The initial mass function (IMF) is a term commonly used to describe the statistical distribution function for the initial masses of stars. Its physical interpretation is that the number of stars with masses in the range is .
If the primary mechanism through which stars accumulate mass is Bondi accretion, then this function can be estimated analytically. We recall that in Bondi accretion the mass accretion rate scales as the mass squared
Solving this ODE yields
where is the initial seed mass at the beginning of the accretion, and is some constant that is independent of . The above relation can also be written in the following way
Hence at a constant time
Assuming that the number of stars is conserved, we can use
Combining the two relations yields
This value is similar to the Salpeter IMF obtained from observations.