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?

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