The production yields of excited oxygen O(¹<i>D</i>) atoms from the near ultraviolet O₃ photolysis are essential quantities for atmospheric chemistry calculations because of its importance as major sources of hydroxyl (OH) radicals and nitric oxide (NO). Recently, new O(¹<i>D</i>) quantum yields from O₃ photolysis between 230 and 305 nm in the Hartley band region were reported, which are almost independent of the photolysis wavelength (0.88-0.93) and smaller than NASA/JPL-2000 recommendations (0.95 between 240 and 300 nm). In order to assess consequences of the new data of O(¹<i>D</i>) quantum yields on the stratospheric chemistry, the changes in stratospheric chemical partitioning and O₃ concentration are examined using a one-dimensional atmospheric model. Our steady state model simulations for 40° N in March indicate that the smaller O(¹<i>D</i>) quantum yields result in increases of stratospheric O₃ (up to ~2% in the upper stratosphere), which are attributed to the changes in HO_x, NO_x, and ClO_x abundance and their catalyzed O₃ loss rates.