Half-Life Measurement for the rp -Process Waiting Point Nuclide Z{sup 80}r
Journal Article
·
· Physical Review Letters
- Department of Chemistry, University of Maryland, College Park, Maryland 20742 (United States)
- Department of Physics, Louisiana State University, Baton Rouge, Louisiana 70803 (United States)
- Department of Physics, University of Notre Dame, Notre Dame, Indiana 46556 (United States)
- UNIRIB, Oak Ridge Associated Universities, Oak Ridge, Tennessee 37831 (United States)
- Department of Physics and Astronomy, University of Tennessee, Knoxville, Tennessee 37996 (United States)
- Department of Chemistry, Clark University, Worcester, Massachusetts 01610 (United States)
- Department of Physics and Astronomy, Vanderbilt University, Nashville, Tennessee 37235 (United States)
X-ray bursts have been suggested as a possible site for the astrophysical rp -process. The time scale for the process is governed by {beta} -decay half-lives of several even-even N=Z waiting point nuclei, in particular, N=Z=40 {sup 80}Zr . A 4.1(+0.8-0.6)- s {beta}{sup +}/EC half-life for {sup 80}Zr was determined by observing delayed 84-keV {gamma} rays depopulating a T{sub 1/2}=4-{mu}s isomer at 312 keV in the daughter {sup 80}Y . As this half-life is lower than many previously predicted values, the calculated excessive production of A=80 nuclides in astrophysical x-ray burst scenarios is reduced, and less extreme conditions are necessary for the production of heavier nuclides. (c) 2000 The American Physical Society.
- OSTI ID:
- 20215642
- Journal Information:
- Physical Review Letters, Journal Name: Physical Review Letters Journal Issue: 10 Vol. 84; ISSN 0031-9007; ISSN PRLTAO
- Country of Publication:
- United States
- Language:
- English
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