出版社:SISSA, Scuola Internazionale Superiore di Studi Avanzati
摘要:The 18F nucleus is one of the radioactive isotopes produced during nova explosions. It is of
particular interest since it is mainly responsible for the 511 keV gamma-ray emission of novae
that could be detected with the INTEGRAL satellite or future gamma-ray telescopes. The amount
of 18F synthesised still suffers from large uncertainties coming from missing nuclear information
concerning the 18F destruction reaction 18F(p,a)15O. In particular, the interference sign between
three 3/2+ resonances in 19Ne, situated slightly above the proton threshold (8 keV and/or 38
keV) and at higher energy (665 keV), is unknown. The maximum effect of these interferences is
lying in the energy range corresponding to the Gamow peak region and has a strong impact on
the 18F(p,a)15O reaction rate. We report here on the direct measurement at low energy (down
to 400 keV in the center-of-mass) of the 18F(p,a)15O total cross section that we performed at
the Louvain-la-Neuve CRC-RIB facility with the high-intensity and -purity 18F radioactive beam
(T1/2 = 110 min). The total cross section for the different incident energies will be presented and
compared to previous experimental data.