¹³C(a,n)¹⁶O

Ciani et al. 2021

This rate comes after the ¹³C(a,n)¹⁶O LUNA measurement, which is the first direct measurement reaching the high energy edge of the Gamow Window (130<E<240 keV). LUNA data cover the energy range 230<Ecm<305 keV corresponding to alpha energy 305<Ea<400 keV. All the points have overall uncertainty lower than 20%. The S factor evaluation is performed by R Matrix using data from our work, Heil, Drotleff and Harissopoulos. This last dataset is rescaled by a factor of 1.37. Uncertainties correspond to 1 sigma range.

Further details in the paper published on PRL and supplemental material

Download “C13an_Ciani_etal_2021” 13Can_Ciani_2021-1.txt – Downloaded 299 times – 10.44 KB

Nuclear reaction rate in the MESA format:

Download “13C_an_CianiG_PRL_2021_MESA” 13C_an_CianiG_PRL_2021_MESA.txt – Downloaded 154 times – 4.22 KB