Astronomy and Astrophysics – Astrophysics
Scientific paper
Mar 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000phrvl..84.2104r&link_type=abstract
Physical Review Letters, Volume 84, Issue 10, March 6, 2000, pp.2104-2107
Astronomy and Astrophysics
Astrophysics
12
Scientific paper
X-ray bursts have been suggested as a possible site for the astrophysical rp-process. The time scale for the process is governed by β-decay half-lives of several even-even N = Z waiting point nuclei, in particular, N = Z = 40 80Zr. A 4.1\(+0.8-0.6\)-s β+/EC half-life for 80Zr was determined by observing delayed 84-keV γ rays depopulating a T1/2 = 4-μs isomer at 312 keV in the daughter 80Y. 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.
Aprahamian Ani
Batchelder Jon C.
Bingham Carrol R.
Brenner Daeg S.
Ginter T. N.
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