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The neutrino-induced nucleosynthesis (ν process) in supernova explosions of massive stars of solar metallicity with initial main sequence masses between 15 and 40 MȮ has been studied. A new extensive set of neutrino-nucleus cross-sections for all the nuclei included in the reaction network is used and the average neutrino energies are reduced to agree with modern supernova simulations. Despite these changes the ν process is found to contribute still significantly to the production of the nuclei 7Li, 11B, 19F, 138La and 180Ta, even though the total yields for those nuclei are reduced. Furthermore we study in detail contributions of the ν process to the production of radioactive isotopes 26Al, 22Na and confirm the production of 92Nb and 98Tc.
Original language | English |
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Title of host publication | EPJ Web of Conferences |
Subtitle of host publication | 13th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG 2015; Beijing; China; 24 June 2015 through 27 June 2015; Code 119590 |
Editors | W P Liu, Z H Li, Y B Wang, B Guo, Y P Shen |
Place of Publication | Les Ulis France |
Publisher | EDP Sciences |
Number of pages | 6 |
Volume | 109 |
DOIs | |
Publication status | Published - 12 Feb 2016 |
Event | International Symposium on Origin of Matter and Evolution of Galaxies (OMEG) 2015 - Prime Hotel, Beijing, China Duration: 24 Jun 2015 → 27 Jun 2015 Conference number: 13th http://esic.ciae.ac.cn/omeg2015/ http://inspirehep.net/record/1409580 |
Name | EPJ Web of Conferences |
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Publisher | EDP Sciences |
ISSN (Print) | 2101-6275 |
Conference | International Symposium on Origin of Matter and Evolution of Galaxies (OMEG) 2015 |
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Abbreviated title | OMEG 2015 |
Country/Territory | China |
City | Beijing |
Period | 24/06/15 → 27/06/15 |
Internet address |
Research output: Chapter in Book/Report/Conference proceeding › Conference Paper › Other › peer-review