Lamb shift line-centre model

ID: lamb-shift-line-centre-model

Consider an original illustrative resonance model, with all numerical settings chosen here. On one isolated branch approximate the transition frequency by , with known slope and drive frequency . Choose , hence resonance field . This local linear model omits hyperfine structure and nonlinear level mixing; it is not the historical hydrogen Zeeman splitting calculation.
Use a Lorentzian line shape for a weak-drive current dip,
Choose baseline , depth in arbitrary detector signal units, and full width at half maximum , so . The half-depth points are ; this checks the factor of four. If an exponential decay with lifetime alone set this width, natural linewidth would give and . The chosen width is an explanatory input, not a measurement of a historical lifetime.
Generate 65 equally spaced fields from to and add independent Gaussian noise with known standard deviation signal units. A simultaneous nonlinear regression fit of gives , and . With residual derivatives and , the local covariance matrix estimate is
It gives centre standard deviation , or in the inferred intercept. This uses the stipulated noise variance and a local linear approximation, rather than treating the width as the centre error. Repeated noisy samples can locate a broad line's centre much more closely than its width.
Figure 1.
Chosen resonance line fit and zero-field intercept
. Original synthetic data and fitted Lorentzian current dip, with a separate linear field-to-frequency construction. All frequencies, fields, widths, signal units and noise are chosen for this example. The zero-field intercept is not a measured Lamb splitting. The displayed uncertainties are standard deviations under the stated model. Details.
Include a common magnetic calibration offset with standard deviation , a fractional gain error , and independent drive-frequency error . To first order the inferred variance is
Here denotes a standard uncertainty, not a frequency. The four contributions in are , , , and ; adding their squares gives . The calibration offset shifts all sampled fields together, so increasing the sample count cannot average it away. Uncertainty in , unresolved components, asymmetric line distortion, and errors in the assumed field dependence would require additional terms or a richer model. The historical inference requires the appropriate Zeeman splitting branches, rather than simply drawing a straight line through one resonance.

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