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| 100 | 1 | _ | |a Göbel, K. |0 P:(DE-HGF)0 |b 0 |e Corresponding author |
| 111 | 2 | _ | |a Nuclear Physics in Astrophysics Conference |g NPA VII |c York |d 2015-05-18 - 2015-05-22 |w Großbrittanien |
| 245 | _ | _ | |a Online tools for nucleosynthesis studies |
| 260 | _ | _ | |a Bristol |c 2018 |b IOP Publ. |
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| 500 | _ | _ | |a Content from this work may be used under the terms of the Creative Commons Attribution 3.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI. |
| 520 | _ | _ | |a The nucleosynthesis of the elements between iron and uranium involves many different astrophysical scenarios covering wide ranges of temperatures and densities. Thousands of nuclei and ten thousands of reaction rates have to be included in the corresponding simulations. We investigate the impact of single rates on the predicted abundance distributions with post-processing nucleosynthesis simulations. We present online tools, which allow the investigation of sensitivities and integrated mass fluxes in different astrophysical scenarios. |
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