$^{180}$Ta production in the classical s-process

Details $^{180}$Ta production in the classical s-process $^{180}$Ta production in the classical s-process

2002-07-04

arxiv.org/abs/astro-ph/0207123v2

Astronomy and Astrophysics

Astrophysics

4 pages, 4 figures

Scientific paper

The production and survival of the quasistable isomer $^{180}$Ta during the
stellar nucleosynthesis has remained a matter of discussion for years. A
careful analysis of the available experimental data and theoretical
calculations enabled us to reproduce the observed solar abundance of $^{180}$Ta
in the classical s-process ($kT=28$ keV -- 33 keV).

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