Examination of n - T9 conditions required by N = 50, 82, 126 waiting points in r-process

Nguyen Duy Ly,Nguyen Ngoc Duy,Nguyen Kim Uyen,Vinh N T Pham

Figure 7. The r-process abundances of isotopes calculated using the nn − T9 conditions based on the AME, DZ10, FRDM, and KTUY mass data sets. Notice that the calculated abundances are upscaled by a factor of 1000 to normalize with the A = 130 peak of the Solar abundance which is taken from [59] (black dots with error bars). The yellow shaded areas indicate the differences among the abundances based on the different models. The thin lines are to guide the eyes at the A ≈ 80, 130, and 190 peaks.