Absorbed-photon normalization in quantum-yield comparisons compares emitted events with the photons actually absorbed by the sample. The quantum yield uses absorbed photons as its denominator; equal incident optical power does not generally establish equal absorbed photon rates.[ref]
For monochromatic incident power , excitation wavelength and absorbance , the idealized absorbed photon flux is
This model assumes that the measured attenuation is attributed appropriately to absorption rather than unaccounted scattering or other optical losses. If background-corrected detected count rate is , where includes the specified collection and detection efficiency, then
Different emission spectra or collection conditions can change ; treating it as equal requires justification.
An original example uses equal incident powers at 400 and 600 nm, with absorbed fractions and . The absorbed photon rates have ratio
If count rates are 10,000 and 22,500 per second at equal detection efficiency, the inferred yield ratio is one. A raw brightness increase by 2.25 is entirely consistent with unchanged fluorescence quantum yield.
The weak-absorption approximation needs its stated range. At , the exact absorbed fraction is 0.5 while the approximation gives . Using it here would overestimate absorbed photons by about 39 percent and underestimate the inferred yield.
NIST's primary fluorescence-calibration guide separately treats emission response, excitation-beam intensity and relative quantum-yield measurement, including refractive-index corrections in its comparison model.[ref] Its framework motivates independently checking excitation and detection corrections. Inner filter effects, photobleaching and chemical changes can also defeat a naive comparison. Normalization corrects a specified measurement model; it should not force the Kasha-Vavilov rule to hold when corrected yields genuinely differ.

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