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Clausius–Mossotti relation

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Through Electromagnetism, Mixture and Refractive index

εr−1εr+2=Nα3ε0

where

In the case that the material consists of a mixture of two or more species, the right hand side of the above equation would consist of the sum of the molecular polarizability contribution from each species, indexed by i in the following form:

εr−1εr+2=∑iNiαi3ε0

In the CGS system of units the Clausius–Mossotti relation is typically rewritten to show the molecular polarizability volume α′=α4πε0 which has units of volume [m3]. Confusion may arise from the practice of using the shorter name "molecular polarizability" for both α and α′ within literature intended for the respective unit system.

The Clausius–Mossotti relation assumes only an induced dipole relevant to its polarizability and is thus inapplicable for substances with a significant permanent dipole. It is applicable to gases such as N2, CO2, CH4 and H2 at sufficiently low densities and pressures. For example, the Clausius–Mossotti relation is accurate for N2 gas up to 1000 atm between 25 °C and 125 °C. Moreover, the Clausius–Mossotti relation may be applicable to substances if the applied electric field is at a sufficiently high frequencies such that any permanent dipole modes are inactive.

Lorentz–Lorenz equation

The Lorentz–Lorenz equation is similar to the Clausius–Mossotti relation, except that it relates the refractive index (rather than the dielectric constant) of a substance to its polarizability. The Lorentz–Lorenz equation is named after the Danish mathematician and scientist Ludvig Lorenz, who published it in 1869, and the Dutch physicist Hendrik Lorentz, who discovered it independently in 1878.

The most general form of the Lorentz–Lorenz equation is (in Gaussian-CGS units)

n2−1n2+2=4π3Nαm

where n is the refractive index, N is the number of molecules per unit volume, and αm is the mean polarizability. This equation is approximately valid for homogeneous solids as well as liquids and gases.

When the square of the refractive index is n2≈1, as it is for many gases, the equation reduces to:

n2−1≈4πNαm

or simply

n−1≈2πNαm

This applies to gases at ordinary pressures. The refractive index n of the gas can then be expressed in terms of the molar refractivity A as:

n≈1+3ApRT

where p is the pressure of the gas, R is the universal gas constant, and T is the (absolute) temperature, which together determine the number density N.

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