Herein "f" is the Sun's spin frequency.
The radius R has to be taken around 0.94 R or 0.95 R according to different models.
The Dalsgaard model for the solar density shows a hyperbolic-like function, whereof the asymptotes intersect at about 0.98 R : at first, there occurs a very quick density increase from 10^-6g/cm³ at R, until 10^-2g/cm³ at nearly 0.95 R and next a slow, almost linear density increase until 1.5x10^2g/cm³ at the Sun’s center. On the other hand, S. Korzennik found that the highest value of the Sun’s rotation is located at about 0.94 R , where the corresponding density is 10^-2g/cm³.
What is your best guess to explain this relationship?