New Astrophysical Reaction Rate for the   $^{12}\textrm{C}(\alpha,\gamma)^{16}\textrm{O}$ Reaction
  A new astrophysical reaction rate for $^{12}$C($\alpha,\gamma$)$^{16}$O has been evaluated on the basis of a global R-matrix fitting to the available experimental data. The reaction rates of $^{12}$C($\alpha,\gamma$)$^{16}$O for stellar temperatures between 0.04 $\leq$ $T_9$ $\leq$ 10 are provided in a tabular form and by an analytical fitting expression. At $T_9$ = 0.2, the reaction rate is (7.83 $\pm$ 0.35)$\times10^{15}$ $\rm{cm^3 mol^{-1} s^{-1}}$, where stellar helium burning occurs. 
Z. D. An, Y. G. Ma, G. T. Fan, Y. J. Li, Z. P. Chen, Y. Y. Sun
nucl-th nucl-ex