Fluorometer

Significance

Fluorescence quantum yield determination using relavitive method

One significant use of the fluorometer (or fluorimeter) is the determination of the fluorescence quantum yield. This is done using a relative method based on a reference compound of known quantum yield. The unknown sample and the reference sample are measured at the same excitation wavelengths and measurement conditions. The wavelength-integrated flourescent intensity of both materials are then used in the calculation:

<math>\phi = \phi_{reference} \frac {F_{sample} / A_{sample}} {F_{reference}/ A_{reference}} \left( \frac {n_{sample}} {n_{reference}} \right) ^2\,\!</math>

where

φ is the quantum yield

F= integrated fluorescence intensity

A= absorbance at excitation wavelength

n= refractive index

Optically dilute solution Intensity of excitation beam should be almost constant along excitation beam Fluorescence signal is proportional to intensity of excitation beam Intensity has to be the same for sample and reference Typically: A ≤ 0.02 over 1 cm pathlength From entrance face to center of cuvette: �A = 0.01

Intensity has changed only by 2% Depending on absorption spectrometer used, measurement of A in this range may not be accurate enough How to proceed? Measure A on higher concentration solution Dilute solution by (accurately) known factor Perform fluorescence measurement on diluted solutions

Choice of excitation wavelength Excitation wavelength should be within the absorption band of the compounds Same excitation wavelength to be used for reference and sample compounds Emission spectrum collected �on the long wavelength side �of the excitation wavelength �(to avoid strong scattered �light from excitation beam) In this test, we are using: �lexc = 350 nm Repeated measurements Prepare multiple dilutions Measure fluorescence emission spectrum of each solution Determine the slope of the line F/A for sample and reference Always a good idea to have multiple data points!

Deviations from linearity could indicate that emission was affected by reabsorption Reabsorption Absorption of the emitted light by the same solution before light exits cuvette More significant for compounds �with small Stokes shifts Reabsorption can appear �as a redshift (or decrease �in fluorescence intensity �on the short wavelength �portion of the spectrum) Effect can be minimized �by reducing concentration �of solution Corrected fluorescence spectra Detectors and gratings do not have the same efficiency at all wavelengths Results need to be corrected �by a factor that accounts �for wavelength response �of the instrument The contribution of the �solvent (Raman scattering) �and noise (dark counts) �should also be subtracted Sample Calculation F/A values n Sample (#1): 1.289 x 1010 cps/mA 1.3288 (methanol) Reference: 1.316 x 1010 cps/mA 1.4266 (cyclohexane)

(freference = 0.87)

<math>\phi = 0.87 * \frac {1.289} {1.316} * \left( \frac {1.3288} {1.4266} \right) ^2\,\!</math>

<math>\phi = \phi_{reference} \frac {F_{sample} / A_{sample}} {F_{reference}/ A_{reference}} \left( \frac {n_{sample}} {n_{reference}} \right) ^2\,\!</math>

External Links

Wikipedia:Fluorescence spectroscopy