Cross-section measurements relevant for the astrophysical p process at the University of Cologne

The astrophysical p process unites all processes that have been introduced to explain the abundance of a group of 30 to 35 neutron-deficient nuclei which are referred to as p nuclei. In general, these p processes include large networks of nuclear reactions and a complete understanding of the individu...

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Bibliographic Details
Main Authors: Heim Felix, Müller Martin, Scholz Philipp, Wilden Svenja, Zilges Andreas
Format: Article
Language:English
Published: EDP Sciences 2022-01-01
Series:EPJ Web of Conferences
Online Access:https://www.epj-conferences.org/articles/epjconf/pdf/2022/04/epjconf_nic16th2022_11001.pdf