Abstract
On the basis of the improved level scheme of it is demonstrated that the stellar s-process production as well as the stellar beta decay rate of that nucleus depend strongly on temperature. This behavior results from the completely different half-lives of the ground state and the isomer; since these states are coupled by induced transitions in the hot stellar photon bath, the effective half-life of is drastically reduced. The state at 838.64 keV was identified as the most efficient mediating level. Consequently, can no longer be considered as a chronometer for the age of the s process; instead, it can be interpreted as an s-process thermometer yielding a temperature range between 2.4× to 3.6× K.
- Received 27 September 1990
DOI:https://doi.org/10.1103/PhysRevC.44.2839
©1991 American Physical Society