Abstract
The 12C+12C fusion reaction is one of the most important for nuclear astrophysics since it determines the carbon ignition in stellar environments. Two experiments which make use of the gamma-particle coincidence technique to measure the 12C+12C S-factors at deep sub barrier energies are discussed. Results are presented showing a decrease of the S-factor below Ec.m. = 3 MeV.
Original language | English |
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Title of host publication | Nuclear Physics in Astrophysics VIII, NPA8 2017 |
Publisher | EDP Sciences |
Number of pages | 6 |
Volume | 165 |
ISBN (Electronic) | 9782759890309 |
DOIs | |
Publication status | Published - 30 Dec 2017 |
Event | 8th International Conference on Nuclear Physics in Astrophysics, NPA8 2017 - Catania, Italy Duration: 18 Jun 2017 → 23 Jun 2017 |
Conference
Conference | 8th International Conference on Nuclear Physics in Astrophysics, NPA8 2017 |
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Country/Territory | Italy |
City | Catania |
Period | 18/06/17 → 23/06/17 |