Research output per year
Research output per year
The neutrino-induced nucleosynthesis (v process) in supernova explosions of massive stars of solar metallicity with initial main sequence masses between 15 and 40 M 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 v 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 v 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 | Journal of Physics: Conference Series |
Subtitle of host publication | 7th Nuclear Physics in Astrophysics Conference, NPA 2015; York; United Kingdom; 18 May 2015 through 22 May 2015 |
Number of pages | 4 |
Volume | 940 |
Edition | 1 |
DOIs | |
Publication status | Published - 31 Jan 2018 |
Event | Nuclear Physics in Astrophysics Conference (NPA) 2015 - The Royal York hotel, York, United Kingdom Duration: 18 May 2015 → 22 May 2015 Conference number: 7th http://iopscience.iop.org/article/10.1088/1742-6596/940/1/011001/pdf (Preface) http://iopscience.iop.org/article/10.1088/1742-6596/940/1/011002/pdf (Staement of peer review) |
Name | Journal of Physics: Conference Series |
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Publisher | IOP Publishing |
ISSN (Print) | 1742-6588 |
Conference | Nuclear Physics in Astrophysics Conference (NPA) 2015 |
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Abbreviated title | NPA 2015 |
Country/Territory | United Kingdom |
City | York |
Period | 18/05/15 → 22/05/15 |
Internet address |
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Research output: Chapter in Book/Report/Conference proceeding › Conference Paper › Research › peer-review