The rates of the 18F(p,α) 15O and 18F(p,γ) 19Ne reactions in astrophysical environments depend on the properties of 19Ne levels above the 18F + p threshold. There are at least 8 levels in the mirror nucleus 19F for which analogs have not been observed in 19Ne in the excitation energy range E x = 6.4-7.6MeV. We have made a search for these levels by measuring the 1H( 18F, p) 18F excitation function over the energy range E c.m. = 0.3-1.3MeV. We have identified and measured the properties of a newly observed level at E x = 7.420±0.014MeV, which is most likely the mirror to the J π = 7/2+ 19F level at 7.56MeV. This new level is found to increase the calculated 18F(p,α) 15O reaction rate by 16%, 63%, and 106% at T = 1, 2, and 3GK, respectively
[Context] Direct observation of γ-ray emission from the decay of 18F ejected in classical nova outbu...
The 15O(α,γ)19Ne reaction is generally considered as a potential breakout reaction from the hot CNO ...
The investigation of the 19F(p, α0) reaction at low bombarding energies allows the study of the spec...
The rates of the F-18 (p, alpha)O-15 and F-18(p, gamma)Ne-19 reactions in astrophysical environments...
The rates of the F-18(p, alpha)O-15 and F-18(p, gamma) Ne-19 reactions in astrophysical environments...
Proton and alpha widths for a 3/2+ ( l p = 0) state in 19Ne at Ex-7.1 MeV have been extracted using ...
The main source of gamma ray emission from novae below 511 keV is likely to be associated with the β...
The degree to which the (p,gamma) and (p,alpha) reactions destroy 18F at temperatures 1-4x10^8 K is ...
International audienceThe main source of gamma ray emission from novae below 511 keV is likely to be...
The nuclear structure of 19Ne near the proton threshold is of interest for understanding the rates o...
Uncertainties in the thermonuclear rates of the O15(a,¿)19Ne and 18F(p,a)15O reactions affect model ...
The observational 19F abundance in stellar environments systematically exceeds the predicted one, th...
Background: Classical novae result from thermonuclear explosions producing several γ-ray emitters wh...
The degree to which the (p, gamma) and (p, alpha) reactions destroy F-18 at temperatures (1-4) x 10(...
The early E < 511 keV gamma-ray emission from novae depends critically on the 18F(p,a)15O reaction. ...
[Context] Direct observation of γ-ray emission from the decay of 18F ejected in classical nova outbu...
The 15O(α,γ)19Ne reaction is generally considered as a potential breakout reaction from the hot CNO ...
The investigation of the 19F(p, α0) reaction at low bombarding energies allows the study of the spec...
The rates of the F-18 (p, alpha)O-15 and F-18(p, gamma)Ne-19 reactions in astrophysical environments...
The rates of the F-18(p, alpha)O-15 and F-18(p, gamma) Ne-19 reactions in astrophysical environments...
Proton and alpha widths for a 3/2+ ( l p = 0) state in 19Ne at Ex-7.1 MeV have been extracted using ...
The main source of gamma ray emission from novae below 511 keV is likely to be associated with the β...
The degree to which the (p,gamma) and (p,alpha) reactions destroy 18F at temperatures 1-4x10^8 K is ...
International audienceThe main source of gamma ray emission from novae below 511 keV is likely to be...
The nuclear structure of 19Ne near the proton threshold is of interest for understanding the rates o...
Uncertainties in the thermonuclear rates of the O15(a,¿)19Ne and 18F(p,a)15O reactions affect model ...
The observational 19F abundance in stellar environments systematically exceeds the predicted one, th...
Background: Classical novae result from thermonuclear explosions producing several γ-ray emitters wh...
The degree to which the (p, gamma) and (p, alpha) reactions destroy F-18 at temperatures (1-4) x 10(...
The early E < 511 keV gamma-ray emission from novae depends critically on the 18F(p,a)15O reaction. ...
[Context] Direct observation of γ-ray emission from the decay of 18F ejected in classical nova outbu...
The 15O(α,γ)19Ne reaction is generally considered as a potential breakout reaction from the hot CNO ...
The investigation of the 19F(p, α0) reaction at low bombarding energies allows the study of the spec...