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PURE Aarhus University
Conference object . 2006
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https://dx.doi.org/10.48550/ar...
Article . 2005
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Nucleosynthesis in neutrino-driven supernovae

Authors: Froehlich, C; Hix, W R; Martínez, G; Liebendoerfer, M; Thielemann, F K; Bravo Guil, Eduardo; Langanke, K; +1 Authors

Nucleosynthesis in neutrino-driven supernovae

Abstract

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 improvement in the composition of the ejecta when compared to observations. Neutrino interactions may also provide a supernova source for light p-process nuclei.

7 pages, 2 figures, in proceedings of Astronomy with Radioactivities V, Clemson University, September 5-9, 2005, to appear in New Astronomy Reviews

Countries
Spain, Switzerland
Keywords

Supernovae, Supernoves, Astrophysics (astro-ph), FOS: Physical sciences, Àrees temàtiques de la UPC::Física::Astronomia i astrofísica, Astrophysics

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selected citations
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This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
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21
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