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In absorption spectroscopy the ratio of the transmitted light intensity to the incident light
intensity at a given frequency is called transmittance, of the sample:
|
(15) |
According to the Lambert-Beer law, the transmitted light intensity varies with the
sample length as
|
(16) |
where is an absorption cross section and is the number of molecules per volume
(concentration). Adequate units are: for , for , and and for
.
Another form of eq. (16) which is widely used in laboratory practice is
|
(17) |
where is the extinction coefficient and is a molar concentration :
|
(18) |
where is the Avogadro number,
. The appropriate
units are mole/liter () for and
for .
Each of the coefficient and can be determined from experimental data
|
(19) |
where the , and are function of the light frequency .
In case if the exponent factor
in eq.(16) is small compare
to unity the exponential function can be expanded over . Keeping in this
expansion only first two terms one comes to the important for practice particular case called
low optical density of the sample:
|
(20) |
Integrating the expression in eq.(20) over the light frequency within the
absorption peak, one obtains the integrated cross section
|
(21) |
where is the Einstein absorption coefficient and is the center of the molecular
absorption line.
Thus the Einstein coefficient can be directly determined from experiment.
Next: Spectral Line Shape
Up: Optical Transitions and Spectral
Previous: Einstein Coefficients
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Markus Hiereth
2005-01-20
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