Beta decay of Lu180

The allowed-unhindered $\ensuremath{\beta}$ decay of $^{180}\mathrm{Lu}$ strongly suggests that the ${\frac{9}{2}}^{\ensuremath{-}}{[514]}_{p}$, ${\frac{7}{2}}^{\ensuremath{-}}{[514]}_{n}$ Nilsson orbitals are involved in the transition. As a result of this proposed interpretation, the ground state Nilsson configuration of $^{180}\mathrm{Lu}$ is most probably ${\frac{9}{2}}^{\ensuremath{-}}{[514]}_{p}$, ${\frac{1}{2}}^{\ensuremath{-}}{[510]}_{n}$ with ${K}^{\ensuremath{\pi}}={5}^{+}$, not ${\frac{7}{2}}^{+}[404]$, ${\frac{1}{2}}^{\ensuremath{-}}{[510]}_{n}$ with ${K}^{\ensuremath{\pi}}={3}^{\ensuremath{-}}$ as previously suggested.RADIOACTIVITY $^{180}\mathrm{Lu}$; $^{180}\mathrm{Hf}$ deduced levels, $J$, $\ensuremath{\pi}$. Calculated two-quasiparticle states $^{180}\mathrm{Hf}$.