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Determination of transit time distribution and Rabi frequency by applying regularized inverse on Ramsey spectra
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10.1063/1.2734476
/content/aip/journal/apl/90/17/10.1063/1.2734476
http://aip.metastore.ingenta.com/content/aip/journal/apl/90/17/10.1063/1.2734476
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Figures

Image of FIG. 1.
FIG. 1.

(Color online) (a) Since the surface has no other local minima near the global minimum point, precise values of Rabi frequencies are found without any ambiguity by applying a parabolic interpolation. (b) Transit time distribution of Cs atoms in KRISS-1 was obtained using our regularized inverse approach.

Image of FIG. 2.
FIG. 2.

(Color online) (a) Statistical uncertainty of quadratic Doppler shift (squares) and the Rabi frequencies (triangles and circles) due to the white noise in the Ramsey spectra. (b) Systematic uncertainty of quadratic Doppler shift at varying modulation depths.

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/content/aip/journal/apl/90/17/10.1063/1.2734476
2007-04-27
2014-04-24
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752b84549af89a08dbdd7fdb8b9568b5 journal.articlezxybnytfddd
Scitation: Determination of transit time distribution and Rabi frequency by applying regularized inverse on Ramsey spectra
http://aip.metastore.ingenta.com/content/aip/journal/apl/90/17/10.1063/1.2734476
10.1063/1.2734476
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