18 pages, 8 figures. Accepted in Nuclear Physics AThe early E $\leq$ 511 keV gamma-ray emission from novae depends critically on the $^{18}$F(p,$\alpha$)$^{15}$O reaction. Unfortunately the reaction rate of the $^{18}$F(p,$\alpha$)$^{15}$O reaction is still largely uncertain due to the unknown strengths of low-lying proton resonances near the $^{18}$F+p threshold which play an important role in the nova temperature regime. We report here our last results concerning the study of the d($^{18}$F,p)$^{19}$F($\alpha$)$^{15}$N transfer reaction. We show in particular that these two low-lying resonances cannot be neglected. These results are then used to perform a careful study of the remaining uncertainties associated to the $^{18}$F(p,$\alpha$)$...
International audienceClassical novae result from thermonuclear explosions producing several $\gamma...
The 18F(p,alpha)15O reaction is recognized to be one of the most important reactions for nova gamma-...
The 18F(p,$\alpha$) reaction determines the rate of destruction of 18F in novae. It represents the k...
18 pages, 8 figures. Accepted in Nuclear Physics AThe early E $\leq$ 511 keV gamma-ray emission from...
The early E < 511 keV gamma-ray emission from novae depends critically on the 18F(p,a)15O reaction. ...
The early E < 511 keV gamma-ray emission from novae depends critically on the 18F(p,a)15O reaction. ...
The degree to which the (p,gamma) and (p,alpha) reactions destroy 18F at temperatures 1-4x10^8 K is ...
Contribution to the Eighth International Symposium on Nuclei in the Cosmos, Vancouver july 19-23. 4 ...
The degree to which the (p, gamma) and (p, alpha) reactions destroy F-18 at temperatures (1-4) x 10(...
Context. Direct observation of ¿-ray emission from the decay of 18F ejected in classical nova outbur...
7 pages, 4 figures, 2 tables, expérience GANIL/SPIRALThe most intense gamma-ray line observable from...
[Context] Direct observation of γ-ray emission from the decay of 18F ejected in classical nova outbu...
The gamma-ray emission of novae at and below 511 keV is mainly due to the positron annihilation comi...
Uncertainties in the thermonuclear rates of the O15(a,¿)19Ne and 18F(p,a)15O reactions affect model ...
The 18F(p,α)15O reaction is the predominant destruction mechanism in novae of the radionuclide F18, ...
International audienceClassical novae result from thermonuclear explosions producing several $\gamma...
The 18F(p,alpha)15O reaction is recognized to be one of the most important reactions for nova gamma-...
The 18F(p,$\alpha$) reaction determines the rate of destruction of 18F in novae. It represents the k...
18 pages, 8 figures. Accepted in Nuclear Physics AThe early E $\leq$ 511 keV gamma-ray emission from...
The early E < 511 keV gamma-ray emission from novae depends critically on the 18F(p,a)15O reaction. ...
The early E < 511 keV gamma-ray emission from novae depends critically on the 18F(p,a)15O reaction. ...
The degree to which the (p,gamma) and (p,alpha) reactions destroy 18F at temperatures 1-4x10^8 K is ...
Contribution to the Eighth International Symposium on Nuclei in the Cosmos, Vancouver july 19-23. 4 ...
The degree to which the (p, gamma) and (p, alpha) reactions destroy F-18 at temperatures (1-4) x 10(...
Context. Direct observation of ¿-ray emission from the decay of 18F ejected in classical nova outbur...
7 pages, 4 figures, 2 tables, expérience GANIL/SPIRALThe most intense gamma-ray line observable from...
[Context] Direct observation of γ-ray emission from the decay of 18F ejected in classical nova outbu...
The gamma-ray emission of novae at and below 511 keV is mainly due to the positron annihilation comi...
Uncertainties in the thermonuclear rates of the O15(a,¿)19Ne and 18F(p,a)15O reactions affect model ...
The 18F(p,α)15O reaction is the predominant destruction mechanism in novae of the radionuclide F18, ...
International audienceClassical novae result from thermonuclear explosions producing several $\gamma...
The 18F(p,alpha)15O reaction is recognized to be one of the most important reactions for nova gamma-...
The 18F(p,$\alpha$) reaction determines the rate of destruction of 18F in novae. It represents the k...