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The reaction rates of the key stellar reaction of$^{14}$O($\alpha$,p)$^{17}$F have been reevaluated. It is thought that theprevious 1$^-$ assignment for the 6.15-MeV state is incorrect by a carefulreanalysis of the previous experimental data [J. G\'{o}mez del Campo {\it etal.}, Phys. Rev. Lett. {\bf 86}, 43 (2001)]. Most probably, the 6.286-MeV stateis the key 1$^-$ state and the 6.15-MeV state is a 2$^-$ one, and hence theresonance at $E_x$=6.286 MeV ($J^{\pi}$=1$^-$) actually dominates the reactionrates in the temperature region of astrophysical interests. The newlycalculated reaction rates for the $^{14}$O($\alpha$,p)$^{17}$F reaction arequite different from the previous ones, for instance, it's only about 1/6 ofthe previous value around 0.4 GK, while it's about 2.4 times larger than theprevious value around 2 GK. The astrophysical implications have been brieflydiscussed based on the present conclusions.

Reevaluation of the $^{14}$O($\alpha$,p)$^{17}$F Resonant Reaction Rate