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.

Details

Title
Online tools for nucleosynthesis studies
Author
Göbel, K 1 ; Glorius, J 2 ; Koloczek, A 1 ; Pignatari, M 3 ; Plag, R 4 ; Reifarth, R 1 ; Ritter, C 5 ; Schmidt, S 6 ; Sonnabend, K 6 ; Thomas, B 6 ; Travaglio, C 7 

 Goethe University Frankfurt, Germany; http://www.nugridstars.org 
 Goethe University Frankfurt, Germany; GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt, Germany 
 http://www.nugridstars.org; Konkoly Observatory of the Hungarian Academy of Sciences, Hungary 
 GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt, Germany 
 Goethe University Frankfurt, Germany; http://www.nugridstars.org; University of Victoria, Canada 
 Goethe University Frankfurt, Germany 
 INAF - Astrophysical Observatory Turin, Italy 
Publication year
2018
Publication date
Jan 2018
Publisher
IOP Publishing
ISSN
17426588
e-ISSN
17426596
Source type
Scholarly Journal
Language of publication
English
ProQuest document ID
2571919503
Copyright
© 2018. This work is published under http://creativecommons.org/licenses/by/3.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.