﹩\mathrm{log}({R}_{2}/{R}_{1})﹩ as a function of ﹩{\rm{\Delta }}({\alpha }_{\mathrm{MLT}}^{-4/3})﹩ at various ages for 0.3 M_⊙ stellar models at α_MLT = 0.8–1.7 (Δ0.05). During the pre-main sequence, the trend decreases with age (see Equation (24)), eventually reaching levels of negligible radius inflation in the main sequence.