Abstract
The -decay half-life of is needed to employ this isotope as a cosmic ray chronometer. We have determined the partial half-life of for positron emission by counting a highly purified source of in GAMMASPHERE to search for the astrophysically interesting decay branch through the observation of coincident positron-annihilation rays. A careful analysis of 97 hours of source counting and 61 hours of background shows a net signal of back-to-back 511-511 keV coincident events. Based on this result, the branch for this decay mode is . The implications of this result for the cosmic-ray chronometer problem are discussed.
- Received 29 July 1997
DOI:https://doi.org/10.1103/PhysRevLett.79.4306
©1997 American Physical Society