EPJ Web Conf.
Volume 146, 2017ND 2016: International Conference on Nuclear Data for Science and Technology
|Number of page(s)||4|
|Section||Astro Nuclear Physics|
|Published online||13 September 2017|
Nuclear level densities and γ-ray strength functions of 180,181Ta and neutron capture cross sections
1 iThemba LABS, PO Box 722, Somerset West, 7129, South Africa
2 Physics Department, University of the Western Cape, Bellville 7535, South Africa
3 Physics Department, University of Stellenbosch, Matieland 7602, South Africa
4 Department of Physics, University of Oslo, 0316 Oslo, Norway
5 Lawrence Livermore National Laboratory, 7000 East Avenue, Livermore, CA 94550-9234, USA
6 Helmholtz Institute Mainz, 55099 Mainz, Germany
7 GSI Helmholtzzentrum für Schwerionenforschung, 64291 Darmstadt, Germany
Published online: 13 September 2017
The γ-ray strength functions and nuclear level densities in the quasi-continuum of 180,181Ta are extracted from particle-γ coincidence events with the Oslo Method, below the Sn. The data were used as input in the TALYS reaction code for calculations of the astrophysical Maxwellian-averaged (n,γ) cross-sections to investigate nucleosynthesis of nature's rarest stable isotope 180Ta.
© The Authors, published by EDP Sciences, 2017
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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