Improved Laboratory Transition Probabilities for Nd ii and Application to the Neodymium Abundances of the Sun and Three Metal‐poor Stars

Radiative lifetimes, accurate to ±5%, have been measured for 168 odd-parity levels of Nd II using laser-induced fluorescence. The lifetimes are combined with branching fractions measured using Fourier-transform spectrometry to determine transition probabilities for over 700 lines of Nd II. This work is the largest-scale laboratory study to date of Nd II transition probabilities using modern methods. This improved data set is used to determine Nd abundances for the Sun and three metal-poor giant stars with neutron-capture enhancement: CS 22892-052, HD 115444, and BD +17°3248. In all four stars the line-to-line scatter is considerably reduced from earlier published results. The solar photospheric abundance is determined to be log (Nd) = 1.45 ± 0.01(σ = 0.05), which is in excellent agreement with meteoric data. The ratio of Nd/Eu is virtually identical in all three metal-poor Galactic halo stars. Furthermore, the newly determined stellar Nd abundances, in comparison with other heavy neutron-capture elements, are consistent with an r -process-only origin early in the history of the Galaxy. These more accurate Nd abundance determinations might help to constrain the predicted solar system r -process abundances, and suggest other elements for further neutron-capture abundance studies.