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where <math>N_A \approx 6.022 \times 10^{23}</math> is the [[Avogadro constant]] and <math>\alpha</math> is the mean [[polarizability]] of a molecule.
where <math>N_A \approx 6.022 \times 10^{23}</math> is the [[Avogadro constant]] and <math>\alpha</math> is the mean [[polarizability]] of a molecule.


Substituting the molar refractivity into the [[Lorentz-Lorenz]] formula gives
Substituting the mola₡
:<math> A = \frac{N_A}{N} \frac{n^2 - 1}{n^2 + 2}, </math>
where <math>N</math> is the number of molecules per unit volume and <math>n</math> is the [[refractive index]]. The ratio <math>N_A / N</math> is simply the [[molar volume]] <math>V_m</math>. Evaluating the [[ideal gas law]] for 1 mole gives
:<math> V_m = \frac{N_A}{N} = \frac{R T}{p}, </math>
where <math>R</math> is the [[universal gas constant]], <math>T</math> is the [[absolute temperature]], and <math>p</math> is the pressure. Then the molar refractivity is
:<math> A = \frac{R T}{p} \frac{n^2 - 1}{n^2 + 2} </math>
:<math> A = \frac{R T}{p} \frac{n^2 - 1}{n^2 + 2} </math>



Revision as of 06:51, 18 February 2013

Molar refractivity, , is a measure of the total polarizability of a mole of a substance and is dependent on the temperature, the index of refraction, and the pressure.

The molar refractivity is defined as

where is the Avogadro constant and is the mean polarizability of a molecule.

Substituting the mola₡

For a gas, , so the molar refractivity can be approximated by

In SI units, has units of J mol−1 K−1, has units K, has no units, and has units of Pa, so the units of are m3 mol−1.

In terms of density, ρ molecular weight, M it can be shown that:

References

  • Born, Max, and Wolf, Emil, Principles of Optics: Electromagnetic Theory of Propagation, Interference and Diffraction of Light (7th ed.), section 2.3.3, Cambridge University Press (1999) ISBN 0-521-64222-1