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Bulletin of the American Physical Society

Time-dependent ac-Stark shift

Zenghu Chang

Published Jun 6, 2012• 0 citations
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Wavelength-dependent ac Stark shift of the S01‐P13 transition at 657nm in Ca

C. Degenhardt, Hardo Stoehr, Uwe Sterr +2 more

We have measured the ac Stark shift of the $4{s}^{2}\phantom{\rule{0.2em}{0ex}}^{1}S_{0}--4s4p\phantom{\rule{0.2em}{0ex}}^{3}P_{1}$ line in $^{40}\mathrm{Ca}$ for perturbing laser wavelengths between $780\phantom{\rule{0.3em}{0ex}}\mathrm{nm}$ and $1064\phantom{\rule{0.3em}{0ex}}\mathrm{nm}$ with a time domain Ramsey-Bord\'e atom interferometer. We found a zero crossing of the shift for the ${m}_{S}=0--{m}_{P}=0$ transition and $\ensuremath{\sigma}$ polarized perturbation at $800.8(22)\phantom{\rule{0.3em}{0ex}}\mathrm{nm}$. The data was analyzed by a model deriving the energy shift from known transition wavelengths and strengths. To fit our data, we adjusted the Einstein $A$ coefficients of the $4s3d\phantom{\rule{0.2em}{0ex}}^{3}D--4s4p\phantom{\rule{0.2em}{0ex}}^{3}P$ and $4s5s\phantom{\rule{0.2em}{0ex}}^{3}S--4s4p\phantom{\rule{0.2em}{0ex}}^{3}P$ fine structure multiplets. With these we can predict vanishing ac Stark shifts for the $^{1}S_{0}\phantom{\rule{0.2em}{0ex}}m=0--^{3}P_{1}\phantom{\rule{0.2em}{0ex}}m=1$ transition and ${\ensuremath{\sigma}}^{\ensuremath{-}}$ light at $983(12)\phantom{\rule{0.3em}{0ex}}\mathrm{nm}$ and at $735.5(20)\phantom{\rule{0.3em}{0ex}}\mathrm{nm}$ for the transition to the $^{3}P_{0}$ level.

arXiv:physics/0406018•Physical Review A•Aug 27, 2004•46 citations

AC-Stark Shift of Atomic Levels

Nikolai B. Delone, В. П. Крайнов

Springer eBooks•Jan 1, 2000•0 citations
We have measured the ac Stark shift of the 4s21S0−−4s4p3P14{s}^{2}\phantom{\rule{0.2em}{0ex}}^{1}S_{0}--4s4p\phantom{\rule{0.2em}{0ex}}^{3}P_{1}4s21S0​−−4s4p3P1​ line in 40Ca^{40}\mathrm{Ca}40Ca for perturbing laser wavelengths between 780nm780\phantom{\rule{0.3em}{0ex}}\mathrm{nm}780nm and 1064nm1064\phantom{\rule{0.3em}{0ex}}\mathrm{nm}1064nm with a time domain Ramsey-Bord\'e atom interferometer. We found a zero crossing of the shift for the mS=0−−mP=0{m}_{S}=0--{m}_{P}=0mS​=0−−mP​=0 transition and $\ensuremath{\sigma}$ polarized perturbation at 800.8(22)nm800.8(22)\phantom{\rule{0.3em}{0ex}}\mathrm{nm}800.8(22)nm. The data was analyzed by a model deriving the energy shift from known transition wavelengths and strengths. To fit our data, we adjusted the Einstein AAA coefficients of the 4s3d3D−−4s4p3P4s3d\phantom{\rule{0.2em}{0ex}}^{3}D--4s4p\phantom{\rule{0.2em}{0ex}}^{3}P4s3d3D−−4s4p3P and 4s5s3S−−4s4p3P4s5s\phantom{\rule{0.2em}{0ex}}^{3}S--4s4p\phantom{\rule{0.2em}{0ex}}^{3}P4s5s3S−−4s4p3P fine structure multiplets. With these we can predict vanishing ac Stark shifts for the 1S0m=0−−3P1m=1^{1}S_{0}\phantom{\rule{0.2em}{0ex}}m=0--^{3}P_{1}\phantom{\rule{0.2em}{0ex}}m=11S0​m=0−−3P1​m=1 transition and ${\ensuremath{\sigma}}^{\ensuremath{-}}$ light at 983(12)nm983(12)\phantom{\rule{0.3em}{0ex}}\mathrm{nm}983(12)nm and at 735.5(20)nm735.5(20)\phantom{\rule{0.3em}{0ex}}\mathrm{nm}735.5(20)nm for the transition to the 3P0^{3}P_{0}3P0​ level.