Normalized differential rotation profile according to the radius normalized by the radius at the top of the radiative zone, rt, for a 1 M⊙ subgiant model with log Teff = 3.70 and log L/L⊙ = 0.35. We compare the smooth profile given in Eq. (12)(red solid line) with the sharp variant given in Eq. (13)(green solid line).
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