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APS

Tune-out wavelength for the 1 s 2 s 3 S - 1 s 3 p 3 P transition of helium: relativistic effects

G. W. F. Drake, Jacob Manalo

Published Apr 1, 2017• 0 citations
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Related papers

Tune-out wavelength for the $\mathbf{1s2s\;^3S - 1s3p\;^3P}$ transition of helium: relativistic effects

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Bulletin of the American Physical Society•Jun 6, 2017•0 citations

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Tune-out wavelength for the 1s2s  3S−1s3p  3P\mathbf{1s2s\;^3S - 1s3p\;^3P}1s2s3S−1s3p3P transition of helium: relativistic effects
Accurate calculation of the 413 nm tune-out wavelength for 23^{\mathrm{3}}3S1_{\mathrm{1}}1​ state of helium
Tune-out Wavelength of 4\mathbf{^{4}}4He for the 1s2s\mathbf{1s2s}1s2s 3\mathbf{^{3}}3S - 1s3p\mathbf{1s3p}1s3p 3\mathbf{^{3}}3P Transition
The six longest tune-out wavelengths for the He(1s2s3S1e1s2s{\phantom{\rule{4pt}{0ex}}}^{3}{S}_{1}^{e}1s2s3S1e​) metastable state are determined by explicit calculation. The tune-out wavelength at 413.02 nm is expected to be sensitive to finite mass, relativistic, and quantum electrodynamic effects upon the transition matrix elements and its measurement would provide a nonenergy test of fundamental atomic structure theory.
Hyperfine Suppression of a 2  32\;^323S1_11​ -- 3  33\;^333P1_11​ Radiative Transition in Helium