Stellar neutron capture on promethium: Implications for the s-process neutron density

R. Reifarth, C. Arlandini, M. Heil, F. Käppeler, P. V. Sedyshev, A. Mengoni, M. Herman, T. Rauscher, R. Gallino, C. Travaglio

Research output: Contribution to journalArticlepeer-review


The unstable isotope 147Pm represents an important branch point in the s-process reaction path. This paper reports on the successful determination of the stellar (n, γ) cross section via the activation technique. The experiment was difficult because the relatively short 147Pm half-life of 2.62 yr enforced the sample mass to be restricted to 28 ng or 1014 atoms only. By means of a modular, high-efficiency Ge Clover array the low induced activity could be identified in spite of considerable backgrounds from various impurities. Both partial cross sections feeding the 5.37 day ground state and the 41.3 day isomer in 147Pm were determined independently, yielding a total (n, γ) cross section of 709 ± 100 mbarn at a thermal energy of kT = 30 keV. The (n, γ) cross sections of the additional branch point isotopes 147Nd and 148Pm as well as the effect of thermally excited states were obtained by detailed statistical model calculations. The present results allowed considerably refined analyses of the s-process branchings at A = 147/148, which are probing the neutron density in the He-burning shell of low-mass asymptotic giant branch stars.

Original languageEnglish
Pages (from-to)1251-1262
Number of pages12
JournalThe Astrophysical Journal
Issue number2 I
Publication statusPublished - 10 Jan 2003
Externally publishedYes


  • Methods: laboratory
  • Nuclear reactions, nucleosynthesis, abundances
  • Stars: late-type


Dive into the research topics of 'Stellar neutron capture on promethium: Implications for the s-process neutron density'. Together they form a unique fingerprint.

Cite this