Photo-nuclear reaction rates of ${}^{157,159}$Ho and ${}^{163,165}$Tm and their impact in the ${\hat{I}}^3$--process

Hao Cheng, Bao-Hua Sun, Li-Hua Zhu +8

Reliable photo-nuclear reaction rates at the stellar conditions are essential to understand the origin of the heavy stable neutron-deficient isotopes between ${}^{74}$Se and ${}^{196}$…