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Publikováno v:
EPJ Web of Conferences. 260:11001
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 re
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::58344d3f6db65b57c1f958e83cad66c6
https://doi.org/10.1051/epjconf/202226011001
https://doi.org/10.1051/epjconf/202226011001
