Inhomogeneous chemical evolution of r-process elements

Wehmeyer, B. and Pignatari, M. and Thielemann, F.-K.. (2016) Inhomogeneous chemical evolution of r-process elements. In: AIP Conference Proceedings, 1743. 040009.

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Official URL: http://edoc.unibas.ch/53856/

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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).
Faculties and Departments:05 Faculty of Science > Departement Physik > Former Organization Units Physics > Theoretische Physik Astrophysik (Thielemann)
UniBasel Contributors:Thielemann, Friedrich-Karl and Wehmeyer, Benjamin
Item Type:Conference or Workshop Item
Conference or workshop item Subtype:Conference Paper
Publisher:AIP Publishing
Note:Publication type according to Uni Basel Research Database: Conference paper
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Last Modified:15 Mar 2017 12:41
Deposited On:15 Mar 2017 12:40

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