Mayer f-function

The Mayer f-function is an auxiliary function that often appears in the series expansion of thermodynamic quantities related to classical many-particle systems.[1] It is named after chemist and physicist Joseph Edward Mayer.

Definition

Consider a system of classical particles interacting through a pair-wise potential

V ( i , j ) {\displaystyle V(\mathbf {i} ,\mathbf {j} )}

where the bold labels i {\displaystyle \mathbf {i} } and j {\displaystyle \mathbf {j} } denote the continuous degrees of freedom associated with the particles, e.g.,

i = r i {\displaystyle \mathbf {i} =\mathbf {r} _{i}}

for spherically symmetric particles and

i = ( r i , Ω i ) {\displaystyle \mathbf {i} =(\mathbf {r} _{i},\Omega _{i})}

for rigid non-spherical particles where r {\displaystyle \mathbf {r} } denotes position and Ω {\displaystyle \Omega } the orientation parametrized e.g. by Euler angles. The Mayer f-function is then defined as

f ( i , j ) = e β V ( i , j ) 1 {\displaystyle f(\mathbf {i} ,\mathbf {j} )=e^{-\beta V(\mathbf {i} ,\mathbf {j} )}-1}

where β = ( k B T ) 1 {\displaystyle \beta =(k_{B}T)^{-1}} the inverse absolute temperature in units of energy−1 .

See also

  • Virial coefficient
  • Cluster expansion
  • Excluded volume

Notes

  1. ^ Donald Allan McQuarrie, Statistical Mechanics (HarperCollins, 1976), page 228