Physics – Nuclear Physics – Nuclear Theory
Scientific paper
Sep 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004rpao.conf...11c&link_type=abstract
THE r-PROCESS The Astrophysical Origin of the Heavy Elements and Related Rare Isotope Accelerator Physics. Proceedings of the Fi
Physics
Nuclear Physics
Nuclear Theory
2
Scientific paper
The astrophysical r-process is thought to be responsible for the creation of more than half of the elements heavier than iron. An explanation of the nuclide abundances requires information on masses, which are best obtained through direct measurements. The Canadian Penning Trap (CPT) mass spectrometer at Argonne National Laboratory has completed the measurement of 26 neutron-rich Ba, La, Ce, and Pr isotopes approaching the r-process path. The results of these measurements and their potential impact on the r-process are presented in this paper.
Barber C. R.
Boudreau C.
Buchinger F.
Clark Adam J.
Crawford Evan J.
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