Measurement of the half-life of 60Fe for a Nearby Supernova Source

Details Measurement of the half-life of 60Fe for a Nearby Supernova Source Measurement of the half-life of 60Fe for a Nearby Supernova Source

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1016..463t&link_type=abstract

ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: The 10th International Symposium on Origin of Matter and Evolution of Galaxies: From

Physics

Supernova Remnants, Sources Of Radioactive Nuclei, Hyperfine Interactions And Isotope Effects, Jahn-Teller Effect

Scientific paper

A nearby supernova (SN) explosion in the past can be confirmed by the
detection of radioisotopes on Earth. The largest error of this estimate
is attributed to the half-life of 60Fe (18%).• We thus
propose a precise measurement of the half-life of 60Fe.

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