Inhomogeneous chemical evolution of r-process elements Article Swipe
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Benjamin Wehmeyer
,
M. Pignatari
,
F.‐K. Thielemann
·
YOU?
·
· 2016
· Open Access
·
· DOI: https://doi.org/10.1063/1.4953301
· OA: W2464572014
YOU?
·
· 2016
· Open Access
·
· DOI: https://doi.org/10.1063/1.4953301
· OA: W2464572014
We report the results of a galactic chemical evolution (GCE) study for r-process- and alpha elements. For this work, we used the inhomogeneous GCE model "ICE", which allows to keep track of the galactic abundances of elements produced by different astrophysical sites. The main input parameters for this study were: a) The Neutron Star Merger (NSM) coalescence time scale, the probability of NSMs, and for the sub-class of "magneto-rotationally driven Supernovae" ("Jet-SNe"), their occurence rate in comparison to "standard" Supernovae (SNe).
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