2009
DOI: 10.1103/physreva.80.022518
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Isotope shifts and hyperfine structure in the 555.8-nmS10P31l

Abstract: We apply our technique of using a Rb-stabilized ring-cavity resonator to measure the frequencies of various spectral components in the 555.8-nm 1 S 0 → 3 P 1 line of Yb. We determine the isotope shifts with 60 kHz precision, which is an order-of-magnitude improvement over the best previous measurement on this line. There are two overlapping transitions, 171 Yb͑1 / 2 → 3 / 2͒ and 173 Yb͑5 / 2 → 3 / 2͒, which we resolve by applying a magnetic field. We thus obtain the hyperfine constants in the 3 P 1 state of th… Show more

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Cited by 30 publications
(28 citation statements)
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“…In our case the enhanced absorption is manifest for the 556 nm beam intensity range of 18 I For the 171 Yb (F = 3/2) hyperfine transition with a nulled magnetic field, a very small perturbation to the line is seen that we attribute to the 173 Yb (F = 3/2) line. It is consistent with previous reports that the latter is within 3 MHz of the 171 Yb (F = 3/2) line and higher in frequency [39,40]. An inverted crossover resonance is again observed for 173 Yb (F = 5 2 → 5 2 ), however the contrast is significantly weaker than for 171 Yb.…”
Section: Saturated Absorption Spectroscopysupporting
confidence: 92%
“…In our case the enhanced absorption is manifest for the 556 nm beam intensity range of 18 I For the 171 Yb (F = 3/2) hyperfine transition with a nulled magnetic field, a very small perturbation to the line is seen that we attribute to the 173 Yb (F = 3/2) line. It is consistent with previous reports that the latter is within 3 MHz of the 171 Yb (F = 3/2) line and higher in frequency [39,40]. An inverted crossover resonance is again observed for 173 Yb (F = 5 2 → 5 2 ), however the contrast is significantly weaker than for 171 Yb.…”
Section: Saturated Absorption Spectroscopysupporting
confidence: 92%
“…Our measurements will also assist those searching for the 1 S 0 − 3 P 0 line(s) in 173 Yb, given the previously reported value for its transition frequency [16]. Furthermore, the absolute optical frequencies of the other 1 S 0 − 3 P 1 isotopic lines can be inferred from previously reported measurements [17][18][19].…”
Section: Introductionsupporting
confidence: 56%
“…Henceforth, denoted with 1 S 0 − 3 P 1 . Based on an absolute frequency measurement of the 1 S 0 − 3 P 1 transition in 176 Yb and the relevant isotopic shift [19], a previous estimate for the 1…”
Section: Introductionmentioning
confidence: 99%
“…) transition, which differ by ∼3MHz [55], much less than the Doppler broadening in the cell. This overlap can explain lower enhancement rates, as the production of 171 YbOH will deplete the available population of other reactants.…”
Section: Resultsmentioning
confidence: 95%