretical
calculations yield $473.375(22)$~nm and $473.145(20)$ nm, respectively. The
$^3\!P_1$ polarizability is dominated by the contributions to the $5p^2\,
^3\!P$ levels and excellent agreement of theory and experiment validates both
theoretical values of these matrix elements and estimates of their
uncertainties. |
Author | Barreiro, Julio T Ton, Khang Filin, Dmytro Safronova, Marianna S Kestler, Grady |
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BackLink | https://doi.org/10.1103/PhysRevA.105.012821$$DView published paper (Access to full text may be restricted) https://doi.org/10.48550/arXiv.2111.04812$$DView paper in arXiv |
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Snippet | Phys. Rev. A 105, 012821 (2022) Predicting magic wavelengths accurately requires precise knowledge of
electric-dipole matrix elements of nearby atomic... |
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SubjectTerms | Physics - Atomic Physics Physics - Quantum Gases Physics - Quantum Physics |
Title | Magic wavelengths of the Sr ($5s^2\;^1\!S_0$--$5s5p\;^3\!P_1$) intercombination transition near the $5s5p\;^3\!P_1$--$5p^2\;^3\!P_2$ transition |
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