The 18F(p,α)15O reaction plays a crucial role in understanding γ-ray emission from novae. Because of the importance of understanding the 18F + p reactions, a number of studies of the A=19 isobars have been made using stable and exotic beams. The interference effects among J π = 3/2+ resonances in the 18F + p system, however, have never been measured, but they can change the S-factor by a factor of 20 at nova energies. R-matrix calculations indicate that the cross sections above the Ec.m. = 665 keV resonance are sensitive to the interference between the Ec.m. = 8, 38, and 665 keV resonances. In order to study the interference effects, an excitation function for the 1H(18F,α)15O reaction has been measured in the energy range of Ec.m. = 663-87...
The 18F nucleus is one of the radioactive isotopes produced during nova explosions. It is of particu...
Gamma ray astronomy has made big strides in the last decades paving the way to a better understandin...
The astrophysical 18F(p,α)15O rate determines, in large part, the extent to which the observable rad...
The F18(p,α)O15 reaction rate is crucial for constraining model predictions of the γ-ray observable ...
Detection of nuclear-decay γ rays provides a sensitive thermometer of nova nucleosynthesis. The most...
A direct test of nova explosion models comes from the observation of γ rays created in the decay of ...
The 18F(p,α)15O reaction is the predominant destruction mechanism in novae of the radionuclide F18, ...
The detection of γ-rays from explosive astrophysical scenarios such as novae provides an excellent ...
The $^{18}$F(p, $\alpha$)$^{15}$O reaction is key to determining the $^{18}$F abundance in classical...
The rate of destruction of 18F via the 18F + p reactions is of importance in both novae and X-ray b...
A recently discovered resonance at 193 keV determines the thermonuclear rates of the O17 +p reaction...
The experiment was performed at the Centre de Recherches du Cyclotron at Louvain-la-Neuve (Belgium) ...
The main source of gamma ray emission from novae below 511 keV is likely to be associated with the β...
Knowledge of the astrophysical rate of the 18F(p,α)15O reaction is important for understanding the γ...
Proton and alpha widths for a 3/2+ ( l p = 0) state in 19Ne at Ex-7.1 MeV have been extracted using ...
The 18F nucleus is one of the radioactive isotopes produced during nova explosions. It is of particu...
Gamma ray astronomy has made big strides in the last decades paving the way to a better understandin...
The astrophysical 18F(p,α)15O rate determines, in large part, the extent to which the observable rad...
The F18(p,α)O15 reaction rate is crucial for constraining model predictions of the γ-ray observable ...
Detection of nuclear-decay γ rays provides a sensitive thermometer of nova nucleosynthesis. The most...
A direct test of nova explosion models comes from the observation of γ rays created in the decay of ...
The 18F(p,α)15O reaction is the predominant destruction mechanism in novae of the radionuclide F18, ...
The detection of γ-rays from explosive astrophysical scenarios such as novae provides an excellent ...
The $^{18}$F(p, $\alpha$)$^{15}$O reaction is key to determining the $^{18}$F abundance in classical...
The rate of destruction of 18F via the 18F + p reactions is of importance in both novae and X-ray b...
A recently discovered resonance at 193 keV determines the thermonuclear rates of the O17 +p reaction...
The experiment was performed at the Centre de Recherches du Cyclotron at Louvain-la-Neuve (Belgium) ...
The main source of gamma ray emission from novae below 511 keV is likely to be associated with the β...
Knowledge of the astrophysical rate of the 18F(p,α)15O reaction is important for understanding the γ...
Proton and alpha widths for a 3/2+ ( l p = 0) state in 19Ne at Ex-7.1 MeV have been extracted using ...
The 18F nucleus is one of the radioactive isotopes produced during nova explosions. It is of particu...
Gamma ray astronomy has made big strides in the last decades paving the way to a better understandin...
The astrophysical 18F(p,α)15O rate determines, in large part, the extent to which the observable rad...