TY  - CONF
AU  - Göbel, K.
AU  - Glorius, J.
AU  - Koloczek, A.
AU  - Pignatari, M.
AU  - Plag, R.
AU  - Reifarth, R.
AU  - Ritter, C.
AU  - Schmidt, S.
AU  - Sonnabend, K.
AU  - Thomas, B.
AU  - Travaglio, C.
TI  - Online tools for nucleosynthesis studies
JO  - Journal of physics / Conference Series
VL  - 940
SN  - 1742-6596
CY  - Bristol
PB  - IOP Publ.
M1  - GSI-2018-00850
SP  - 012006
PY  - 2018
N1  - 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. 
AB  - 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.
T2  - Nuclear Physics in Astrophysics Conference
CY  - 18 May 2015 - 22 May 2015, York (Großbrittanien)
Y2  - 18 May 2015 - 22 May 2015
M2  - York, Großbrittanien
LB  - PUB:(DE-HGF)16 ; PUB:(DE-HGF)8
UR  - <Go to ISI:>//WOS:000431673700006
DO  - DOI:10.1088/1742-6596/940/1/012006
UR  - https://repository.gsi.de/record/213290
ER  -