Published 1983 | Version v1
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β-decays of 180Hf/sup m/ and 180Lu and the origin of 180Ta

Description

We are interested in determining the nucleosynthetic mechanism responsible for the production of the naturally occurring isomer, 180Ta. An attractive idea is the suggestion by Beer and Ward that 180Ta may be produced in the standard s- and r-processes through previously undetected β-decay branches of 180Hf/sup m/ and 180Lu. The 5.5 hour, J/sup π/=8-180Hf isomer lies 204 keV above the long-lived J/sup π/=9- isomer in 180Ta; therefore an allowed Gammow-Teller β-transition should compete with the K-inhibited electromagnetic decays to the ground state rotational band of 180Hf. The 180Hf/sup m/ branching ratio to 180Ta, f/sub β/, need only be 3.1% to account for the 180Ta abundance by the s-process alone, while log-ft considerations predict a range of from 0.14% to 22%

Availability note (English)

MF available from INIS under the Report Number; Available from NTIS, PC A02/MF A01; 1 as DE83015733.

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Additional details

Publishing Information

Imprint Pagination
3 p.
Report number
DOE/ER/40048--65

Conference

Title
Workshop on nuclear astrophysics.
Dates
6-10 Jun 1983.
Place
Bad Wiessee (Germany, F.R.).

Optional Information

Secondary number(s)
CONF-8306114--1.