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Microscopic calculations of weak interaction rates of nuclei in stellar environment for A = 18 to 100

✍ Scribed by J.-U. Nabi; H.V. Klapdor-Kleingrothaus


Book ID
106259074
Publisher
Springer
Year
1999
Tongue
English
Weight
76 KB
Volume
5
Category
Article
ISSN
1434-601X

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Based on large-scale shell-model calculations we have determined the electron capture, positron capture and beta-decay rates for more than 100 nuclei in the mass range A = 45-65. The rates are given for densities ρY e = 10 7 -10 10 mol/cm 3 and temperatures T = 10 9 -10 10 K and hence are relevant f

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The weak interaction rates in stellar environments are computed for p f -shell nuclei in the mass range A = 45-65 using large-scale shell-model calculations. The calculated capture and decay rates take into consideration the latest experimental energy levels and log f t-values. The rates are tabulat