3 research outputs found

    Frequency comparisons and absolute frequency measurements of 171Yb+ single-ion optical frequency standards

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    We describe experiments with an optical frequency standard based on a laser cooled 171^{171}Yb+^+ ion confined in a radiofrequency Paul trap. The electric-quadrupole transition from the 2S1/2(F=0)^2S_{1/2}(F=0) ground state to the 2D3/2(F=2)^2D_{3/2}(F=2) state at the wavelength of 436 nm is used as the reference transition. In order to compare two 171^{171}Yb+^+ standards, separate frequency servo systems are employed to stabilize two probe laser frequencies to the reference transition line centers of two independently stored ions. The experimental results indicate a relative instability (Allan standard deviation) of the optical frequency difference between the two systems of σy(1000s)=51016\sigma_y(1000 {\rm s})=5\cdot 10^{-16} only, so that shifts in the sub-hertz range can be resolved. Shifts of several hertz are observed if a stationary electric field gradient is superimposed on the radiofrequency trap field. The absolute optical transition frequency of Yb+^+ at 688 THz was measured with a cesium atomic clock at two times separated by 2.8 years. A temporal variation of this frequency can be excluded within a 1σ1\sigma relative uncertainty of 4.410154.4\cdot 10^{-15} yr1^{-1}. Combined with recently published values for the constancy of other transition frequencies this measurement provides a limit on the present variability of the fine structure constant α\alpha at the level of 2.010152.0\cdot 10^{-15} yr1^{-1}.Comment: 12 pages, 5 figures, Proceedings of MPLP'04, Novosibirsk, August 22.-27., 200

    Coulomb energy contribution to the excitation energy in 229^{229}Th and enhanced effect of α\alpha variation

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    We calculated the contribution of Coulomb energy to the spacing between the ground and first excited state of 229^{229}Th nucleus as a function of the deformation parameter δ\delta. We show that despite the fact that the odd particle is a neutron, the change in Coulomb energy between these two states can reach several hundreds KeV.This means that the effect of the variation of the fine structure constant α=e2/c\alpha=e^2/\hbar c may be enhanced ΔUC/E104\Delta U_C/E \sim 10^4 times in the E=E=7.6 eV "nuclear clock" transition between the ground and first excited states in the 229^{229}Th nucleus.Comment: 6 pages,2 figure
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