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arXiv · 0804.0223

Thermal Equilibration of 176-Lu via K-Mixing

Vadas Gintautas·Arthur E. Champagne·Filip G. Kondev·Richard Longland
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Abstract

In astrophysical environments, the long-lived (\T_1/2 = 37.6 Gy) ground state of 176-Lu can communicate with a short-lived (T_1/2 = 3.664 h) isomeric level through thermal excitations. Thus, the lifetime of 176-Lu in an astrophysical environment can be quite different than in the laboratory. We examine the possibility that the rate of equilibration can be enhanced via K-mixing of two levels near E_x = 725 keV and estimate the relevant gamma-decay rates. We use this result to illustrate the effect of K-mixing on the effective stellar half-life. We also present a network calculation that includes the equilibrating transitions allowed by K-mixing. Even a small amount of K-mixing will ensure that 176-Lu reaches at least a quasi-equilibrium during an s-process triggered by the 22-Ne neutron source.

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Vadas Gintautas, Arthur E. Champagne, Filip G. Kondev, Richard Longland. 2008-04-01. Thermal Equilibration of 176-Lu via K-Mixing. https://doi.org/10.1103/physrevc.80.015806

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