Hyperfine quenching of the $2s^22p^{5}3s\ ^3P_2$ state of Ne-like ions

The many-body perturbation theory (RMBPT) is used to calculate energies and multipole matrix elements to evaluate hyperfine quenching of the $2s^22p^53s\ 3P_2$ state in Ne-like ions. In particular, the $^3P_2$ excited state decays to the $^1S_0$ ground state by M2 emission, while both $^1P_1$ and $^3P_1$ states decay to the ground-state by E1 emission, which is substantially faster. For odd-A nuclei, the hyperfine interaction induces admixtures of $^3P_1$ and $^1P_1$ states into the $^3P_2$ state, resulting in an increase of the $^3P_2$ transition rate and a corresponding reduction of the $^3P_2$ lifetime. We consider 22 Ne like ions with $Z$ = 14 - 94 and nuclear moment $I$ =1/2. We found that the largess hyperfine quenching contribution by a factor of 2 are for Ne-like $^{31}$P and $^{203}$Tl. The smallest (less than 1\%) induced contribution are the following Ne-like ions: $^{57}$Fe, $^{107}$Ag, $^{109}$Ag, $^{183}$W, and $^{187}$Os ions. For another 15 Ne-like ions the hyperfine quenching contribution is between 15\% and 35\%. Applications to x-ray line polarization of Ne-like lines is considered.