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@INPROCEEDINGS{Gbel:213290,
author = {Göbel, K. and Glorius, J. and Koloczek, A. and Pignatari,
M. and Plag, R. and Reifarth, R. and Ritter, C. and Schmidt,
S. and Sonnabend, K. and Thomas, B. and Travaglio, C.},
title = {{O}nline tools for nucleosynthesis studies},
journal = {Journal of physics / Conference Series},
volume = {940},
issn = {1742-6596},
address = {Bristol},
publisher = {IOP Publ.},
reportid = {GSI-2018-00850},
pages = {012006},
year = {2018},
note = {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.},
abstract = {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.},
month = {May},
date = {2015-05-18},
organization = {Nuclear Physics in Astrophysics
Conference, York (Großbrittanien), 18
May 2015 - 22 May 2015},
cin = {ATP / KRA},
ddc = {530},
cid = {I:(DE-Ds200)ATP-20051214OR020 /
I:(DE-Ds200)KRA-20150901OR349},
pnm = {6211 - Extreme States of Matter: From Cold Ions to Hot
Plasmas (POF3-621) / HGF-IVF-VH-GS-201 - HGS-HIRe :
(HGF-IVF-VH-GS-201)},
pid = {G:(DE-HGF)POF3-6211 / G:(DE-Ds200)HGF-IVF-VH-GS-201},
typ = {PUB:(DE-HGF)16 / PUB:(DE-HGF)8},
UT = {WOS:000431673700006},
doi = {10.1088/1742-6596/940/1/012006},
url = {https://repository.gsi.de/record/213290},
}