β+Decay Partial Half-Life of54Mnand Cosmic Ray Chronometry

Abstract
The weak β+ decay of the astrophysically significant radioisotope 54Mn has been observed. The energies of positrons from a chemically purified 54Mn source were measured using the APEX spectrometer at Argonne National Laboratory. We deduce a β+ decay branch of (1.20±0.26)×109, corresponding to a partial half-life of (7.1±1.5)×108yr. The implications of this value for cosmic-ray confinement times are discussed in light of recent satellite measurements of the cosmic-ray abundance of 54Mn.

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