13 FIG. 4: (Color online) Stellar reaction rates (including f*) for temperatures between T=0.1 and 3 GK. Compared are the temperature-dependences of this work obtained with different extrapolations based on different evaluations. Also shown are the predictions of the Hauser-Feshbach models NON-SMOKER [17, 44] and MOST 2005 [19], each with their original values and renormalized to reproduce our data at kT=25 keV (0.29 GK). It should be noted that above 0.29 GK all values (including the ones from the evaluations) are based on energy dependences derived from Hauser-Feshbach models.