Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

The nucleosynthesis of sup 180 Ta

Thesis/Dissertation ·
OSTI ID:5097164
It has been proposed by Beer and Ward that the abundance of nature's rarest isotope, {sup 180}Ta, could be quantitatively accounted for in the standard stellar slow (s) and/or rapid (r) neutron-capture processes through the existence of small, previously unmeasured {beta}-branches which drain and feed the population of the t{sub {1/2}} = 5.5 hour isomer of {sup 180}Hf(BE81). We have conducted a series of experiments designed to measure these small {beta}-branches. We have: (1) measured the direct (isomer-to-isomer) 214-keV-endpoint {beta} branch from {sup 180}Hf{sup m} to {sup 180}Ta{sup m} to be f{sub {beta}} = 0.30 {plus minus} 0.07 {plus minus} 0.07% (KE87), (2) observed a new {gamma} ray in the decay of {sup 180}Hf{sup m} which indicated a small {beta}-branch of 0.023% to an excited state in {sup 180}Ta (KE85), (3) established a stringent limit of 0.023% on the fraction f{sub m} of {sup 180}Lu decays which populate {sup 180}Hf{sup m} (KE86), (4) sought to identify a possible high-spin, short-lived isomer of {sup 180}Lu, and established upper limits on its possible half-life (LE86), (5) established limits on the {sup 180}Ta{sup m} photodeexcitation cross-section via resonant and nonresonant processes (NO84a), and (6) calculated upper-limits on the life-time of {sup 180}Ta{sup m} in a stellar environment. Taken together, this body of work makes it unlikely that the Beer and Ward model can account for the observed solar-system abundance of {sup 180}Ta. Other possible production schemes are reviewed and directions for further research are suggested.
Research Organization:
Washington Univ., Seattle, WA (USA)
OSTI ID:
5097164
Country of Publication:
United States
Language:
English