Molar refractivity

Molar refractivity, 
 
 
 
 
 R
 
 m
 
 
 
 
 {\displaystyle R_{m}}
 
, is a measure of the total <a href="/facts/Polarizability/0XRkXwUu">polarizability</a> of a <a href="/facts/Mole_(unit)/kCMFwCc0">mole</a> of a substance.
For a <a href="/facts/Perfect_gas/kghecDr8">perfect dielectric</a> which is made of one type of molecule, the molar refractivity is proportional to the polarizability of a single molecule of the substance. For real materials, intermolecular interactions (the effect of the induced dipole moment of one molecule on the field felt by nearby molecules) give rise to a density dependence.
The molar refractivity is commonly expressed as a sum of components, where the leading order is the value for a perfect dielectric, followed by the density-dependent corrections:

R
          
            m
          
        
        =
        A
        +
        B
        ⋅
        ρ
        +
        C
        ⋅
        
          ρ
          
            2
          
        
        +
        .
        .
        .
      
    
    {\displaystyle R_{m}=A+B\cdot \rho +C\cdot \rho ^{2}+...}

The coefficients 
 
 
 
 A
 ,
 B
 ,
 C
 ,
 .
 .
 .
 
 
 {\displaystyle A,B,C,...}
 
 are called the refractivity virial coefficients. Some research papers are dedicated to finding the values of the subleading coefficients of different substances. In other contexts, the material can be assumed to be approximately perfect, so that the only coefficient of interest is 
 
 
 
 A
 
 
 {\displaystyle A}
 
.
The coefficients depend on the wavelength of the applied field (and on the type and composition of the material), but not on <a href="/facts/Thermodynamics/q4hIx3yP">thermodynamic</a> <a href="/facts/State_variable/HNF1dCXu">state variables</a> such as <a href="/facts/Temperature/QyGe4gmj">temperature</a> or <a href="/facts/Pressure/eyc37GRG">pressure</a>.
The leading order (perfect dielectric) molar refractivity is defined as

A
        =
        
          
            
              4
              π
            
            3
          
        
        
          N
          
            A
          
        
        
          α
          
            
              m
            
          
        
        ,
      
    
    {\displaystyle A={\frac {4\pi }{3}}N_{A}\alpha _{\mathrm {m} },}

where 
 
 
 
 
 N
 
 A
 
 
 ≈
 6.022
 ×
 
 10
 
 23
 
 
 
 
 {\displaystyle N_{A}\approx 6.022\times 10^{23}}
 
 is the <a href="/facts/Avogadro_constant/SwajCq22">Avogadro constant</a> and 
 
 
 
 
 α
 
 
 m
 
 
 
 
 
 {\displaystyle \alpha _{\mathrm {m} }}
 
 is the mean <a href="/facts/Polarizability/0XRkXwUu">polarizability</a> of a molecule.
Substituting the molar refractivity into the <a href="/facts/Lorentz-Lorenz/JEAPwu7b">Lorentz-Lorenz</a> formula gives, for gasses

n
                
                  2
                
              
              −
              1
            
            
              
                n
                
                  2
                
              
              +
              2
            
          
        
        =
        A
        
          
            p
            
              R
              T
            
          
        
      
    
    {\displaystyle {\frac {n^{2}-1}{n^{2}+2}}=A{\frac {p}{RT}}}

where 
 
 
 
 n
 
 
 {\displaystyle n}
 
 is the <a href="/facts/Refractive_index/yjkzvgeE">refractive index</a>, 
 
 
 
 p
 
 
 {\displaystyle p}
 
 is the pressure of the gas, 
 
 
 
 R
 
 
 {\displaystyle R}
 
 is the <a href="/facts/Universal_gas_constant/RUXszrMH">universal gas constant</a>, and 
 
 
 
 T
 
 
 {\displaystyle T}
 
 is the (absolute) temperature; the <a href="/facts/Ideal_gas_law/Pphokwhf">ideal gas law</a> was used here to convert the particle density (appearing in the Lorentz-Lorenz formula) to pressure and temperature.
For a gas, 
 
 
 
 
 n
 
 2
 
 
 ≈
 1
 
 
 {\displaystyle n^{2}\approx 1}
 
, so the molar refractivity can be approximated by

A
        =
        
          
            
              R
              T
            
            p
          
        
        
          
            
              
                n
                
                  2
                
              
              −
              1
            
            3
          
        
        .
      
    
    {\displaystyle A={\frac {RT}{p}}{\frac {n^{2}-1}{3}}.}

The molar refractivity 
 
 
 
 A
 
 
 {\displaystyle A}
 
 does not depend on 
 
 
 
 T
 
 
 {\displaystyle T}
 
, 
 
 
 
 p
 
 
 {\displaystyle p}
 
 or 
 
 
 
 n
 
 
 {\displaystyle n}
 
, since they are not independent quantities.
In terms of <a href="/facts/Density/92p6hh9I">density</a> ρ and <a href="/facts/Molecular_weight/FWueGMed">molecular weight</a> M, it can be shown that:

A
        =
        
          
            M
            ρ
          
        
        
          
            
              
                n
                
                  2
                
              
              −
              1
            
            
              
                n
                
                  2
                
              
              +
              2
            
          
        
        ≈
        
          
            M
            ρ
          
        
        
          
            
              
                n
                
                  2
                
              
              −
              1
            
            3
          
        
        .
      
    
    {\displaystyle A={\frac {M}{\rho }}{\frac {n^{2}-1}{n^{2}+2}}\approx {\frac {M}{\rho }}{\frac {n^{2}-1}{3}}.}

Molar refractivity open-in-new

Molar refractivity