Nucleosynthesis in neutrino-driven supernovae

Fröhlich, C. and Hix, W. R. and Martinez-Pinedo, G. and Liebendörfer, M. and Thielemann, F. -K. and Bravo, E. and Langanke, K. and Zinner, N. T.. (2006) Nucleosynthesis in neutrino-driven supernovae. New astronomy reviews, Vol. 50. pp. 496-499.

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Official URL: http://edoc.unibas.ch/dok/A5253785

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Core collapse supernovae are the leading actor in the story of the cosmic origin of the chemical elements. Existing models, which generally assume spherical symmetry and parameterize the explosion, have been able to broadly replicate the observed elemental pattern. However, inclusion of neutrino interactions produces noticeable improvements in the iron peak composition of the ejecta when compared to observations. Neutrino interactions may also provide a supernova source for light p-process nuclei.
Faculties and Departments:05 Faculty of Science > Departement Physik > Former Organization Units Physics > Astrophysik (Liebendörfer)
05 Faculty of Science > Departement Physik > Former Organization Units Physics > Theoretische Physik Astrophysik (Thielemann)
UniBasel Contributors:Liebendörfer, Matthias and Fröhlich, Carla and Thielemann, Friedrich-Karl
Item Type:Article, refereed
Article Subtype:Research Article
Note:Publication type according to Uni Basel Research Database: Journal article
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Last Modified:22 Mar 2012 14:27
Deposited On:22 Mar 2012 13:56

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